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Rogers RR, Williams TD, Nester EB, Owens GM, Ballmann CG. The Influence of Music Preference on Countermovement Jump and Maximal Isometric Performance in Active Females. J Funct Morphol Kinesiol 2023; 8:jfmk8010034. [PMID: 36976131 PMCID: PMC10051532 DOI: 10.3390/jfmk8010034] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 02/06/2023] [Revised: 03/09/2023] [Accepted: 03/10/2023] [Indexed: 03/29/2023] Open
Abstract
Previous studies have shown that listening to preferred music during resistance and endurance exercises improves performance. However, it is unknown if these phenomena translate to short-duration explosive exercises. The purpose of this study was to investigate the influences of preferred and non-preferred music on countermovement jump (CMJ) performance, isometric mid-thigh pull (IMTP), and psychological responses to music during explosive movements. Physically active females (age 18-25) volunteered to take part in the study. In a counterbalanced, crossover design, participants completed three trials: (1) no music (NM), (2) non-preferred (NP), and (3) preferred (PV) music. Participants completed three maximal IMTP tests on a force-plate-equipped IMTP apparatus with an immovable bar. Attempts lasted 5 s and were separated by 3 min of rest. Furthermore, participants completed three single maximal CMJ attempts separated by 3 min of rest on force plates. All attempts were averaged for analysis. At the commencement of IMTP and CMJ testing, participants were asked to rate how motivated and psyched up they felt during the exercise portion using a visual analog scale. For isometric performance, listening to PM resulted in increased peak force (p = 0.039; d = 0.41) and rate of force development at 200 ms (p = 0.023; d = 0.91) compared with NP. For CMJ, there were no differences between conditions for jump height (p = 0.912; η2 = 0.007) or peak power during the propulsive phase (p = 0.460; η2 = 0.003). Levels of motivation were significantly higher with PM compared with NM (p < 0.001; d = 2.3) and NP (p = 0.001; d = 2.0). Feelings of being psyched up were significantly higher with PM compared with NM (p < 0.001; d = 4.2) and NP (p = 0.001; d = 2.8). Findings suggest that preferred music enhances isometric strength and increases motivation and feelings of being psyched up. Thus, PM may be used as an ergogenic aid during short-duration maximal-effort activities.
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Affiliation(s)
- Rebecca R Rogers
- Center for Engagement in Disability Health and Rehabilitation Sciences (CEDHARS), School of Health Professions, University of Alabama at Birmingham, 3810 Ridgeway, Birmingham, AL 35209, USA
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
| | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
| | - Emma B Nester
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
| | - Grace M Owens
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
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Benjamin CL, Dobbins LW, Sullivan SG, Rogers RR, Williams TD, Marshall MR, Ballmann CG. The Effect of Fluid Availability on Consumption and Perceptual Measures during Aerobic Exercise. Int J Environ Res Public Health 2023; 20:1310. [PMID: 36674064 PMCID: PMC9858706 DOI: 10.3390/ijerph20021310] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 11/22/2022] [Revised: 01/05/2023] [Accepted: 01/06/2023] [Indexed: 06/17/2023]
Abstract
Fluid availability may alter drinking behavior; however, it is currently unknown if the availability of fluid impacts behavior and gastrointestinal issues (GI) that are often associated with increased fluid intake. The purpose of this study was to determine if ad libitum (AL) versus periodic (PER) fluid intake influences fluid consumption and GI distress during exercise in trained athletes. Male and female Division I NCAA Cross Country athletes (n = 11; age = 20 ± 1 years) participated in this counterbalanced crossover study. Each participant completed a moderate intensity 10 km run on two separate occasions. In one trial, participants had unlimited availability to fluid to consume AL. In the other trial, participants consumed PER fluid at stations placed every 3.2 km. Assurance of euhydration prior to each trial was confirmed via urine specific gravity (USG) and urine color. Subjective perceptions of thirst and gastric fullness were assessed pre- and post-exercise via Likert questioning and a visual analog scale, respectively. Participants started each trial euhydrated (AL = 1.009 USG ± 0.009; PER = 1.009 USG ± 0.009; urine color AL, 3 ± 1; urine color PER, 2 ± 1). Fluid volume consumption was significantly higher during the AL condition compared to PER (p = 0.050). Thirst significantly increased from pre- to post-run regardless of treatment (p < 0.001); however, there was no significant difference between the groups (p = 0.492). Feelings of fullness did not change pre-post trial (p = 0.304) or between trials (p = 0.958). Increased fluid availability allows for increased fluid consumption without the negative experience of GI discomfort.
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Affiliation(s)
| | - Luke W. Dobbins
- Department of Kinesiology, Samford University, Birmingham, AL 35226, USA
| | | | - Rebecca R. Rogers
- Department of Kinesiology, Samford University, Birmingham, AL 35226, USA
- SHP Research Collaborative, University of Alabama at Birmingham, Birmingham, AL 35226, USA
| | - Tyler D. Williams
- Department of Kinesiology, Samford University, Birmingham, AL 35226, USA
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Lownie TJR, Jubinville I, Williams TD, Phillips RA, Crossin GT. Varying aerobic capacity in relation to breeding stage and reproductive success in giant petrels (Macronectes spp.). Comp Biochem Physiol A Mol Integr Physiol 2022; 266:111155. [PMID: 35051629 DOI: 10.1016/j.cbpa.2022.111155] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/16/2021] [Revised: 01/11/2022] [Accepted: 01/12/2022] [Indexed: 11/16/2022]
Abstract
Reproduction, and parental care in particular, are among the most energy-demanding activities within the annual cycle of adult birds. Parents that cannot meet the metabolic demands and other physiological costs of raising offspring may opt to abandon chicks in favour of self-maintenance and future reproduction. Recent work examining reproductive trade-offs in birds revealed an important role of oxygen carrying capacity in mediating variation in parental effort. This study explores the aerobic factors underlying the success or failure of parental care in two closely-related petrel species during their breeding season on Bird Island, South Georgia: northern giant petrels (Macronectes halli) and southern giant petrels (M. giganteus). Failed breeders of both sexes and species had significantly lower hematocrit levels (by 5.48 ± 0.64%) than successful breeders, and reticulocyte counts also tended to be lower in failed males, consistent with the hypothesis that parental care and workload depend on aerobic capacity. We discuss these results in relation to differences in the foraging ecology of both species and sexes.
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Affiliation(s)
- T J R Lownie
- Department of Biology, Dalhousie University, Halifax, Nova Scotia B3H 4R2, Canada.
| | - I Jubinville
- Department of Biology, Dalhousie University, Halifax, Nova Scotia B3H 4R2, Canada
| | - T D Williams
- Department of Biological Sciences, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada
| | - R A Phillips
- British Antarctic Survey, National Environment Research Council, High Cross, Madingley Road, Cambridge CB3 0ET, UK
| | - G T Crossin
- Department of Biology, Dalhousie University, Halifax, Nova Scotia B3H 4R2, Canada.
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Lehman JT, Whitmire BG, Rogers RR, Williams TD, Ballmann CG. Effects of Respite Music on Repeated Upper-body Resistance Exercise Performance. Int J Exerc Sci 2022; 15:79-87. [PMID: 36896024 PMCID: PMC9987432] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Subscribe] [Scholar Register] [Indexed: 03/11/2023]
Abstract
The purpose of this study was to investigate the effects of self-selected respite music on upper-body resistance exercise performance. In a crossover, counterbalanced study design, resistance-trained males (n = 10) participated in two bench press trials each with a different condition: 1) No music (NM), 2) Listening to respite music (RM; i.e. during rest periods). Following a warm-up, participants completed 3 sets × repetitions to failure (RTF) at 75% of 1-RM separated by 2 minutes of rest. During the 2-minute rest, participants either listened to NM or RM until the next subsequent set. A linear position transducer was used to measure mean barbell velocity during the first 3 repetitions and averaged for analysis. Rate of perceived exertion (RPE) and motivation were obtained after each set. Results indicate that mean velocity was higher during set 2 (p = 0.009; d = 1.34) and set 3 (p = 0.048; d = 0.95) while listening to RM versus NM. Furthermore, motivation was significantly higher following set 2 (p = 0.005; d = 1.15) and set 3 (p < 0.001; d = 1.79) while listening to RM compared to NM. No changes in RTF or RPE were noted between conditions (p > 0.05). These findings indicate listening to music during recovery may enhance subsequent explosive resistance performance and suggest that listening to music in between bouts of maximal effort could be an effective tool for optimizing performance during competition or training.
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Affiliation(s)
| | | | - Rebecca R Rogers
- Department of Kinesiology, Samford University, Birmingham, AL, USA
| | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, AL, USA
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Benjamin CL, Norton EP, Shirley BM, Rogers RR, Williams TD, Marshall MR, Ballmann CG. Fluid Restriction Negatively Influences Perceived Morning Alertness and Visuomotor Ability. Int J Environ Res Public Health 2021; 19:370. [PMID: 35010630 PMCID: PMC8745019 DOI: 10.3390/ijerph19010370] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 11/14/2021] [Revised: 12/27/2021] [Accepted: 12/28/2021] [Indexed: 06/14/2023]
Abstract
The purpose of this study was to assess the effect of two fluid intake protocols on alertness and reaction time before and after fluid intake. Healthy college-age males (n = 12) followed two fluid intake protocols on separate occasions: (1) prescribed fluid (PF) and fluid restricted (FR). In PF, participants were instructed to consume 500 mL of fluid the night prior to and the morning of data collection. In FR, participants were instructed to refrain from the consumption of fluid for 12 h. To assess hydration status, urine specific gravity and urine color were measured. Participants perceived level of thirst and alertness were also recorded. Participants then completed visuomotor reaction time tests using the Dynavision LED board, using both a central visuomotor test and a peripheral visuomotor test (PVRT) prior to (1) and following (2) the ingestion of 100 mL of water. Participants displayed significantly improved PVRT in PF state as compared to FR (PF1 = 1.13 ± 0.16, PF2 = 1.04 ± 0.14; FR1 = 1.27 ± 0.27, FR2 = 1.18 ± 0.20; p = 0.038, ηp2 = 0.363). Both CVRT and PVRT improved over time, following the ingestion of 100 mL of fluid. Participants in the PF state were also significantly more alert than participants in the FR state (PF = 4 ± 2, FR = 5 ± 2; p = 0.019, ES = 0.839). Collectively, perceived alertness and PVRT were negatively impacted by FR.
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Blazer HJ, Jordan CL, Pederson JA, Rogers RR, Williams TD, Marshall MR, Ballmann CG. Effects of Time-of-Day Training Preference on Resistance-Exercise Performance. Res Q Exerc Sport 2021; 92:492-499. [PMID: 32633217 DOI: 10.1080/02701367.2020.1751032] [Citation(s) in RCA: 4] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/15/2020] [Accepted: 03/31/2020] [Indexed: 06/11/2023]
Abstract
Purpose: The purpose of this study was to investigate how time-of-day training preference influences resistance-exercise performance. Methods: Resistance trained males (n = 12) were recruited for this study. In a crossover, counterbalanced design, participants completed two separate bench-press exercise trials at different times of day: (a) morning (AM; 8:00 hr) and (b) evening (PM; 16:00 hr). Participants answered a questionnaire on time-of-day training preference and completed a preferred (PREF) and nonpreferred (NON-PREF) time-of-day trial. For each trial, motivation was measured using a visual analog scale prior to exercise. Participants completed 2 sets × 2 repetitions at 75% 1-RM with maximum explosiveness separated by 5 min of rest. Mean barbell velocity was measured using a linear position transducer. Participants then completed 1 set × repetitions to failure (RTF) at 75% 1-RM. Rate of perceived exertion (RPE) was measured immediately following exercise. Results: Regardless of preference, velocity (p = .025; effect size (ES) = 0.43) was higher during the PM versus AM trial. However, there were no significant differences in velocity (p = .368; ES = 0.37) between PREF and NON-PREF time of day. There were no significant differences for repetitions between PREF and NON-PREF times (p = .902; ES = 0.03). Motivation was higher in the PREF time versus NON-PREF (p = .015; ES = 0.68). Furthermore, RPE was significantly lower during the PREF time of day (p = .048; 0.55). Conclusions: Despite higher barbell velocity collectively at PM times, time-of-training preference did not largely influence resistance-exercise performance, while motivation is higher and RPE is lower during preferred times.
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Meglic CE, Orman CM, Rogers RR, Williams TD, Ballmann CG. Influence of Warm-Up Music Preference on Anaerobic Exercise Performance in Division I NCAA Female Athletes. J Funct Morphol Kinesiol 2021; 6:jfmk6030064. [PMID: 34449658 PMCID: PMC8395765 DOI: 10.3390/jfmk6030064] [Citation(s) in RCA: 5] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 06/27/2021] [Revised: 07/16/2021] [Accepted: 07/16/2021] [Indexed: 11/16/2022] Open
Abstract
The purpose of this study was to investigate the effects of listening to preferred versus non-preferred warm-up music on anaerobic sprint performance in Division I NCAA female athletes. Female collegiate athletes (n = 14) were recruited for this study. In a counterbalanced, crossover study design, participants completed two separate visits, each with a different warm-up music condition: preferred (Pref) or non-preferred (Non-pref). During each visit, participants completed a 3 min standardized cycling warm-up at 50 Watts while listening to Pref or Non-pref music. Following this, participants completed 3 × 15 s Wingate Anaerobic Tests (WAnTs) with a 2 min active recovery period in between tests. Motivation to exercise was measured immediately following the warm-up (WU), WAnT1, WAnT2, and WAnT3. The rate of perceived exertion (RPE) was also measured after each WAnT. Each visit was separated by a minimal recovery period of 48 h. Mean power, total work, RPE, and motivation were analyzed. Mean power (p = 0.044; d = 0.91) and total work (p = 0.045; d = 0.78) were significantly higher during the Pref music condition versus Non-pref. RPE remained unchanged regardless of condition (p = 0.536; d = 0.01). Motivation was significantly higher with Pref warm-up music compared to Non-pref (p < 0.001; d = 1.55). These results show that listening to Pref warm-up music has an ergogenic benefit during repeated sprints in comparison to Non-pref music and improves motivation to exercise. Listening to warm-up music prior to high-intensity repeated exercise may aid in optimizing performance and training in collegiate athletes.
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Ballmann CG, McCullum MJ, Rogers RR, Marshall MR, Williams TD. Effects of Preferred vs. Nonpreferred Music on Resistance Exercise Performance. J Strength Cond Res 2021; 35:1650-1655. [PMID: 30531416 DOI: 10.1519/jsc.0000000000002981] [Citation(s) in RCA: 26] [Impact Index Per Article: 8.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
Abstract
ABSTRACT Ballmann, CG, McCullum, MJ, Rogers, RR, Marshall, MR , and Williams, TD. Effects of preferred vs. nonpreferred music on resistance exercise performance. J Strength Cond Res 35(6): 1650-1655, 2021-The purpose of this study was to examine the effects of listening to preferred vs. nonpreferred music on resistance exercise performance. Twelve resistance-trained college-aged males (age = 20.5 ± 1.24 years, height = 183.9 ± 6.8 cm, and body mass = 97.0 ± 18.2 kg) were recruited for this study. In a within-groups counterbalanced study design, subjects either listened to preferred or nonpreferred music during a bench press exercise test. Subjects completed as many repetitions as possible at 75% of their 1 repetition maximum with maximum explosive intent. Power and velocity of the barbell movement was measured for the first 3 repetitions using a linear position transducer. Motivation was measured using a visual analog scale immediately after exercise. Each exercise trial was separated by a 48-hour washout period. Results indicate that listening to preferred music increased overall bench press repetitions completed (p = 0.005; effect size [ES] = 0.84). During the first 3 repetitions, mean velocity (p = 0.001; ES = 1.6), relative mean power (p = 0.012; ES = 0.55), peak velocity (p = 0.011; ES = 0.99), and peak power (p = 0.009; ES = 0.35) were higher while listening to preferred music vs. nonpreferred music. Finally, motivation during the lift (p < 0.001; ES = 5.9) was significantly higher while listening to preferred vs. nonpreferred music. Current findings suggest that listening to preferred music by the individual results in greater performance than nonpreferred during resistance exercise. Athletes may benefit from the option to listen to their preferred music to increase motivation and resistance exercise performance.
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Ruberg EJ, Elliott JE, Williams TD. Review of petroleum toxicity and identifying common endpoints for future research on diluted bitumen toxicity in marine mammals. Ecotoxicology 2021; 30:537-551. [PMID: 33761025 PMCID: PMC8060214 DOI: 10.1007/s10646-021-02373-x] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 02/15/2021] [Indexed: 05/15/2023]
Abstract
Large volumes of conventional crude oil continue to be shipped by sea from production to consumption areas across the globe. In addition, unconventional petroleum products also transverse pelagic habitats; for example, diluted bitumen from Canada's oilsands which is shipped along the Pacific coast to the United States and Asia. Therefore, there is a continuing need to assess the toxicological consequences of chronic and catastrophic petroleum spillage on marine wildlife. Peer-reviewed literature on the toxicity of unconventional petroleum such as diluted bitumen exists for teleost fish, but not for fauna such as marine mammals. In order to inform research needs for unconventional petroleum toxicity we conducted a comprehensive literature review of conventional petroleum toxicity on marine mammals. The common endpoints observed in conventional crude oil exposures and oil spills include hematological injury, modulation of immune function and organ weight, genotoxicity, eye irritation, neurotoxicity, lung disease, adrenal dysfunction, metabolic and clinical abnormalities related to oiling of the pelage, behavioural impacts, decreased reproductive success, mortality, and population-level declines. Based on our findings and the body of literature we accessed, our recommendations for future research include: 1) improved baseline data on PAH and metals exposure in marine mammals, 2) improved pre- and post-spill data on marine mammal populations, 3) the use of surrogate mammalian models for petroleum toxicity testing, and 4) the need for empirical data on the toxicity of unconventional petroleum to marine mammals.
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Affiliation(s)
- E J Ruberg
- Department of Biological Sciences, Simon Fraser University, Burnaby, BC, Canada
| | - J E Elliott
- Pacific Wildlife Research Centre, Environment and Climate Change Canada, Delta, BC, Canada.
| | - T D Williams
- Department of Biological Sciences, Simon Fraser University, Burnaby, BC, Canada
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Pavlik M, Williams TD, Green DJ. Female Songbirds Can Initiate the Transition from a Migratory to a Reproductive Physiology during Spring Migration. Physiol Biochem Zool 2021; 94:188-198. [PMID: 33852373 DOI: 10.1086/714218] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
Abstract
AbstractThe high energetic costs of both migration and reproduction and the physiological changes to support these costs suggest that these life-history stages should be compartmentalized with little overlap between stages. In contrast, previous studies have shown that male birds can initiate reproductive development during migration before arrival on the breeding grounds with increases in plasma testosterone levels and testis size. However, sex differences in seasonal gonadal function are now recognized as profound, and few studies to date have shown that females can initiate the costly, but critical, estrogen-dependent final stages of gonadal maturation and changes in liver function (yolk precursor synthesis, vitellogenesis) while on migration. Here, we show that female yellow warblers (Setophaga petechia) arrive on the breeding grounds with elevated plasma triglyceride levels compared with males. Some females had plasma triglyceride levels of 5-7 mmol L-1, suggesting that they arrived in a relatively advanced stage of yolk precursor production. Furthermore, we show that females that arrived with higher plasma triglyceride levels took less time to initiate their first clutch. Adaptive plasticity in the timing of the transition from a migratory to a reproductive physiology might help migrant birds buffer against a mismatch between timing of arrival and conditions on the breeding grounds and allow them to advance timing of breeding to maximize breeding productivity.
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Ballmann CG, Favre ML, Phillips MT, Rogers RR, Pederson JA, Williams TD. Effect of Pre-Exercise Music on Bench Press Power, Velocity, and Repetition Volume. Percept Mot Skills 2021; 128:1183-1196. [PMID: 33722102 DOI: 10.1177/00315125211002406] [Citation(s) in RCA: 17] [Impact Index Per Article: 5.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
The purpose of this study was to examine the effects of listening to pre-exercise music on bench press performance. We recruited 10 resistance trained males (M age= 22.8, SD = 5.8 years; M height= 173.7, SD = 8.3 cm; M body mass = 81.0, SD = 18.2 kg) for this crossover counterbalanced research design. Participants completed two bench press exercise trials of (a) No music (NM), and (b) Pre-exercise music (PreExM) separated by at least 48 hours. For each trial, following a warm-up, participants listened to music or no music for three minutes. After this 3-minute period, they completed one set of bench press repetitions with maximum explosive intent at 75% one repetition maximum (1 RPM). We used a rotary encoder to measure power and velocity of barbell movement. After a 3-minute rest during which they again listened to music or no music, participants completed another set of repetitions to failure (RTF) at 75% of 1RM. Immediately following this second set of repetitions, we measured exercise motivation with a visual analog scale (VAS). We found that the PreExM condition increased mean power output (p = 0.005; d = 0.792) and barbell velocity (p = 0.015; d = 0.722). RTF were significantly higher during the PreExM versus NM trial (p = 0.002; d = 0.985), and motivation was significantly higher in the PreExM trial versus NM (p = 0.001; d = 0.932). These findings suggest improved muscle power explosiveness and strength-endurance when listening to music before a bench press exercise. From a practical standpoint, athletes who have the option of listening to music immediately prior to resistance exercise may benefit from its use.
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Affiliation(s)
| | - Mason L Favre
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Matthew T Phillips
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Rebecca R Rogers
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Joseph A Pederson
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
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Nickerson BS, Williams TD, Snarr RL, Garza JM, Salinas G. Evaluation of Load-Velocity Relationships and Repetitions-to-Failure Equations in the Presence of Male and Female Spotters. J Strength Cond Res 2021; 34:2427-2433. [PMID: 32740290 DOI: 10.1519/jsc.0000000000003731] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
Abstract
Nickerson, BS, Williams, TD, Snarr, RL, Garza, JM, and Salinas, G. Evaluation of load-velocity relationships and repetitions-to-failure equations in the presence of male and female spotters. J Strength Cond Res 34(9): 2427-2433, 2020-The purpose of this study was 2 fold: (a) to determine whether differences in mean concentric velocity (MCV), repetitions-to-failure (RTF), measured 1 repetition maximum (1RM), and 1RM prediction methods vary between lifter and spotter sex and (b) determine the accuracy of velocity-based 1RM (MCV1RM) and repetitions-to-failure-based 1RM (RTF1RM) prediction equations in the presence of either a male or female spotter. Twenty resistance-trained individuals (50% men) participated in this study. The initial 2 visits involved measuring 1RM for the bench press with a male or female spotter. Visits 3 and 4 required subjects to lift loads at 30 (5-repetitions), 50 (5-repetitions), and 70% 1RM (RTF) in the presence of a male or female spotter. Velocity-based 1RM was determined through individual regression equations using the submaximal loads (MCV30, MCV50, and MCV70). Repetitions-to-failure-based 1RM was determined through the RTF at 70% 1RM using Wathen (Wathen1RM), Mayhew (Mayhew1RM), and Epley (Epley1RM) equations. There were significant interactions when assessing Wathen1RM and Mayhew1RM (p < 0.05). Female lifters produced significantly higher estimated 1RM values during the male spotter condition using Wathen1RM and Mayhew1RM than the female spotter condition (p = 0.032 and 0.033, respectively). MCV1RM and Epley1RM produced smaller mean differences than Wathen1RM and Mayhew1RM when compared with measured 1RM. However, MCV1RM produced the largest standard error of estimate, whereas Epley1RM produced the lowest values. Epley1RM should be used over MCV1RM, Wathen1RM, and Mayhew1RM when loads up to 70% 1RM are implemented. Also, spotter sex only seems to impact female lifters when using the RTF1RM prediction equations of Wathen1RM and Mayhew1RM.
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Affiliation(s)
- Brett S Nickerson
- College of Nursing and Health Sciences, Texas A&M, International University, Laredo, Texas
| | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, Alabama
| | - Ronald L Snarr
- Department of Health Sciences and Kinesiology, Georgia Southern University, Statesboro, Georgia; and
| | - Jessica M Garza
- Department of Psychology and Communication, Texas A&M International University, Laredo, Texas
| | - Gilberto Salinas
- Department of Psychology and Communication, Texas A&M International University, Laredo, Texas
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Williams TD, Esco MR, Fedewa MV, Bishop PA. Inter- and Intra-Day Comparisons of Smartphone-Derived Heart Rate Variability across Resistance Training Overload and Taper Microcycles. Int J Environ Res Public Health 2020; 18:ijerph18010177. [PMID: 33383719 PMCID: PMC7795557 DOI: 10.3390/ijerph18010177] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 11/24/2020] [Revised: 12/21/2020] [Accepted: 12/23/2020] [Indexed: 11/16/2022]
Abstract
The purposes of this study were: (1) to determine if smartphone-derived heart rate variability (HRV) could detect changes in training load during an overload microcycle and taper, and (2) to determine the reliability of HRV measured in the morning and measured immediately prior to the testing session. Twelve powerlifters (male = 10, female = 2) completed a 3-week resistance training program consisting of an introduction microcycle, overload microcycle, and taper. Using a validated smartphone application, daily measures of resting, ultra-short natural logarithm of root mean square of successive differences were recorded in the morning (LnRMSSDM) and immediately before the test session (LnRMSSDT) following baseline, post-overload, and post-taper testing. LnRMSSDM decreased from baseline (82.9 ± 13.0) to post-overload (75.0 ± 9.9, p = 0.019), while post-taper LnRMSSDM (81.9 ± 7.1) was not different from post-overload (p = 0.056) or baseline (p = 0.998). No differences in LnRMSSDT (p < 0.05) were observed between baseline (78.3 ± 9.0), post-overload (74.4 ± 10.2), and post-taper (78.3 ± 8.0). LnRMSSDM and LnRMSSDT were strongly correlated at baseline (ICC = 0.71, p < 0.001) and post-overload (ICC = 0.65, p = 0.010), whereas there was no relationship at post-taper (ICC = 0.44, p = 0.054). Bland–Altman analyses suggest extremely wide limits of agreement (Bias ± 1.96 SD) between LnRMSSDM and LnRMSSDT at baseline (4.7 ± 15.2), post-overload (0.5 ± 16.9), and post-taper (3.7 ± 15.3). Smartphone-derived HRV, recorded upon waking, was sensitive to resistance training loads across an overload and taper microcycles in competitive strength athletes, whereas the HRV was taken immediately prior to the testing session was not.
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Affiliation(s)
- Tyler D. Williams
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
- Department of Kinesiology, University of Alabama, Tuscaloosa, AL 35487, USA; (M.R.E.); (M.V.F.); (P.A.B.)
- Correspondence:
| | - Michael R. Esco
- Department of Kinesiology, University of Alabama, Tuscaloosa, AL 35487, USA; (M.R.E.); (M.V.F.); (P.A.B.)
| | - Michael V. Fedewa
- Department of Kinesiology, University of Alabama, Tuscaloosa, AL 35487, USA; (M.R.E.); (M.V.F.); (P.A.B.)
| | - Phillip A. Bishop
- Department of Kinesiology, University of Alabama, Tuscaloosa, AL 35487, USA; (M.R.E.); (M.V.F.); (P.A.B.)
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Williams TD, Esco MR, Fedewa MV, Bishop PA. Bench Press Load-Velocity Profiles and Strength After Overload and Taper Microcyles in Male Powerlifters. J Strength Cond Res 2020; 34:3338-3345. [PMID: 33021581 DOI: 10.1519/jsc.0000000000003835] [Citation(s) in RCA: 4] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
Abstract
Williams, TD, Esco, MR, Fedewa, MV, and Bishop, PA. Bench press load-velocity profiles and strength after overload and taper microcyles in male powerlifters. J Strength Cond Res 34(12): 3338-3345, 2020-The purpose of this study was to quantify the effect of an overload microcycle and taper on bench press velocity and to determine if the load-velocity relationship could accurately predict 1-repetition maximum (1RM). Twelve male powerlifters participated in resistance training structured into an introduction microcycle, overload microcycle (PostOL), and taper (PostTP). At the end of each microcycle, subjects completed a bench press for 1RM assessment consisting of warm-up sets at 40, 55, 70, and 85% of a previously established 1RM. The mean concentric velocity (MCV) was recorded during each warm-up set. A predicted 1RM (p1RM) was calculated using an individualized load-velocity profile (LVP). The average MCV decreased after PostOL (0.66 ± 0.07 m·s) compared with baseline (BL) (p = 0.003; 0.60 ± 0.11 m·s) but increased after PostTP (0.67 ± 0.09 m·s). One-repetition maximum increased from PostOL (146.7 ± 19.8 kg) to PostTP (p = 0.002; 156.1 ± 21.0 kg), with no differences observed between other test sessions (p > 0.05). Bland-Altman analysis indicated that p1RM was consistently higher than measured 1RM (3.4-7.8 kg), and the limits of agreement were extremely wide. However, very large to near perfect correlations (r = 0.89 to 0.96) were observed between p1RM and 1RM during BL, PostOL, and PostTP. The load-velocity relationship established from submaximal sets did not accurately predict 1RM, but MCV was affected by changes in weekly training loads. Velocity-based measurements seem to be more sensitive to changes in training loads than maximal strength.
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Affiliation(s)
- Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, Alabama; and.,Department of Kinesiology, University of Alabama, Tuscaloosa, Alabama
| | - Michael R Esco
- Department of Kinesiology, University of Alabama, Tuscaloosa, Alabama
| | - Michael V Fedewa
- Department of Kinesiology, University of Alabama, Tuscaloosa, Alabama
| | - Phillip A Bishop
- Department of Kinesiology, University of Alabama, Tuscaloosa, Alabama
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Williams TD, Martin MP, Mintz JA, Rogers RR, Ballmann CG. Effect of Acute Beetroot Juice Supplementation on Bench Press Power, Velocity, and Repetition Volume. J Strength Cond Res 2020; 34:924-928. [PMID: 31913252 DOI: 10.1519/jsc.0000000000003509] [Citation(s) in RCA: 35] [Impact Index Per Article: 8.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
Abstract
Williams, TD, Martin, MP, Mintz, JA, Rogers, RR, and Ballmann, CG. Effect of acute beetroot juice supplementation on bench press power, velocity, and repetition volume. J Strength Cond Res 34(4): 924-928, 2020-The purpose of this study was to examine the effects of acute beetroot juice (BRJ) supplementation on power, velocity, and repetitions to failure (RTF) during bench press exercise. Resistance-trained male subjects (n = 11) were recruited for this study. Using a double-blinded, counterbalanced, crossover study design, subjects were supplemented with either 70 ml of BRJ or placebo (PL; black currant juice) 2 hours before exercise. During each exercise trial, subjects began by completing 2 sets × 2 repetitions of bench press at 70% 1 repetition maximum (1RM) with maximum explosive intent. Barbell velocity and power were measured using a linear position transducer. Subjects then completed 3 sets × RTF at 70% 1RM separated by 2 minutes of rest between each set. Maximum mean power, velocity, and repetitions were analyzed. Mean velocity (p = 0.011; effect size [ES] = 0.54) and mean power (p = 0.015; ES = 0.51) were significantly higher with BRJ when compared with PL. Total RTF (p = 0.002; ES = 0.46) was higher during the BRJ condition vs. PL. Results indicate that acute BRJ supplementation positively impacts velocity, power, and total repetitions during free-weight bench press exercise.
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Affiliation(s)
- Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, Alabama
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Duckworth SC, Higginbotham CS, Pederson JA, Rogers RR, Marshall MR, Williams TD, Ballmann CG. Physical and Cognitive Performance During Upper-Extremity Versus Full-Body Exercise Under Dual Tasking Conditions. Percept Mot Skills 2020; 128:338-352. [PMID: 32741251 DOI: 10.1177/0031512520945088] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022]
Abstract
The purpose of this study was to investigate physical and cognitive performance during dual task conditions of upper-extremity (UE) or full-body (FB) rowing exercise. In a crossover counterbalanced design, college-aged male and female participants completed five conditions: (a) Sitting, (b) Single task UE rowing, (c) Single task FB rowing, (d) Dual task UE rowing, and (e) Dual task FB rowing. For single task UE and FB rowing conditions, participants were asked to row as hard as possible. After sitting and dual-task conditions, we administered the Paced Auditory Serial Addition Test (PASAT) and a word-list memory test. We analyzed participants' absolute differences (single task - dual task) in power output and their cognitive test scores to compare UE and FB rowing. There were no significant absolute differences from sitting to dual task conditions of UE and FB rowing for either PASAT (p = 0.958) or word list memory (p = 0.899) cognitive scores. Absolute power output loss from single to dual task conditions was significantly higher in FB versus UE for PASAT (p = 0.039; d = 0.54) and word list memory (p = 0.021; d = 0.66) in the dual task condition. These results suggest that, while cognitive performance was preserved regardless of the amount of muscle mass activated during dual task rowing, physical performance suffered more during FB than UE rowing under the dual task condition. These findings have important implications for optimizing cognitive and physical performance in dual task situations.
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Affiliation(s)
- Sarah C Duckworth
- Department of Kinesiology, 1744Samford University, Birmingham, Alabama, United States
| | - Carrie S Higginbotham
- Department of Kinesiology, 1744Samford University, Birmingham, Alabama, United States
| | - Joseph A Pederson
- Department of Kinesiology, 1744Samford University, Birmingham, Alabama, United States
| | - Rebecca R Rogers
- Department of Kinesiology, 1744Samford University, Birmingham, Alabama, United States
| | - Mallory R Marshall
- Department of Kinesiology, 1744Samford University, Birmingham, Alabama, United States
| | - Tyler D Williams
- Department of Kinesiology, 1744Samford University, Birmingham, Alabama, United States
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Karow MC, Rogers RR, Pederson JA, Williams TD, Marshall MR, Ballmann CG. Effects of Preferred and Nonpreferred Warm-Up Music on Exercise Performance. Percept Mot Skills 2020; 127:912-924. [PMID: 32493179 DOI: 10.1177/0031512520928244] [Citation(s) in RCA: 18] [Impact Index Per Article: 4.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/17/2022]
Abstract
This study investigated the effects of preferred and non-preferred warm-up music listening conditions on subsequent exercise performance. A total of 12 physically active male and female participants engaged in a crossover, counterbalanced research design in which they completed exercise trials after 3 different warm-up experiences of (a) no music (NM), (b) preferred music (PREF), and (c) nonpreferred music (NON-PREF). Participants began warming up by rowing at 50% of of age-predicted heart rate maximum (HRmax) for 5 minutes while exposed to the three music conditions. Immediately following the warm-up and cessation of any music, participants completed a 2000-m rowing time trial as fast as possible. Relative power output, trial time, heart rate, rating of perceived exertion, and motivation were analyzed. Results indicated that, compared with NM, relative power output was significantly higher (p = .018), trial time was significantly lower (p = .044), and heart rate was significantly higher (p = .032) during the PREF but not the NON-PREF condition. Rating of perceived exertion was not altered, regardless of music condition (p > .05). Motivation to exercise was higher during the PREF condition versus the NM (p = .001) and NON-PREF (p < .001) conditions. Listening to preferred warm-up music improved subsequent exercise performance compared with no music, while nonpreferred music did not impart ergogenic benefit.
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Affiliation(s)
- Morgan C Karow
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Rebecca R Rogers
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Joseph A Pederson
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Mallory R Marshall
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
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Nickerson BS, Williams TD, Snarr RL, Park KS. Individual and Combined Effect of Inter-repetition Rest and Elastic Bands on Jumping Potentiation in Resistance-Trained Men. J Strength Cond Res 2019; 33:2087-2093. [PMID: 29863591 DOI: 10.1519/jsc.0000000000002593] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
Abstract
Nickerson, BS, Williams, TD, Snarr, RL, and Park, K-S. Individual and combined effect of inter-repetition rest and elastic bands on jumping potentiation in resistance-trained men. J Strength Cond Res 33(8): 2087-2093, 2019-The purpose of this study was to determine the individual and combined effects of cluster sets (CS) and elastic bands for jumping potentiation in resistance-trained men. Twelve resistance-trained men (age: 22 ± 3 years) participated in this study. In a random order, participants completed 1 set of 3 repetitions at 85% 1-repetition maximum for the parallel back squat: (a) traditional set with continuous repetitions; (b) continuous repetitions with elastic bands (BANDS); (c) CS with 30 seconds of rest between each repetition (CS30); and (d) CS with 30 seconds of rest between each repetition and elastic bands (CS + BANDS). Vertical jump height (JH) and peak power (PP) were measured before exercise (baseline) and at 1, 4, 7, and 10 minutes after exercise for each condition. Results revealed that PP at 10 minutes was significantly higher than 7 minutes for BANDS (p = 0.035) and that 4 and 7minutes were both significantly higher than baseline for CS + BANDS (p = 0.008 and 0.031, respectively). No other differences were observed. There were medium effect sizes (ESs) for PP with BANDS (ES = 0.58 at 10 minutes), CS30 (ES = 0.53 and 0.64 at 7 and 10 minutes, respectively), and CS + BANDS (ES = 0.64, 0.78, and 0.66 at 4, 7, and 10 minutes, respectively). All remaining ES for JH and PP were trivial to small. Based on the moderate magnitude of effect, BANDS, CS30, and CS + BANDS were effective at potentiating vertical jump power. CS + BANDS is a more practical approach to potentiate vertical jump power when athletes are under strict time restraints.
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Affiliation(s)
- Brett S Nickerson
- Department of Professional Programs, Texas A&M International University, Laredo, Texas
| | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, Alabama
| | - Ronald L Snarr
- Department of Health Sciences and Kinesiology, Georgia Southern University, Statesboro, Georgia
| | - Kyung-Shin Park
- Department of Professional Programs, Texas A&M International University, Laredo, Texas
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Fedewa MV, Spencer SO, Williams TD, Becker ZE, Fuqua CA. Effect of branched-Chain Amino Acid Supplementation on Muscle Soreness following Exercise: A Meta-Analysis. INT J VITAM NUTR RES 2019; 89:348-356. [DOI: 10.1024/0300-9831/a000543] [Citation(s) in RCA: 18] [Impact Index Per Article: 3.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/16/2023]
Abstract
Abstract. Delayed onset muscle soreness (DOMS) is a symptom of exercise-induced muscle damage that occurs following exercise. Previous research has indicated that branched-chain amino acid (BCAA) supplementation may attenuate exercise-induced muscle damage that causes delayed onset muscle soreness, however the results are inconsistent. The primary aim of this study was to examine the previous literature assessing the effect of BCAA supplementation on DOMS following an acute bout of exercise in adults. This review was conducted in accordance with PRISMA guidelines (Preferred Reporting Items for Systematic Reviews and Meta-analyses), and identified peer-reviewed articles comparing a BCAA supplement to a placebo non-BCAA supplement following an acute bout of exercise. An electronic search of three databases (EbscoHost, Web of Science, and SPORTDiscus) yielded 42 articles after duplicates were removed. All studies included in the current analyis were: 1) peer-reviewed publications; 2) available in English; 3) utilized a random control design that compared a BCAA group to a placebo control group following exercise; 4) and assessed soreness of muscle tissue during recovery. DOMS was assessed in 61 participants following ingestion of a BCAA supplement over the course of these interventions. The cumulative results of 37 effects gathered from 8 studies published between 2007 and 2017 indicated that BCAA supplementation reduced DOMS following exercise training (ES = 0.7286, 95% CI: 0.5017 to 0.9555, p < 0.001). A large decrease in DOMS occurs following BCAA supplementation after exercise compared to a placebo supplement.
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Affiliation(s)
- Michael V. Fedewa
- Department of Kinesiology, The University of Alabama, Tuscaloosa, Alabama, United States
| | - Steven O. Spencer
- Department of Kinesiology, The University of Alabama, Tuscaloosa, Alabama, United States
| | - Tyler D. Williams
- Department of Kinesiology, The University of Alabama, Tuscaloosa, Alabama, United States
- Department of Kinesiology, Samford University, Birmingham, Alabama, United States
| | - Zachery E. Becker
- Department of Kinesiology, The University of Alabama, Tuscaloosa, Alabama, United States
| | - Collin A. Fuqua
- Department of Kinesiology, The University of Alabama, Tuscaloosa, Alabama, United States
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Miller RA, Rogers RR, Williams TD, Marshall MR, Moody JR, Hensarling RW, Ballmann CG. Effects of Protective American Football Headgear on Peripheral Vision Reaction Time and Visual Target Detection in Division I NCAA Football Players. Sports (Basel) 2019; 7:E213. [PMID: 31527412 PMCID: PMC6783852 DOI: 10.3390/sports7090213] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/25/2019] [Revised: 09/10/2019] [Accepted: 09/11/2019] [Indexed: 11/16/2022] Open
Abstract
The purpose of this study was to examine the effects of protective football headgear on peripheral vision reaction time and visual target detection. Twenty-five Division I NCAA football players (age = 20.5 yrs ± 0.9, height = 185.9 cm ± 6.8, body mass = 99.2 kg ± 19.2, BMI = 29.6 ± 4.5) participated. In a crossover counterbalanced study design, subjects participated in one visit with three conditions: Baseline (BL) without headgear, helmet only (HO), helmet with an eye shield (HE). Subjects completed a 1-min peripheral vision reaction time test for each condition separated by 3-min recovery periods. Tests were administered using a 64 light Dynavision D2 Visuomotor board. Target detection (total hit score) was higher during BL than HO (p < 0.001) and HE (p < 0.001). Average (p < 0.001), peak (p < 0.001), minimum (p < 0.001), and median (p < 0.001) peripheral reaction times were faster during BL than HO and HE. No significant differences were observed for any measures between HO and HE conditions (p > 0.05). Findings indicate that protective football headgear impaired reaction time to peripheral visual stimuli. The addition of an eye shield to the helmet had a small non-significant effect on reaction time and target detection. These results may hold important implications in helmet design and player safety.
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Affiliation(s)
- Rachel A Miller
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA.
| | - Rebecca R Rogers
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA.
| | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA.
| | - Mallory R Marshall
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA.
| | - Justin R Moody
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA.
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Ballmann CG, Maynard DJ, Lafoon ZN, Marshall MR, Williams TD, Rogers RR. Effects of Listening to Preferred versus Non-Preferred Music on Repeated Wingate Anaerobic Test Performance. Sports (Basel) 2019; 7:E185. [PMID: 31362419 PMCID: PMC6723041 DOI: 10.3390/sports7080185] [Citation(s) in RCA: 22] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/21/2019] [Revised: 07/22/2019] [Accepted: 07/25/2019] [Indexed: 11/17/2022] Open
Abstract
The purpose of this study was to examine the effects of listening to preferred or non-preferred music on repeated sprint performance. Fourteen physically active males (ages 18-25 years) were recruited for this study. In a counterbalanced crossover study design, participants completed two separate visits. During each visit, participants listened to either preferred or non-preferred music and completed 3 × 15 s Wingate Anaerobic Tests (WAnTs) separated by 2 min active recovery periods. Each visit was separated by a minimal recovery period of 48 h. Anaerobic performance measures, heart rate, rate of perceived exertion (RPE), and motivation were analyzed. Mean power (p = 0.846, effect size (ES) = 0.019), anaerobic capacity (p = 0.686, ES = 0.058), and total work (p = 0.677, ES = 0.039) were not significantly different between preferred and non-preferred music conditions. Mean heart rate (p = 0.608; ES = 0.125) was also unchanged. Motivation to exercise (p < 0.001; ES = 1.520) was significantly higher in the preferred music condition. Additionally, the rate of perceived exertion (RPE) (p = 0.028; ES = 0.540) was significantly lower during the preferred music condition. Our results show that listening to preferred music showed no ergogenic benefit during repeated anaerobic cycling sprints when compared to non-preferred music. However, preferred music increased motivation to exercise and decreased perceived exertion. The results from this study could hold important implications for the application of music and enduring repeated high-intensity sprint exercise.
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Affiliation(s)
| | - Daniel J Maynard
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
| | - Zachary N Lafoon
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
| | - Mallory R Marshall
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
| | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
| | - Rebecca R Rogers
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
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Ballmann CG, Martin MP, Rogers RR, Williams TD. Effects of Acute Beetroot Juice Supplementation on Power, Velocity, and Repetitions to Failure during Resistance Exercise. FASEB J 2019. [DOI: 10.1096/fasebj.2019.33.1_supplement.839.3] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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Fedewa MV, Hathaway ED, Ward-Ritacco CL, Williams TD, Dobbs WC. The Effect of Chronic Exercise Training on Leptin: A Systematic Review and Meta-Analysis of Randomized Controlled Trials. Sports Med 2018; 48:1437-1450. [PMID: 29582381 DOI: 10.1007/s40279-018-0897-1] [Citation(s) in RCA: 66] [Impact Index Per Article: 11.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/07/2023]
Abstract
BACKGROUND Leptin is a hormone associated with satiety, lipid oxidation, energy expenditure, and energy homeostasis. To date, the current body of research examining the effect of chronic exercise training on leptin has yielded inconsistent results. OBJECTIVE The purpose of this meta-analysis was to provide a quantitative estimate of the magnitude of change in leptin levels following participation in exercise interventions lasting ≥ 2 weeks. METHODS All studies included were peer-reviewed and published in English. To be included, studies randomized human participants to an exercise training group or non-exercise comparison group for an exercise training intervention. Leptin levels were measured at baseline, during, and/or after completion of the exercise training program. Random-effects models were used to aggregate a mean effect size (ES) and 95% confidence intervals (CIs), and identify potential moderators. RESULTS Seventy-two randomized controlled trials met the inclusion criteria and resulted in 107 effects (n = 3826). The mean ES of 0.24 (95% CI 0.16-0.32, p < 0.0001) indicated a decrease in leptin following an exercise training program. A decrease in %Fat (β = - 0.07, p < 0.01) was associated with a decrease in leptin after accounting for the type of control group (β = - 0.38, p < 0.0001) used in each study. CONCLUSION These results suggest that engaging in chronic exercise training (≥ 2 weeks) is associated with a decrease in leptin levels for individuals regardless of age and sex. However, a greater decrease in leptin occurred with a decreased percentage of body fat.
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Affiliation(s)
- Michael V Fedewa
- Department of Kinesiology, The University of Alabama, 2003 Moore Hall, Box 870312, Tuscaloosa, AL, 35487-0231, USA.
| | - Elizabeth D Hathaway
- Department of Health and Human Performance, The University of Tennessee at Chattanooga, Chattanooga, TN, USA
| | | | - Tyler D Williams
- Department of Kinesiology, Samford University, Birmingham, AL, USA
| | - Ward C Dobbs
- Department of Kinesiology, The University of Alabama, 2003 Moore Hall, Box 870312, Tuscaloosa, AL, 35487-0231, USA
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Nickerson BS, Mangine GT, Williams TD, Martinez IA. Effect of cluster set warm-up configurations on sprint performance in collegiate male soccer players. Appl Physiol Nutr Metab 2018; 43:625-630. [DOI: 10.1139/apnm-2017-0610] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/22/2022]
Abstract
The purpose of this study was to determine if back squat cluster sets (CS) with varying inter-repetition rest periods would potentiate greater sprint performance compared with a traditional set parallel back squat in collegiate soccer players. Twelve collegiate male soccer players (age, 21.0 ± 2.0 years; height, 180.0 ± 9.0 cm; body mass, 79.0 ± 9.5 kg) performed a 20-m sprint prior to a potentiation complex and at 1, 4, 7, and 10 min postexercise on 3 separate, randomized occasions. On each occasion, the potentiation complex consisted of 1 set of 3 repetitions at 85% 1-repetition maximum (1RM) for the traditional parallel back squat. However, on 1 occasion the 3-repetition set was performed in a traditional manner (i.e., continuously), whereas on the other 2 occasions, 30s (CS30) and 60 s (CS60) of rest were allotted between each repetition. Repeated-measures ANOVA revealed greater (p = 0.022) mean barbell velocity on CS60 compared with the traditional set. However, faster (p < 0.040) 20-m sprint times were observed for CS30 (3.15 ± 0.16 s) compared with traditional (3.20 ± 0.17 s) only at 10 min postexercise. No other differences were observed. These data suggest that a single cluster set of 3 repetitions with 30-s inter-repetition rest periods at 85% 1RM acutely improves 20-m sprinting performance. Strength and conditioning professionals and their athletes might consider its inclusion during the specific warm-up to acutely improve athletic performance during the onset (≤10 min) of training or competition.
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Affiliation(s)
- Brett S. Nickerson
- Texas A&M International University Exercise Physiology Laboratory, USA
- Department of Professional Programs, Texas A&M International University, Laredo, TX 78041, USA
| | - Gerald T. Mangine
- Department of Exercise Science and Sport Management, Kennesaw State University, Kennesaw, GA 30144, USA
| | - Tyler D. Williams
- Department of Kinesiology, Samford University, Birmingham, AL 35229, USA
| | - Ismael A. Martinez
- Texas A&M International University Exercise Physiology Laboratory, USA
- Department of Professional Programs, Texas A&M International University, Laredo, TX 78041, USA
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Affiliation(s)
- R I Holt
- Thanet District Hospital St Peter's Road, Margate, Kent, England
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Bishop PA, Williams TD, Heldman AN, Vanderburgh PM. System for Evaluating Powerlifting and Other Multievent Performances. J Strength Cond Res 2018; 32:201-204. [DOI: 10.1519/jsc.0000000000001808] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/08/2022]
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Davis ML, Elliott JE, Williams TD. The Glaucous-Winged Gull (Larus glaucescens) as an Indicator of Chemical Contaminants in the Canadian Pacific Marine Environment: Evidence from Stable Isotopes. Arch Environ Contam Toxicol 2017; 73:247-255. [PMID: 28528408 DOI: 10.1007/s00244-017-0368-y] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/23/2016] [Accepted: 01/17/2017] [Indexed: 06/07/2023]
Abstract
The Glaucous-winged gull (Larus glaucescens) has been selected by Environment Canada as a marine indicator species for long-term monitoring of persistent contaminants in the Canadian Pacific. However, the indicator value of this species depends on its trophic level and proportion of marine prey in its diet. Eggs, used as the monitoring medium, are produced entirely from maternal resources and knowledge of adult diet before and during egg production is critical to interpreting contaminant levels. Due to a lack of recent and reliable dietary ecology work, we examined the diet of breeding Glaucous-winged gulls through carbon (δ13C) and nitrogen (δ15N) stable isotope analysis at three colonies on the Pacific coast. Near-shore marine prey, occupying a high trophic level (δ15N), composed a predominant component of all Glaucous-winged gull diet. Adult diet composition from colonies in the Salish Sea was more varied than the west coast of Vancouver Island, reflecting the opportunistic foraging nature of this species in areas where the abundance of marine prey is known to fluctuate. Compared with incubating adults, pre-laying adults had a significantly lower trophic level that may reflect the need to consume marine invertebrates to acquire specific nutrients necessary for egg production. Interannual variation in both trophic level and prey source (δ13C) in egg and chick tissues indicates the need to pair ongoing contaminant monitoring with stable isotope analysis. The predominantly marine diet and relatively high trophic level of this gull supports its use as an indicator of marine pollution on the Pacific coast.
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Affiliation(s)
- M L Davis
- Centre for Wildlife Ecology, Department of Biological Sciences, Simon Fraser University, 8888 University Drive, Burnaby, BC, V5A 1S6, Canada
- Hemmera, 4730 Kingsway, Burnaby, BC, V5H OC6, Canada
| | - J E Elliott
- Centre for Wildlife Ecology, Department of Biological Sciences, Simon Fraser University, 8888 University Drive, Burnaby, BC, V5A 1S6, Canada.
- Pacific Wildlife Research Centre, Environment Canada, Delta, BC, V4K 3N2, Canada.
| | - T D Williams
- Centre for Wildlife Ecology, Department of Biological Sciences, Simon Fraser University, 8888 University Drive, Burnaby, BC, V5A 1S6, Canada
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Fedewa MV, Hathaway ED, Ward-Ritacco CL, Williams TD. The Effect Of Exercise Training On Leptin. Med Sci Sports Exerc 2017. [DOI: 10.1249/01.mss.0000519156.44913.86] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/21/2022]
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Fedewa MV, Hathaway ED, Williams TD, Schmidt MD. Effect of Exercise Training on Non-Exercise Physical Activity: A Systematic Review and Meta-Analysis of Randomized Controlled Trials. Sports Med 2016; 47:1171-1182. [DOI: 10.1007/s40279-016-0649-z] [Citation(s) in RCA: 23] [Impact Index Per Article: 2.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/08/2023]
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Aasi J, Abbott BP, Abbott R, Abbott T, Abernathy MR, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, Affeldt C, Agathos M, Aggarwal N, Aguiar OD, Ajith P, Alemic A, Allen B, Allocca A, Amariutei D, Andersen M, Anderson RA, Anderson SB, Anderson WG, Arai K, Araya MC, Arceneaux C, Areeda JS, Ast S, Aston SM, Astone P, Aufmuth P, Augustus H, Aulbert C, Aylott BE, Babak S, Baker PT, Ballardin G, Ballmer SW, Barayoga JC, Barbet M, Barish BC, Barker D, Barone F, Barr B, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Basti A, Batch JC, Bauchrowitz J, Bauer TS, Baune C, Bavigadda V, Behnke B, Bejger M, Beker MG, Belczynski C, Bell AS, Bell C, Bergmann G, Bersanetti D, Bertolini A, Betzwieser J, Bilenko IA, Billingsley G, Birch J, Biscans S, Bitossi M, Biwer C, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bloemen S, Bock O, Bodiya TP, Boer M, Bogaert G, Bogan C, Bond C, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Boschi V, Bose S, Bosi L, Bradaschia C, Brady PR, Braginsky VB, Branchesi M, Brau JE, Briant T, Bridges DO, Brillet A, Brinkmann M, Brisson V, Brooks AF, Brown DA, Brown DD, Brückner F, Buchman S, Buikema A, Bulik T, Bulten HJ, Buonanno A, Burman R, Buskulic D, Buy C, Cadonati L, Cagnoli G, Calderón Bustillo J, Calloni E, Camp JB, Campsie P, Cannon KC, Canuel B, Cao J, Capano CD, Carbognani F, Carbone L, Caride S, Castaldi G, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Celerier C, Cella G, Cepeda C, Cesarini E, Chakraborty R, Chalermsongsak T, Chamberlin SJ, Chao S, Charlton P, Chassande-Mottin E, Chen X, Chen Y, Chincarini A, Chiummo A, Cho HS, Cho M, Chow JH, Christensen N, Chu Q, Chua SSY, Chung S, Ciani G, Clara F, Clark DE, Clark JA, Clayton JH, Cleva F, Coccia E, Cohadon PF, Colla A, Collette C, Colombini M, Cominsky L, Constancio M, Conte A, Cook D, Corbitt TR, Cornish N, Corsi A, Costa CA, Coughlin MW, Coulon JP, Countryman S, Couvares P, Coward DM, Cowart MJ, Coyne DC, Coyne R, Craig K, Creighton JDE, Croce RP, Crowder SG, Cumming A, Cunningham L, Cuoco E, Cutler C, Dahl K, Dal Canton T, Damjanic M, Danilishin SL, D'Antonio S, Danzmann K, Dattilo V, Daveloza H, Davier M, Davies GS, Daw EJ, Day R, Dayanga T, DeBra D, Debreczeni G, Degallaix J, Deléglise S, Del Pozzo W, Denker T, Dent T, Dereli H, Dergachev V, De Rosa R, DeRosa RT, DeSalvo R, Dhurandhar S, Díaz M, Dickson J, Di Fiore L, Di Lieto A, Di Palma I, Di Virgilio A, Dolique V, Dominguez E, Donovan F, Dooley KL, Doravari S, Douglas R, Downes TP, Drago M, Drever RWP, Driggers JC, Du Z, Ducrot M, Dwyer S, Eberle T, Edo T, Edwards M, Effler A, Eggenstein HB, Ehrens P, Eichholz J, Eikenberry SS, Endrőczi G, Essick R, Etzel T, Evans M, Evans T, Factourovich M, Fafone V, Fairhurst S, Fan X, Fang Q, Farinon S, Farr B, Farr WM, Favata M, Fazi D, Fehrmann H, Fejer MM, Feldbaum D, Feroz F, Ferrante I, Ferreira EC, Ferrini F, Fidecaro F, Finn LS, Fiori I, Fisher RP, Flaminio R, Fournier JD, Franco S, Frasca S, Frasconi F, Frede M, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fulda P, Fyffe M, Gair JR, Gammaitoni L, Gaonkar S, Garufi F, Gehrels N, Gemme G, Gendre B, Genin E, Gennai A, Ghosh S, Giaime JA, Giardina KD, Giazotto A, Gleason J, Goetz E, Goetz R, Gondan L, González G, Gordon N, Gorodetsky ML, Gossan S, Goßler S, Gouaty R, Gräf C, Graff PB, Granata M, Grant A, Gras S, Gray C, Greenhalgh RJS, Gretarsson AM, Groot P, Grote H, Grover K, Grunewald S, Guidi GM, Guido CJ, Gushwa K, Gustafson EK, Gustafson R, Ha J, Hall ED, Hamilton W, Hammer D, Hammond G, Hanke M, Hanks J, Hanna C, Hannam MD, Hanson J, Harms J, Harry GM, Harry IW, Harstad ED, Hart M, Hartman MT, Haster CJ, Haughian K, Heidmann A, Heintze M, Heitmann H, Hello P, Hemming G, Hendry M, Heng IS, Heptonstall AW, Heurs M, Hewitson M, Hild S, Hoak D, Hodge KA, Hofman D, Holt K, Hopkins P, Horrom T, Hoske D, Hosken DJ, Hough J, Howell EJ, Hu Y, Huerta E, Hughey B, Husa S, Huttner SH, Huynh M, Huynh-Dinh T, Idrisy A, Ingram DR, Inta R, Islas G, Isogai T, Ivanov A, Iyer BR, Izumi K, Jacobson M, Jang H, Jaranowski P, Ji Y, Jiménez-Forteza F, Johnson WW, Jones DI, Jones R, Jonker RJG, Ju L, Haris K, Kalmus P, Kalogera V, Kandhasamy S, Kang G, Kanner JB, Karlen J, Kasprzack M, Katsavounidis E, Katzman W, Kaufer H, Kaufer S, Kaur T, Kawabe K, Kawazoe F, Kéfélian F, Keiser GM, Keitel D, Kelley DB, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khazanov EA, Kim C, Kim K, Kim NG, Kim N, Kim S, Kim YM, King EJ, King PJ, Kinzel DL, Kissel JS, Klimenko S, Kline J, Koehlenbeck S, Kokeyama K, Kondrashov V, Koranda S, Korth WZ, Kowalska I, Kozak DB, Kringel V, Krishnan B, Królak A, Kuehn G, Kumar A, Kumar DN, Kumar P, Kumar R, Kuo L, Kutynia A, Lam PK, Landry M, Lantz B, Larson S, Lasky PD, Lazzarini A, Lazzaro C, Leaci P, Leavey S, Lebigot EO, Lee CH, Lee HK, Lee HM, Lee J, Lee PJ, Leonardi M, Leong JR, Leonor I, Le Roux A, Leroy N, Letendre N, Levin Y, Levine B, Lewis J, Li TGF, Libbrecht K, Libson A, Lin AC, Littenberg TB, Lockerbie NA, Lockett V, Lodhia D, Loew K, Logue J, Lombardi AL, Lopez E, Lorenzini M, Loriette V, Lormand M, Losurdo G, Lough J, Lubinski MJ, Lück H, Lundgren AP, Ma Y, Macdonald EP, MacDonald T, Machenschalk B, MacInnis M, Macleod DM, Magaña-Sandoval F, Magee R, Mageswaran M, Maglione C, Mailand K, Majorana E, Maksimovic I, Malvezzi V, Man N, Manca GM, Mandel I, Mandic V, Mangano V, Mangini NM, Mansell G, Mantovani M, Marchesoni F, Marion F, Márka S, Márka Z, Markosyan A, Maros E, Marque J, Martelli F, Martin IW, Martin RM, Martinelli L, Martynov D, Marx JN, Mason K, Masserot A, Massinger TJ, Matichard F, Matone L, Mavalvala N, May G, Mazumder N, Mazzolo G, McCarthy R, McClelland DE, McGuire SC, McIntyre G, McIver J, McLin K, Meacher D, Meadors GD, Mehmet M, Meidam J, Meinders M, Melatos A, Mendell G, Mercer RA, Meshkov S, Messenger C, Meyer MS, Meyers PM, Mezzani F, Miao H, Michel C, Mikhailov EE, Milano L, Miller J, Minenkov Y, Mingarelli CMF, Mishra C, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Moe B, Moggi A, Mohan M, Mohapatra SRP, Moraru D, Moreno G, Morgado N, Morriss SR, Mossavi K, Mours B, Mow-Lowry CM, Mueller CL, Mueller G, Mukherjee S, Mullavey A, Munch J, Murphy D, Murray PG, Mytidis A, Nagy MF, Nardecchia I, Naticchioni L, Nayak RK, Necula V, Nelemans G, Neri I, Neri M, Newton G, Nguyen T, Nielsen AB, Nissanke S, Nitz AH, Nocera F, Nolting D, Normandin MEN, Nuttall LK, Ochsner E, O'Dell J, Oelker E, Oh JJ, Oh SH, Ohme F, Omar S, Oppermann P, Oram R, O'Reilly B, Ortega W, O'Shaughnessy R, Osthelder C, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Padilla C, Pai A, Palashov O, Palomba C, Pan H, Pan Y, Pankow C, Paoletti F, Papa MA, Paris H, Pasqualetti A, Passaquieti R, Passuello D, Pedraza M, Pele A, Penn S, Perreca A, Phelps M, Pichot M, Pickenpack M, Piergiovanni F, Pierro V, Pinard L, Pinto IM, Pitkin M, Poeld J, Poggiani R, Poteomkin A, Powell J, Prasad J, Predoi V, Premachandra S, Prestegard T, Price LR, Prijatelj M, Privitera S, Prodi GA, Prokhorov L, Puncken O, Punturo M, Puppo P, Pürrer M, Qin J, Quetschke V, Quintero E, Quitzow-James R, Raab FJ, Rabeling DS, Rácz I, Radkins H, Raffai P, Raja S, Rajalakshmi G, Rakhmanov M, Ramet C, Ramirez K, Rapagnani P, Raymond V, Razzano M, Re V, Recchia S, Reed CM, Regimbau T, Reid S, Reitze DH, Reula O, Rhoades E, Ricci F, Riesen R, Riles K, Robertson NA, Robinet F, Rocchi A, Roddy SB, Rolland L, Rollins JG, Romano R, Romanov G, Romie JH, Rosińska D, Rowan S, Rüdiger A, Ruggi P, Ryan K, Salemi F, Sammut L, Sandberg V, Sanders JR, Sankar S, Sannibale V, Santiago-Prieto I, Saracco E, Sassolas B, Sathyaprakash BS, Saulson PR, Savage R, Scheuer J, Schilling R, Schilman M, Schmidt P, Schnabel R, Schofield RMS, Schreiber E, Schuette D, Schutz BF, Scott J, Scott SM, Sellers D, Sengupta AS, Sentenac D, Sequino V, Sergeev A, Shaddock DA, Shah S, Shahriar MS, Shaltev M, Shao Z, Shapiro B, Shawhan P, Shoemaker DH, Sidery TL, Siellez K, Siemens X, Sigg D, Simakov D, Singer A, Singer L, Singh R, Sintes AM, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith RJE, Smith-Lefebvre ND, Son EJ, Sorazu B, Souradeep T, Staley A, Stebbins J, Steinke M, Steinlechner J, Steinlechner S, Stephens BC, Steplewski S, Stevenson S, Stone R, Stops D, Strain KA, Straniero N, Strigin S, Sturani R, Stuver AL, Summerscales TZ, Susmithan S, Sutton PJ, Swinkels B, Tacca M, Talukder D, Tanner DB, Tao J, Tarabrin SP, Taylor R, Tellez G, Thirugnanasambandam MP, Thomas M, Thomas P, Thorne KA, Thorne KS, Thrane E, Tiwari V, Tokmakov KV, Tomlinson C, Tonelli M, Torres CV, Torrie CI, Travasso F, Traylor G, Tse M, Tshilumba D, Tuennermann H, Ugolini D, Unnikrishnan CS, Urban AL, Usman SA, Vahlbruch H, Vajente G, Valdes G, Vallisneri M, van Beuzekom M, van den Brand JFJ, Van Den Broeck C, van der Sluys MV, van Heijningen J, van Veggel AA, Vass S, Vasúth M, Vaulin R, Vecchio A, Vedovato G, Veitch J, Veitch PJ, Venkateswara K, Verkindt D, Vetrano F, Viceré A, Vincent-Finley R, Vinet JY, Vitale S, Vo T, Vocca H, Vorvick C, Vousden WD, Vyachanin SP, Wade AR, Wade L, Wade M, Walker M, Wallace L, Walsh S, Wang M, Wang X, Ward RL, Was M, Weaver B, Wei LW, Weinert M, Weinstein AJ, Weiss R, Welborn T, Wen L, Wessels P, West M, Westphal T, Wette K, Whelan JT, White DJ, Whiting BF, Wiesner K, Wilkinson C, Williams K, Williams L, Williams R, Williams TD, Williamson AR, Willis JL, Willke B, Wimmer M, Winkler W, Wipf CC, Wiseman AG, Wittel H, Woan G, Wolovick N, Worden J, Wu Y, Yablon J, Yakushin I, Yam W, Yamamoto H, Yancey CC, Yang H, Yoshida S, Yvert M, Zadrożny A, Zanolin M, Zendri JP, Zhang F, Zhang L, Zhao C, Zhu H, Zhu XJ, Zucker ME, Zuraw S, Zweizig J, Aptekar RL, Atteia JL, Cline T, Connaughton V, Frederiks DD, Golenetskii SV, Hurley K, Krimm HA, Marisaldi M, Pal'shin VD, Palmer D, Svinkin DS, Terada Y, von Kienlin A. Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network. Phys Rev Lett 2014; 113:011102. [PMID: 25032916 DOI: 10.1103/physrevlett.113.011102] [Citation(s) in RCA: 10] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/07/2014] [Indexed: 05/21/2023]
Abstract
We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M⊙c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
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Affiliation(s)
- J Aasi
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B P Abbott
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Abbott
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T Abbott
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - M R Abernathy
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - F Acernese
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - K Ackley
- University of Florida, Gainesville, Florida 32611, USA
| | - C Adams
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Adams
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - P Addesso
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - R X Adhikari
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Affeldt
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Agathos
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - N Aggarwal
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - O D Aguiar
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - P Ajith
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bangalore 560012, India
| | - A Alemic
- Syracuse University, Syracuse, New York 13244, USA
| | - B Allen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Allocca
- Università di Siena, I-53100 Siena, Italy and INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - D Amariutei
- University of Florida, Gainesville, Florida 32611, USA
| | - M Andersen
- Stanford University, Stanford, California 94305, USA
| | - R A Anderson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S B Anderson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - W G Anderson
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - K Arai
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M C Araya
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Arceneaux
- The University of Mississippi, University, Mississippi 38677, USA
| | - J S Areeda
- California State University Fullerton, Fullerton, California 92831, USA
| | - S Ast
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S M Aston
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Astone
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - P Aufmuth
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - H Augustus
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - C Aulbert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B E Aylott
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Babak
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - P T Baker
- Montana State University, Bozeman, Montana 59717, USA
| | - G Ballardin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S W Ballmer
- Syracuse University, Syracuse, New York 13244, USA
| | - J C Barayoga
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Barbet
- University of Florida, Gainesville, Florida 32611, USA
| | - B C Barish
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D Barker
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Barone
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - B Barr
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Barsotti
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Barsuglia
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - M A Barton
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - I Bartos
- Columbia University, New York, New York 10027, USA
| | - R Bassiri
- Stanford University, Stanford, California 94305, USA
| | - A Basti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - J C Batch
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Bauchrowitz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Th S Bauer
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - C Baune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Bavigadda
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - B Behnke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | | | - M G Beker
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - C Belczynski
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A S Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Bergmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Bersanetti
- Università degli Studi di Genova, I-16146 Genova, Italy and INFN, Sezione di Genova, I-16146 Genova, Italy
| | - A Bertolini
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J Betzwieser
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - I A Bilenko
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - G Billingsley
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Birch
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Biscans
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Biwer
- Syracuse University, Syracuse, New York 13244, USA
| | - M A Bizouard
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - E Black
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J K Blackburn
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - L Blackburn
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - D Blair
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Bloemen
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - O Bock
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T P Bodiya
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Boer
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G Bogaert
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - C Bogan
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Bond
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - F Bondu
- Institut de Physique de Rennes, CNRS, Université de Rennes 1, F-35042 Rennes, France
| | - L Bonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - R Bonnand
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - R Bork
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Boschi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - Sukanta Bose
- Washington State University, Pullman, Washington 99164, USA and Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - L Bosi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | | | - P R Brady
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
| | - V B Braginsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - M Branchesi
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J E Brau
- University of Oregon, Eugene, Oregon 97403, USA
| | - T Briant
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - D O Bridges
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Brillet
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Brinkmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Brisson
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - A F Brooks
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D A Brown
- Syracuse University, Syracuse, New York 13244, USA
| | - D D Brown
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - F Brückner
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Buchman
- Stanford University, Stanford, California 94305, USA
| | - A Buikema
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Bulik
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - H J Bulten
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | - A Buonanno
- University of Maryland, College Park, Maryland 20742, USA
| | - R Burman
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D Buskulic
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C Buy
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - L Cadonati
- Cardiff University, Cardiff CF24 3AA, United Kingdom and University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - G Cagnoli
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | | | - E Calloni
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J B Camp
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - P Campsie
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - K C Cannon
- Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario, M5S 3H8, Canada
| | - B Canuel
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J Cao
- Tsinghua University, Beijing 100084, China
| | - C D Capano
- University of Maryland, College Park, Maryland 20742, USA
| | - F Carbognani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - L Carbone
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Caride
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - G Castaldi
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Caudill
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Cavaglià
- The University of Mississippi, University, Mississippi 38677, USA
| | - F Cavalier
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - R Cavalieri
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Celerier
- Stanford University, Stanford, California 94305, USA
| | - G Cella
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Cepeda
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E Cesarini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - R Chakraborty
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T Chalermsongsak
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S J Chamberlin
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Chao
- National Tsing Hua University, Hsinchu 300, Taiwan
| | - P Charlton
- Charles Sturt University, Wagga Wagga, New South Wales 2678, Australia
| | - E Chassande-Mottin
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - X Chen
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Chen
- Caltech-CaRT, Pasadena, California 91125, USA
| | | | - A Chiummo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - H S Cho
- Pusan National University, Busan 609-735, Korea
| | - M Cho
- University of Maryland, College Park, Maryland 20742, USA
| | - J H Chow
- Australian National University, Canberra, ACT 0200, Australia
| | | | - Q Chu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S S Y Chua
- Australian National University, Canberra, ACT 0200, Australia
| | - S Chung
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - G Ciani
- University of Florida, Gainesville, Florida 32611, USA
| | - F Clara
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E Clark
- Stanford University, Stanford, California 94305, USA
| | - J A Clark
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - J H Clayton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Cleva
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Coccia
- Università di Roma Tor Vergata, I-00133 Roma, Italy and INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy
| | - P-F Cohadon
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - A Colla
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - C Collette
- University of Brussels, Brussels 1050, Belgium
| | - M Colombini
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - L Cominsky
- Sonoma State University, Rohnert Park, California 94928, USA
| | - M Constancio
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - A Conte
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - D Cook
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T R Corbitt
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Cornish
- Montana State University, Bozeman, Montana 59717, USA
| | - A Corsi
- The George Washington University, Washington, DC 20052, USA
| | - C A Costa
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - M W Coughlin
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - J-P Coulon
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Countryman
- Columbia University, New York, New York 10027, USA
| | - P Couvares
- Syracuse University, Syracuse, New York 13244, USA
| | - D M Coward
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M J Cowart
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D C Coyne
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Coyne
- The George Washington University, Washington, DC 20052, USA
| | - K Craig
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J D E Creighton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - R P Croce
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S G Crowder
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - A Cumming
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Cunningham
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Cuoco
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Cutler
- Caltech-CaRT, Pasadena, California 91125, USA
| | - K Dahl
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Dal Canton
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Damjanic
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S L Danilishin
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S D'Antonio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - V Dattilo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - H Daveloza
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - M Davier
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - G S Davies
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Daw
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - R Day
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - T Dayanga
- Washington State University, Pullman, Washington 99164, USA
| | - D DeBra
- Stanford University, Stanford, California 94305, USA
| | - G Debreczeni
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - J Degallaix
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S Deléglise
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - W Del Pozzo
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - T Denker
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Dent
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - H Dereli
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - V Dergachev
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R De Rosa
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - R T DeRosa
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - R DeSalvo
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Dhurandhar
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - M Díaz
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - J Dickson
- Australian National University, Canberra, ACT 0200, Australia
| | - L Di Fiore
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Di Lieto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - I Di Palma
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | | | - V Dolique
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - E Dominguez
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - F Donovan
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K L Dooley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Doravari
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - R Douglas
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T P Downes
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Drago
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - R W P Drever
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J C Driggers
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - Z Du
- Tsinghua University, Beijing 100084, China
| | - M Ducrot
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - S Dwyer
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T Eberle
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Edo
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M Edwards
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Effler
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - H-B Eggenstein
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Ehrens
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Eichholz
- University of Florida, Gainesville, Florida 32611, USA
| | | | - G Endrőczi
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - R Essick
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Etzel
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Evans
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Evans
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - V Fafone
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Fairhurst
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - X Fan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - Q Fang
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Farinon
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Farr
- Northwestern University, Evanston, Illinois 60208, USA
| | - W M Farr
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Favata
- Montclair State University, Montclair, New Jersey 07043, USA
| | - D Fazi
- Northwestern University, Evanston, Illinois 60208, USA
| | - H Fehrmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M M Fejer
- Stanford University, Stanford, California 94305, USA
| | - D Feldbaum
- University of Florida, Gainesville, Florida 32611, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - F Feroz
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - I Ferrante
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - E C Ferreira
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - F Ferrini
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Fidecaro
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - L S Finn
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - I Fiori
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R P Fisher
- Syracuse University, Syracuse, New York 13244, USA
| | - R Flaminio
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - J-D Fournier
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Franco
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - S Frasca
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - F Frasconi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - M Frede
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Z Frei
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - A Freise
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Frey
- University of Oregon, Eugene, Oregon 97403, USA
| | - T T Fricke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Fritschel
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V V Frolov
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Fulda
- University of Florida, Gainesville, Florida 32611, USA
| | - M Fyffe
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J R Gair
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - L Gammaitoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - S Gaonkar
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - F Garufi
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - N Gehrels
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - G Gemme
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Gendre
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Genin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Gennai
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - S Ghosh
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - J A Giaime
- Louisiana State University, Baton Rouge, Louisiana 70803, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K D Giardina
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Giazotto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - J Gleason
- University of Florida, Gainesville, Florida 32611, USA
| | - E Goetz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Goetz
- University of Florida, Gainesville, Florida 32611, USA
| | - L Gondan
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - G González
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Gordon
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M L Gorodetsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - S Gossan
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Goßler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Gouaty
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C Gräf
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P B Graff
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - M Granata
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - A Grant
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Gras
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - C Gray
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R J S Greenhalgh
- Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom
| | - A M Gretarsson
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - P Groot
- Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - H Grote
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Grover
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Grunewald
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - G M Guidi
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - C J Guido
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Gushwa
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E K Gustafson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Gustafson
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - J Ha
- Seoul National University, Seoul 151-742, Korea
| | - E D Hall
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - W Hamilton
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D Hammer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - G Hammond
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Hanke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Hanks
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Hanna
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA and Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2 L 2Y5, Canada
| | - M D Hannam
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Hanson
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Harms
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G M Harry
- American University, Washington, DC 20016, USA
| | - I W Harry
- Syracuse University, Syracuse, New York 13244, USA
| | - E D Harstad
- University of Oregon, Eugene, Oregon 97403, USA
| | - M Hart
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M T Hartman
- University of Florida, Gainesville, Florida 32611, USA
| | - C-J Haster
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Haughian
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Heidmann
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - M Heintze
- University of Florida, Gainesville, Florida 32611, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H Heitmann
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - P Hello
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - G Hemming
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Hendry
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - I S Heng
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A W Heptonstall
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Heurs
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Hild
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - D Hoak
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - K A Hodge
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D Hofman
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - K Holt
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Hopkins
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - T Horrom
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - D Hoske
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - D J Hosken
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - J Hough
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Howell
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Hu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Huerta
- Syracuse University, Syracuse, New York 13244, USA
| | - B Hughey
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - S Husa
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - S H Huttner
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Huynh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T Huynh-Dinh
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Idrisy
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - D R Ingram
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R Inta
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - G Islas
- California State University Fullerton, Fullerton, California 92831, USA
| | - T Isogai
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ivanov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B R Iyer
- Raman Research Institute, Bangalore, Karnataka 560080, India
| | - K Izumi
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M Jacobson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - H Jang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | | | - Y Ji
- Tsinghua University, Beijing 100084, China
| | | | - W W Johnson
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D I Jones
- University of Southampton, Southampton SO17 1BJ, United Kingdom
| | - R Jones
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R J G Jonker
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - L Ju
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Haris
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - P Kalmus
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kalogera
- Northwestern University, Evanston, Illinois 60208, USA
| | - S Kandhasamy
- The University of Mississippi, University, Mississippi 38677, USA
| | - G Kang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - J B Kanner
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Karlen
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - M Kasprzack
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy and LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - E Katsavounidis
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - W Katzman
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - T Kaur
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Kawabe
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Kawazoe
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Kéfélian
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G M Keiser
- Stanford University, Stanford, California 94305, USA
| | - D Keitel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D B Kelley
- Syracuse University, Syracuse, New York 13244, USA
| | - W Kells
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D G Keppel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Khalaidovski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Y Khalili
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - E A Khazanov
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - C Kim
- Seoul National University, Seoul 151-742, Korea and Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - K Kim
- Hanyang University, Seoul 133-791, Korea
| | - N G Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - N Kim
- Stanford University, Stanford, California 94305, USA
| | - S Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - Y-M Kim
- Pusan National University, Busan 609-735, Korea
| | - E J King
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - P J King
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D L Kinzel
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J S Kissel
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Klimenko
- University of Florida, Gainesville, Florida 32611, USA
| | - J Kline
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Koehlenbeck
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Kokeyama
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - V Kondrashov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S Koranda
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - W Z Korth
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - I Kowalska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - D B Kozak
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kringel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Krishnan
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Królak
- NCBJ, 05-400 Świerk-Otwock, Poland and IM-PAN, 00-956 Warsaw, Poland
| | - G Kuehn
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Kumar
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - D Nanda Kumar
- University of Florida, Gainesville, Florida 32611, USA
| | - P Kumar
- Syracuse University, Syracuse, New York 13244, USA
| | - R Kumar
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Kuo
- National Tsing Hua University, Hsinchu 300, Taiwan
| | | | - P K Lam
- Australian National University, Canberra, ACT 0200, Australia
| | - M Landry
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - B Lantz
- Stanford University, Stanford, California 94305, USA
| | - S Larson
- Northwestern University, Evanston, Illinois 60208, USA
| | - P D Lasky
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - A Lazzarini
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Lazzaro
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Leaci
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - S Leavey
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | | | - C H Lee
- Pusan National University, Busan 609-735, Korea
| | - H K Lee
- Hanyang University, Seoul 133-791, Korea
| | - H M Lee
- Seoul National University, Seoul 151-742, Korea
| | - J Lee
- Hanyang University, Seoul 133-791, Korea
| | - P J Lee
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Leonardi
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - J R Leong
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - I Leonor
- University of Oregon, Eugene, Oregon 97403, USA
| | - A Le Roux
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - N Leroy
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - N Letendre
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - Y Levin
- Monash University, Victoria 3800, Australia
| | - B Levine
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Lewis
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T G F Li
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - K Libbrecht
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - A Libson
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A C Lin
- Stanford University, Stanford, California 94305, USA
| | | | - N A Lockerbie
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - V Lockett
- California State University Fullerton, Fullerton, California 92831, USA
| | - D Lodhia
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Loew
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J Logue
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A L Lombardi
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - E Lopez
- Louisiana Tech University, Ruston, Louisiana 71272, USA
| | - M Lorenzini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - M Lormand
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - G Losurdo
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J Lough
- Syracuse University, Syracuse, New York 13244, USA
| | - M J Lubinski
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - H Lück
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A P Lundgren
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Y Ma
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - E P Macdonald
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - T MacDonald
- Stanford University, Stanford, California 94305, USA
| | - B Machenschalk
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M MacInnis
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D M Macleod
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | | | - R Magee
- Washington State University, Pullman, Washington 99164, USA
| | - M Mageswaran
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Maglione
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - K Mailand
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E Majorana
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | | | - V Malvezzi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - N Man
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G M Manca
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - I Mandel
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - V Mandic
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Mangano
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - N M Mangini
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - G Mansell
- Australian National University, Canberra, ACT 0200, Australia
| | | | - F Marchesoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
| | - F Marion
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - S Márka
- Columbia University, New York, New York 10027, USA
| | - Z Márka
- Columbia University, New York, New York 10027, USA
| | - A Markosyan
- Stanford University, Stanford, California 94305, USA
| | - E Maros
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Marque
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Martelli
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - I W Martin
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R M Martin
- University of Florida, Gainesville, Florida 32611, USA
| | - L Martinelli
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - D Martynov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J N Marx
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - K Mason
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Masserot
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | | | - F Matichard
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - L Matone
- Columbia University, New York, New York 10027, USA
| | - N Mavalvala
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - G May
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Mazumder
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - G Mazzolo
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R McCarthy
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E McClelland
- Australian National University, Canberra, ACT 0200, Australia
| | - S C McGuire
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - G McIntyre
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J McIver
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - K McLin
- Sonoma State University, Rohnert Park, California 94928, USA
| | - D Meacher
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G D Meadors
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - M Mehmet
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Meidam
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - M Meinders
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Melatos
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - G Mendell
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R A Mercer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Meshkov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Messenger
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M S Meyer
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P M Meyers
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - F Mezzani
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - H Miao
- Caltech-CaRT, Pasadena, California 91125, USA
| | - C Michel
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - E E Mikhailov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - L Milano
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J Miller
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Y Minenkov
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - C Mishra
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - S Mitra
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - V P Mitrofanov
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | | | - R Mittleman
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - B Moe
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - A Moggi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - M Mohan
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | | | - D Moraru
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - G Moreno
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - N Morgado
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S R Morriss
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - K Mossavi
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Mours
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C M Mow-Lowry
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C L Mueller
- University of Florida, Gainesville, Florida 32611, USA
| | - G Mueller
- University of Florida, Gainesville, Florida 32611, USA
| | - S Mukherjee
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - A Mullavey
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - J Munch
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - D Murphy
- Columbia University, New York, New York 10027, USA
| | - P G Murray
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Mytidis
- University of Florida, Gainesville, Florida 32611, USA
| | - M F Nagy
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - I Nardecchia
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - L Naticchioni
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R K Nayak
- IISER-Kolkata, Mohanpur, West Bengal 741252, India
| | - V Necula
- University of Florida, Gainesville, Florida 32611, USA
| | - G Nelemans
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - I Neri
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - M Neri
- Università degli Studi di Genova, I-16146 Genova, Italy and INFN, Sezione di Genova, I-16146 Genova, Italy
| | - G Newton
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Nguyen
- Australian National University, Canberra, ACT 0200, Australia
| | - A B Nielsen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Nissanke
- Caltech-CaRT, Pasadena, California 91125, USA
| | - A H Nitz
- Syracuse University, Syracuse, New York 13244, USA
| | - F Nocera
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - D Nolting
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M E N Normandin
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - L K Nuttall
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - E Ochsner
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - J O'Dell
- Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom
| | - E Oelker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J J Oh
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - S H Oh
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - F Ohme
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - S Omar
- Stanford University, Stanford, California 94305, USA
| | - P Oppermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Oram
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B O'Reilly
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Ortega
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - R O'Shaughnessy
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - C Osthelder
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D J Ottaway
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - R S Ottens
- University of Florida, Gainesville, Florida 32611, USA
| | - H Overmier
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B J Owen
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - C Padilla
- California State University Fullerton, Fullerton, California 92831, USA
| | - A Pai
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - O Palashov
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - C Palomba
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - H Pan
- National Tsing Hua University, Hsinchu 300, Taiwan
| | - Y Pan
- University of Maryland, College Park, Maryland 20742, USA
| | - C Pankow
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M A Papa
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - H Paris
- Stanford University, Stanford, California 94305, USA
| | - A Pasqualetti
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Passaquieti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | | | - M Pedraza
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - A Pele
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Penn
- Hobart and William Smith Colleges, Geneva, New York 14456, USA
| | - A Perreca
- Syracuse University, Syracuse, New York 13244, USA
| | - M Phelps
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Pichot
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Pickenpack
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Piergiovanni
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - V Pierro
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - L Pinard
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - I M Pinto
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - M Pitkin
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Poeld
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Poggiani
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - A Poteomkin
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - J Powell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Prasad
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - V Predoi
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | | | - T Prestegard
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - L R Price
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Prijatelj
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S Privitera
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G A Prodi
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - L Prokhorov
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - O Puncken
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - M Punturo
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - P Puppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - M Pürrer
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Qin
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - V Quetschke
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - E Quintero
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | | | - F J Raab
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D S Rabeling
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | - I Rácz
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - H Radkins
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P Raffai
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - S Raja
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - G Rajalakshmi
- Tata Institute for Fundamental Research, Mumbai 400005, India
| | - M Rakhmanov
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - C Ramet
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Ramirez
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - P Rapagnani
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - V Raymond
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Razzano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - V Re
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Recchia
- Università di Roma Tor Vergata, I-00133 Roma, Italy and INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy
| | - C M Reed
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T Regimbau
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Reid
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - D H Reitze
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and University of Florida, Gainesville, Florida 32611, USA
| | - O Reula
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - E Rhoades
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - F Ricci
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R Riesen
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Riles
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - N A Robertson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F Robinet
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - A Rocchi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - S B Roddy
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L Rolland
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - J G Rollins
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Romano
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - G Romanov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - J H Romie
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D Rosińska
- CAMK-PAN, 00-716 Warsaw, Poland and Institute of Astronomy, 65-265 Zielona Góra, Poland
| | - S Rowan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Rüdiger
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Ruggi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Ryan
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Salemi
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - L Sammut
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - V Sandberg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J R Sanders
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - S Sankar
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V Sannibale
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | | | - E Saracco
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - B Sassolas
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | | | - P R Saulson
- Syracuse University, Syracuse, New York 13244, USA
| | - R Savage
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Scheuer
- Northwestern University, Evanston, Illinois 60208, USA
| | - R Schilling
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Schilman
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - P Schmidt
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - R Schnabel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | | | - E Schreiber
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Schuette
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B F Schutz
- Cardiff University, Cardiff CF24 3AA, United Kingdom and Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - J Scott
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S M Scott
- Australian National University, Canberra, ACT 0200, Australia
| | - D Sellers
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A S Sengupta
- Indian Institute of Technology, Gandhinagar, Ahmedabad, Gujarat 382424, India
| | - D Sentenac
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - V Sequino
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Sergeev
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - D A Shaddock
- Australian National University, Canberra, ACT 0200, Australia
| | - S Shah
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - M S Shahriar
- Northwestern University, Evanston, Illinois 60208, USA
| | - M Shaltev
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Z Shao
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B Shapiro
- Stanford University, Stanford, California 94305, USA
| | - P Shawhan
- University of Maryland, College Park, Maryland 20742, USA
| | - D H Shoemaker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T L Sidery
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Siellez
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - X Siemens
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - D Sigg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D Simakov
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Singer
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - L Singer
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Singh
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A M Sintes
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - B J J Slagmolen
- Australian National University, Canberra, ACT 0200, Australia
| | - J Slutsky
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - J R Smith
- California State University Fullerton, Fullerton, California 92831, USA
| | - M R Smith
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R J E Smith
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - N D Smith-Lefebvre
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E J Son
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - B Sorazu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Souradeep
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - A Staley
- Columbia University, New York, New York 10027, USA
| | - J Stebbins
- Stanford University, Stanford, California 94305, USA
| | - M Steinke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - B C Stephens
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Steplewski
- Washington State University, Pullman, Washington 99164, USA
| | - S Stevenson
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Stone
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - D Stops
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K A Strain
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Straniero
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S Strigin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - R Sturani
- Instituto de Física Teórica, Universidade Estadual Paulista/ICTP South American Institute for Fundamental Research, São Paulo, São Paulo 01140-070, Brazil
| | - A L Stuver
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - S Susmithan
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P J Sutton
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B Swinkels
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Tacca
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - D Talukder
- University of Oregon, Eugene, Oregon 97403, USA
| | - D B Tanner
- University of Florida, Gainesville, Florida 32611, USA
| | - J Tao
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S P Tarabrin
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Taylor
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G Tellez
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - M Thomas
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Thomas
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - K A Thorne
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K S Thorne
- Caltech-CaRT, Pasadena, California 91125, USA
| | - E Thrane
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Tiwari
- University of Florida, Gainesville, Florida 32611, USA
| | - K V Tokmakov
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - C Tomlinson
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - C V Torres
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - C I Torrie
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F Travasso
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - G Traylor
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Tse
- Columbia University, New York, New York 10027, USA
| | - D Tshilumba
- University of Brussels, Brussels 1050, Belgium
| | - H Tuennermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Ugolini
- Trinity University, San Antonio, Texas 78212, USA
| | | | - A L Urban
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S A Usman
- Syracuse University, Syracuse, New York 13244, USA
| | - H Vahlbruch
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Vajente
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - G Valdes
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - M van Beuzekom
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J F J van den Brand
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | | | - M V van der Sluys
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | | | - A A van Veggel
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Vass
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Vasúth
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - R Vaulin
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Vecchio
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - G Vedovato
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - J Veitch
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - P J Veitch
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - K Venkateswara
- University of Washington, Seattle, Washington 98195, USA
| | - D Verkindt
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - F Vetrano
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - A Viceré
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - R Vincent-Finley
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - J-Y Vinet
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Vitale
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Vo
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - H Vocca
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - C Vorvick
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - W D Vousden
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S P Vyachanin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - A R Wade
- Australian National University, Canberra, ACT 0200, Australia
| | - L Wade
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Wade
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Walker
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - L Wallace
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S Walsh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Wang
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - X Wang
- Tsinghua University, Beijing 100084, China
| | - R L Ward
- Australian National University, Canberra, ACT 0200, Australia
| | - M Was
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Weaver
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - L-W Wei
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Weinert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A J Weinstein
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Weiss
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Welborn
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L Wen
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P Wessels
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M West
- Syracuse University, Syracuse, New York 13244, USA
| | - T Westphal
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Wette
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J T Whelan
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - D J White
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - B F Whiting
- University of Florida, Gainesville, Florida 32611, USA
| | - K Wiesner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Wilkinson
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - K Williams
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - L Williams
- University of Florida, Gainesville, Florida 32611, USA
| | - R Williams
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T D Williams
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | | | - J L Willis
- Abilene Christian University, Abilene, Texas 79699, USA
| | - B Willke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M Wimmer
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - W Winkler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C C Wipf
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A G Wiseman
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - H Wittel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - G Woan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Wolovick
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - J Worden
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - Y Wu
- University of Florida, Gainesville, Florida 32611, USA
| | - J Yablon
- Northwestern University, Evanston, Illinois 60208, USA
| | - I Yakushin
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Yam
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - H Yamamoto
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C C Yancey
- University of Maryland, College Park, Maryland 20742, USA
| | - H Yang
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Yoshida
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | - M Yvert
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | | | - M Zanolin
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J-P Zendri
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - Fan Zhang
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA and Tsinghua University, Beijing 100084, China
| | - L Zhang
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Zhao
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - H Zhu
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - X J Zhu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M E Zucker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S Zuraw
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - J Zweizig
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R L Aptekar
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - J L Atteia
- Université de Toulouse, UPS-OMP, IRAP, Toulouse, France and CNRS, IRAP, 14, Avenue Edouard Belin, F-31400 Toulouse, France
| | - T Cline
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - V Connaughton
- CSPAR, University of Alabama in Huntsville, Huntsville, Alabama 35899, USA
| | - D D Frederiks
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - S V Golenetskii
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - K Hurley
- University of California-Berkeley, Space Sciences Lab, 7 Gauss Way, Berkeley, California 94720, USA
| | - H A Krimm
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA and Universities Space Research Association, 7178 Columbia Gateway Drive Columbia, Maryland 21046, USA
| | - M Marisaldi
- INAF-IASF Bologna, Via Piero Gobetti 101, 40129 Bologna, Italy
| | - V D Pal'shin
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation and Saint Petersburg State Polytechnical University, 195251, Saint Petersburg, Russia
| | - D Palmer
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - D S Svinkin
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - Y Terada
- Graduate School of Science and Engineering, Saitama University, Saitama City, Japan
| | - A von Kienlin
- Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany
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Aasi J, Abbott BP, Abbott R, Abbott T, Abernathy MR, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, Affeldt C, Agathos M, Aggarwal N, Aguiar OD, Ajith P, Alemic A, Allen B, Allocca A, Amariutei D, Andersen M, Anderson RA, Anderson SB, Anderson WG, Arai K, Araya MC, Arceneaux C, Areeda JS, Ast S, Aston SM, Astone P, Aufmuth P, Augustus H, Aulbert C, Aylott BE, Babak S, Baker PT, Ballardin G, Ballmer SW, Barayoga JC, Barbet M, Barish BC, Barker D, Barone F, Barr B, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Basti A, Batch JC, Bauchrowitz J, Bauer TS, Baune C, Bavigadda V, Behnke B, Bejger M, Beker MG, Belczynski C, Bell AS, Bell C, Bergmann G, Bersanetti D, Bertolini A, Betzwieser J, Bilenko IA, Billingsley G, Birch J, Biscans S, Bitossi M, Biwer C, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bloemen S, Bock O, Bodiya TP, Boer M, Bogaert G, Bogan C, Bond C, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Boschi V, Bose S, Bosi L, Bradaschia C, Brady PR, Braginsky VB, Branchesi M, Brau JE, Briant T, Bridges DO, Brillet A, Brinkmann M, Brisson V, Brooks AF, Brown DA, Brown DD, Brückner F, Buchman S, Buikema A, Bulik T, Bulten HJ, Buonanno A, Burman R, Buskulic D, Buy C, Cadonati L, Cagnoli G, Calderón Bustillo J, Calloni E, Camp JB, Campsie P, Cannon KC, Canuel B, Cao J, Capano CD, Carbognani F, Carbone L, Caride S, Castaldi G, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Celerier C, Cella G, Cepeda C, Cesarini E, Chakraborty R, Chalermsongsak T, Chamberlin SJ, Chao S, Charlton P, Chassande-Mottin E, Chen X, Chen Y, Chincarini A, Chiummo A, Cho HS, Cho M, Chow JH, Christensen N, Chu Q, Chua SSY, Chung S, Ciani G, Clara F, Clark DE, Clark JA, Clayton JH, Cleva F, Coccia E, Cohadon PF, Colla A, Collette C, Colombini M, Cominsky L, Constancio M, Conte A, Cook D, Corbitt TR, Cornish N, Corsi A, Costa CA, Coughlin MW, Coulon JP, Countryman S, Couvares P, Coward DM, Cowart MJ, Coyne DC, Coyne R, Craig K, Creighton JDE, Croce RP, Crowder SG, Cumming A, Cunningham L, Cuoco E, Cutler C, Dahl K, Dal Canton T, Damjanic M, Danilishin SL, D'Antonio S, Danzmann K, Dattilo V, Daveloza H, Davier M, Davies GS, Daw EJ, Day R, Dayanga T, DeBra D, Debreczeni G, Degallaix J, Deléglise S, Del Pozzo W, Denker T, Dent T, Dereli H, Dergachev V, De Rosa R, DeRosa RT, DeSalvo R, Dhurandhar S, Díaz M, Dickson J, Di Fiore L, Di Lieto A, Di Palma I, Di Virgilio A, Dolique V, Dominguez E, Donovan F, Dooley KL, Doravari S, Douglas R, Downes TP, Drago M, Drever RWP, Driggers JC, Du Z, Ducrot M, Dwyer S, Eberle T, Edo T, Edwards M, Effler A, Eggenstein HB, Ehrens P, Eichholz J, Eikenberry SS, Endrőczi G, Essick R, Etzel T, Evans M, Evans T, Factourovich M, Fafone V, Fairhurst S, Fan X, Fang Q, Farinon S, Farr B, Farr WM, Favata M, Fazi D, Fehrmann H, Fejer MM, Feldbaum D, Feroz F, Ferrante I, Ferreira EC, Ferrini F, Fidecaro F, Finn LS, Fiori I, Fisher RP, Flaminio R, Fournier JD, Franco S, Frasca S, Frasconi F, Frede M, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fulda P, Fyffe M, Gair JR, Gammaitoni L, Gaonkar S, Garufi F, Gehrels N, Gemme G, Gendre B, Genin E, Gennai A, Ghosh S, Giaime JA, Giardina KD, Giazotto A, Gleason J, Goetz E, Goetz R, Gondan L, González G, Gordon N, Gorodetsky ML, Gossan S, Goßler S, Gouaty R, Gräf C, Graff PB, Granata M, Grant A, Gras S, Gray C, Greenhalgh RJS, Gretarsson AM, Groot P, Grote H, Grover K, Grunewald S, Guidi GM, Guido CJ, Gushwa K, Gustafson EK, Gustafson R, Ha J, Hall ED, Hamilton W, Hammer D, Hammond G, Hanke M, Hanks J, Hanna C, Hannam MD, Hanson J, Harms J, Harry GM, Harry IW, Harstad ED, Hart M, Hartman MT, Haster CJ, Haughian K, Heidmann A, Heintze M, Heitmann H, Hello P, Hemming G, Hendry M, Heng IS, Heptonstall AW, Heurs M, Hewitson M, Hild S, Hoak D, Hodge KA, Hofman D, Holt K, Hopkins P, Horrom T, Hoske D, Hosken DJ, Hough J, Howell EJ, Hu Y, Huerta E, Hughey B, Husa S, Huttner SH, Huynh M, Huynh-Dinh T, Idrisy A, Ingram DR, Inta R, Islas G, Isogai T, Ivanov A, Iyer BR, Izumi K, Jacobson M, Jang H, Jaranowski P, Ji Y, Jiménez-Forteza F, Johnson WW, Jones DI, Jones R, Jonker RJG, Ju L, Haris K, Kalmus P, Kalogera V, Kandhasamy S, Kang G, Kanner JB, Karlen J, Kasprzack M, Katsavounidis E, Katzman W, Kaufer H, Kaufer S, Kaur T, Kawabe K, Kawazoe F, Kéfélian F, Keiser GM, Keitel D, Kelley DB, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khazanov EA, Kim C, Kim K, Kim NG, Kim N, Kim S, Kim YM, King EJ, King PJ, Kinzel DL, Kissel JS, Klimenko S, Kline J, Koehlenbeck S, Kokeyama K, Kondrashov V, Koranda S, Korth WZ, Kowalska I, Kozak DB, Kringel V, Krishnan B, Królak A, Kuehn G, Kumar A, Kumar DN, Kumar P, Kumar R, Kuo L, Kutynia A, Lam PK, Landry M, Lantz B, Larson S, Lasky PD, Lazzarini A, Lazzaro C, Leaci P, Leavey S, Lebigot EO, Lee CH, Lee HK, Lee HM, Lee J, Lee PJ, Leonardi M, Leong JR, Leonor I, Le Roux A, Leroy N, Letendre N, Levin Y, Levine B, Lewis J, Li TGF, Libbrecht K, Libson A, Lin AC, Littenberg TB, Lockerbie NA, Lockett V, Lodhia D, Loew K, Logue J, Lombardi AL, Lopez E, Lorenzini M, Loriette V, Lormand M, Losurdo G, Lough J, Lubinski MJ, Lück H, Lundgren AP, Ma Y, Macdonald EP, MacDonald T, Machenschalk B, MacInnis M, Macleod DM, Magaña-Sandoval F, Magee R, Mageswaran M, Maglione C, Mailand K, Majorana E, Maksimovic I, Malvezzi V, Man N, Manca GM, Mandel I, Mandic V, Mangano V, Mangini NM, Mansell G, Mantovani M, Marchesoni F, Marion F, Márka S, Márka Z, Markosyan A, Maros E, Marque J, Martelli F, Martin IW, Martin RM, Martinelli L, Martynov D, Marx JN, Mason K, Masserot A, Massinger TJ, Matichard F, Matone L, Mavalvala N, May G, Mazumder N, Mazzolo G, McCarthy R, McClelland DE, McGuire SC, McIntyre G, McIver J, McLin K, Meacher D, Meadors GD, Mehmet M, Meidam J, Meinders M, Melatos A, Mendell G, Mercer RA, Meshkov S, Messenger C, Meyer MS, Meyers PM, Mezzani F, Miao H, Michel C, Mikhailov EE, Milano L, Miller J, Minenkov Y, Mingarelli CMF, Mishra C, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Moe B, Moggi A, Mohan M, Mohapatra SRP, Moraru D, Moreno G, Morgado N, Morriss SR, Mossavi K, Mours B, Mow-Lowry CM, Mueller CL, Mueller G, Mukherjee S, Mullavey A, Munch J, Murphy D, Murray PG, Mytidis A, Nagy MF, Nardecchia I, Naticchioni L, Nayak RK, Necula V, Nelemans G, Neri I, Neri M, Newton G, Nguyen T, Nielsen AB, Nissanke S, Nitz AH, Nocera F, Nolting D, Normandin MEN, Nuttall LK, Ochsner E, O'Dell J, Oelker E, Oh JJ, Oh SH, Ohme F, Omar S, Oppermann P, Oram R, O'Reilly B, Ortega W, O'Shaughnessy R, Osthelder C, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Padilla C, Pai A, Palashov O, Palomba C, Pan H, Pan Y, Pankow C, Paoletti F, Papa MA, Paris H, Pasqualetti A, Passaquieti R, Passuello D, Pedraza M, Pele A, Penn S, Perreca A, Phelps M, Pichot M, Pickenpack M, Piergiovanni F, Pierro V, Pinard L, Pinto IM, Pitkin M, Poeld J, Poggiani R, Poteomkin A, Powell J, Prasad J, Predoi V, Premachandra S, Prestegard T, Price LR, Prijatelj M, Privitera S, Prodi GA, Prokhorov L, Puncken O, Punturo M, Puppo P, Pürrer M, Qin J, Quetschke V, Quintero E, Quitzow-James R, Raab FJ, Rabeling DS, Rácz I, Radkins H, Raffai P, Raja S, Rajalakshmi G, Rakhmanov M, Ramet C, Ramirez K, Rapagnani P, Raymond V, Razzano M, Re V, Recchia S, Reed CM, Regimbau T, Reid S, Reitze DH, Reula O, Rhoades E, Ricci F, Riesen R, Riles K, Robertson NA, Robinet F, Rocchi A, Roddy SB, Rolland L, Rollins JG, Romano R, Romanov G, Romie JH, Rosińska D, Rowan S, Rüdiger A, Ruggi P, Ryan K, Salemi F, Sammut L, Sandberg V, Sanders JR, Sankar S, Sannibale V, Santiago-Prieto I, Saracco E, Sassolas B, Sathyaprakash BS, Saulson PR, Savage R, Scheuer J, Schilling R, Schilman M, Schmidt P, Schnabel R, Schofield RMS, Schreiber E, Schuette D, Schutz BF, Scott J, Scott SM, Sellers D, Sengupta AS, Sentenac D, Sequino V, Sergeev A, Shaddock DA, Shah S, Shahriar MS, Shaltev M, Shao Z, Shapiro B, Shawhan P, Shoemaker DH, Sidery TL, Siellez K, Siemens X, Sigg D, Simakov D, Singer A, Singer L, Singh R, Sintes AM, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith RJE, Smith-Lefebvre ND, Son EJ, Sorazu B, Souradeep T, Staley A, Stebbins J, Steinke M, Steinlechner J, Steinlechner S, Stephens BC, Steplewski S, Stevenson S, Stone R, Stops D, Strain KA, Straniero N, Strigin S, Sturani R, Stuver AL, Summerscales TZ, Susmithan S, Sutton PJ, Swinkels B, Tacca M, Talukder D, Tanner DB, Tao J, Tarabrin SP, Taylor R, Tellez G, Thirugnanasambandam MP, Thomas M, Thomas P, Thorne KA, Thorne KS, Thrane E, Tiwari V, Tokmakov KV, Tomlinson C, Tonelli M, Torres CV, Torrie CI, Travasso F, Traylor G, Tse M, Tshilumba D, Tuennermann H, Ugolini D, Unnikrishnan CS, Urban AL, Usman SA, Vahlbruch H, Vajente G, Valdes G, Vallisneri M, van Beuzekom M, van den Brand JFJ, Van Den Broeck C, van der Sluys MV, van Heijningen J, van Veggel AA, Vass S, Vasúth M, Vaulin R, Vecchio A, Vedovato G, Veitch J, Veitch PJ, Venkateswara K, Verkindt D, Vetrano F, Viceré A, Vincent-Finley R, Vinet JY, Vitale S, Vo T, Vocca H, Vorvick C, Vousden WD, Vyachanin SP, Wade AR, Wade L, Wade M, Walker M, Wallace L, Walsh S, Wang M, Wang X, Ward RL, Was M, Weaver B, Wei LW, Weinert M, Weinstein AJ, Weiss R, Welborn T, Wen L, Wessels P, West M, Westphal T, Wette K, Whelan JT, White DJ, Whiting BF, Wiesner K, Wilkinson C, Williams K, Williams L, Williams R, Williams TD, Williamson AR, Willis JL, Willke B, Wimmer M, Winkler W, Wipf CC, Wiseman AG, Wittel H, Woan G, Wolovick N, Worden J, Wu Y, Yablon J, Yakushin I, Yam W, Yamamoto H, Yancey CC, Yang H, Yoshida S, Yvert M, Zadrożny A, Zanolin M, Zendri JP, Zhang F, Zhang L, Zhao C, Zhu H, Zhu XJ, Zucker ME, Zuraw S, Zweizig J, Aptekar RL, Atteia JL, Cline T, Connaughton V, Frederiks DD, Golenetskii SV, Hurley K, Krimm HA, Marisaldi M, Pal'shin VD, Palmer D, Svinkin DS, Terada Y, von Kienlin A. Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network. Phys Rev Lett 2014; 113:011102. [PMID: 25032916 DOI: 10.1103/physrevd.89.122004] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/07/2014] [Indexed: 05/21/2023]
Abstract
We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M⊙c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
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Affiliation(s)
- J Aasi
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B P Abbott
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Abbott
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T Abbott
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - M R Abernathy
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - F Acernese
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - K Ackley
- University of Florida, Gainesville, Florida 32611, USA
| | - C Adams
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Adams
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - P Addesso
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - R X Adhikari
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Affeldt
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Agathos
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - N Aggarwal
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - O D Aguiar
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - P Ajith
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bangalore 560012, India
| | - A Alemic
- Syracuse University, Syracuse, New York 13244, USA
| | - B Allen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Allocca
- Università di Siena, I-53100 Siena, Italy and INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - D Amariutei
- University of Florida, Gainesville, Florida 32611, USA
| | - M Andersen
- Stanford University, Stanford, California 94305, USA
| | - R A Anderson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S B Anderson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - W G Anderson
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - K Arai
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M C Araya
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Arceneaux
- The University of Mississippi, University, Mississippi 38677, USA
| | - J S Areeda
- California State University Fullerton, Fullerton, California 92831, USA
| | - S Ast
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S M Aston
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Astone
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - P Aufmuth
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - H Augustus
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - C Aulbert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B E Aylott
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Babak
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - P T Baker
- Montana State University, Bozeman, Montana 59717, USA
| | - G Ballardin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S W Ballmer
- Syracuse University, Syracuse, New York 13244, USA
| | - J C Barayoga
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Barbet
- University of Florida, Gainesville, Florida 32611, USA
| | - B C Barish
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D Barker
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Barone
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - B Barr
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Barsotti
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Barsuglia
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - M A Barton
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - I Bartos
- Columbia University, New York, New York 10027, USA
| | - R Bassiri
- Stanford University, Stanford, California 94305, USA
| | - A Basti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - J C Batch
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Bauchrowitz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Th S Bauer
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - C Baune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Bavigadda
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - B Behnke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | | | - M G Beker
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - C Belczynski
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A S Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Bergmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Bersanetti
- Università degli Studi di Genova, I-16146 Genova, Italy and INFN, Sezione di Genova, I-16146 Genova, Italy
| | - A Bertolini
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J Betzwieser
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - I A Bilenko
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - G Billingsley
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Birch
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Biscans
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Biwer
- Syracuse University, Syracuse, New York 13244, USA
| | - M A Bizouard
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - E Black
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J K Blackburn
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - L Blackburn
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - D Blair
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Bloemen
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - O Bock
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T P Bodiya
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Boer
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G Bogaert
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - C Bogan
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Bond
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - F Bondu
- Institut de Physique de Rennes, CNRS, Université de Rennes 1, F-35042 Rennes, France
| | - L Bonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - R Bonnand
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - R Bork
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Boschi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - Sukanta Bose
- Washington State University, Pullman, Washington 99164, USA and Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - L Bosi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | | | - P R Brady
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
| | - V B Braginsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - M Branchesi
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J E Brau
- University of Oregon, Eugene, Oregon 97403, USA
| | - T Briant
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - D O Bridges
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Brillet
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Brinkmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Brisson
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - A F Brooks
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D A Brown
- Syracuse University, Syracuse, New York 13244, USA
| | - D D Brown
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - F Brückner
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Buchman
- Stanford University, Stanford, California 94305, USA
| | - A Buikema
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Bulik
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - H J Bulten
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | - A Buonanno
- University of Maryland, College Park, Maryland 20742, USA
| | - R Burman
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D Buskulic
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C Buy
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - L Cadonati
- Cardiff University, Cardiff CF24 3AA, United Kingdom and University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - G Cagnoli
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | | | - E Calloni
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J B Camp
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - P Campsie
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - K C Cannon
- Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario, M5S 3H8, Canada
| | - B Canuel
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J Cao
- Tsinghua University, Beijing 100084, China
| | - C D Capano
- University of Maryland, College Park, Maryland 20742, USA
| | - F Carbognani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - L Carbone
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Caride
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - G Castaldi
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Caudill
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Cavaglià
- The University of Mississippi, University, Mississippi 38677, USA
| | - F Cavalier
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - R Cavalieri
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Celerier
- Stanford University, Stanford, California 94305, USA
| | - G Cella
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Cepeda
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E Cesarini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - R Chakraborty
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T Chalermsongsak
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S J Chamberlin
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Chao
- National Tsing Hua University, Hsinchu 300, Taiwan
| | - P Charlton
- Charles Sturt University, Wagga Wagga, New South Wales 2678, Australia
| | - E Chassande-Mottin
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - X Chen
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Chen
- Caltech-CaRT, Pasadena, California 91125, USA
| | | | - A Chiummo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - H S Cho
- Pusan National University, Busan 609-735, Korea
| | - M Cho
- University of Maryland, College Park, Maryland 20742, USA
| | - J H Chow
- Australian National University, Canberra, ACT 0200, Australia
| | | | - Q Chu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S S Y Chua
- Australian National University, Canberra, ACT 0200, Australia
| | - S Chung
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - G Ciani
- University of Florida, Gainesville, Florida 32611, USA
| | - F Clara
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E Clark
- Stanford University, Stanford, California 94305, USA
| | - J A Clark
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - J H Clayton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Cleva
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Coccia
- Università di Roma Tor Vergata, I-00133 Roma, Italy and INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy
| | - P-F Cohadon
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - A Colla
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - C Collette
- University of Brussels, Brussels 1050, Belgium
| | - M Colombini
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - L Cominsky
- Sonoma State University, Rohnert Park, California 94928, USA
| | - M Constancio
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - A Conte
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - D Cook
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T R Corbitt
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Cornish
- Montana State University, Bozeman, Montana 59717, USA
| | - A Corsi
- The George Washington University, Washington, DC 20052, USA
| | - C A Costa
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - M W Coughlin
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - J-P Coulon
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Countryman
- Columbia University, New York, New York 10027, USA
| | - P Couvares
- Syracuse University, Syracuse, New York 13244, USA
| | - D M Coward
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M J Cowart
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D C Coyne
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Coyne
- The George Washington University, Washington, DC 20052, USA
| | - K Craig
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J D E Creighton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - R P Croce
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S G Crowder
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - A Cumming
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Cunningham
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Cuoco
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Cutler
- Caltech-CaRT, Pasadena, California 91125, USA
| | - K Dahl
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Dal Canton
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Damjanic
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S L Danilishin
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S D'Antonio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - V Dattilo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - H Daveloza
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - M Davier
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - G S Davies
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Daw
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - R Day
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - T Dayanga
- Washington State University, Pullman, Washington 99164, USA
| | - D DeBra
- Stanford University, Stanford, California 94305, USA
| | - G Debreczeni
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - J Degallaix
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S Deléglise
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - W Del Pozzo
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - T Denker
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Dent
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - H Dereli
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - V Dergachev
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R De Rosa
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - R T DeRosa
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - R DeSalvo
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Dhurandhar
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - M Díaz
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - J Dickson
- Australian National University, Canberra, ACT 0200, Australia
| | - L Di Fiore
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Di Lieto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - I Di Palma
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | | | - V Dolique
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - E Dominguez
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - F Donovan
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K L Dooley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Doravari
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - R Douglas
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T P Downes
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Drago
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - R W P Drever
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J C Driggers
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - Z Du
- Tsinghua University, Beijing 100084, China
| | - M Ducrot
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - S Dwyer
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T Eberle
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Edo
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M Edwards
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Effler
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - H-B Eggenstein
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Ehrens
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Eichholz
- University of Florida, Gainesville, Florida 32611, USA
| | | | - G Endrőczi
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - R Essick
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Etzel
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Evans
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Evans
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - V Fafone
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Fairhurst
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - X Fan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - Q Fang
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Farinon
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Farr
- Northwestern University, Evanston, Illinois 60208, USA
| | - W M Farr
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Favata
- Montclair State University, Montclair, New Jersey 07043, USA
| | - D Fazi
- Northwestern University, Evanston, Illinois 60208, USA
| | - H Fehrmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M M Fejer
- Stanford University, Stanford, California 94305, USA
| | - D Feldbaum
- University of Florida, Gainesville, Florida 32611, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - F Feroz
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - I Ferrante
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - E C Ferreira
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - F Ferrini
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Fidecaro
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - L S Finn
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - I Fiori
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R P Fisher
- Syracuse University, Syracuse, New York 13244, USA
| | - R Flaminio
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - J-D Fournier
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Franco
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - S Frasca
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - F Frasconi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - M Frede
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Z Frei
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - A Freise
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Frey
- University of Oregon, Eugene, Oregon 97403, USA
| | - T T Fricke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Fritschel
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V V Frolov
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Fulda
- University of Florida, Gainesville, Florida 32611, USA
| | - M Fyffe
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J R Gair
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - L Gammaitoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - S Gaonkar
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - F Garufi
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - N Gehrels
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - G Gemme
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Gendre
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Genin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Gennai
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - S Ghosh
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - J A Giaime
- Louisiana State University, Baton Rouge, Louisiana 70803, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K D Giardina
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Giazotto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - J Gleason
- University of Florida, Gainesville, Florida 32611, USA
| | - E Goetz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Goetz
- University of Florida, Gainesville, Florida 32611, USA
| | - L Gondan
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - G González
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Gordon
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M L Gorodetsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - S Gossan
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Goßler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Gouaty
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C Gräf
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P B Graff
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - M Granata
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - A Grant
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Gras
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - C Gray
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R J S Greenhalgh
- Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom
| | - A M Gretarsson
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - P Groot
- Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - H Grote
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Grover
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Grunewald
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - G M Guidi
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - C J Guido
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Gushwa
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E K Gustafson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Gustafson
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - J Ha
- Seoul National University, Seoul 151-742, Korea
| | - E D Hall
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - W Hamilton
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D Hammer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - G Hammond
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Hanke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Hanks
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Hanna
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA and Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2 L 2Y5, Canada
| | - M D Hannam
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Hanson
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Harms
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G M Harry
- American University, Washington, DC 20016, USA
| | - I W Harry
- Syracuse University, Syracuse, New York 13244, USA
| | - E D Harstad
- University of Oregon, Eugene, Oregon 97403, USA
| | - M Hart
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M T Hartman
- University of Florida, Gainesville, Florida 32611, USA
| | - C-J Haster
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Haughian
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Heidmann
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - M Heintze
- University of Florida, Gainesville, Florida 32611, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H Heitmann
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - P Hello
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - G Hemming
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Hendry
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - I S Heng
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A W Heptonstall
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Heurs
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Hild
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - D Hoak
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - K A Hodge
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D Hofman
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - K Holt
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Hopkins
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - T Horrom
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - D Hoske
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - D J Hosken
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - J Hough
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Howell
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Hu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Huerta
- Syracuse University, Syracuse, New York 13244, USA
| | - B Hughey
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - S Husa
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - S H Huttner
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Huynh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T Huynh-Dinh
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Idrisy
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - D R Ingram
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R Inta
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - G Islas
- California State University Fullerton, Fullerton, California 92831, USA
| | - T Isogai
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ivanov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B R Iyer
- Raman Research Institute, Bangalore, Karnataka 560080, India
| | - K Izumi
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M Jacobson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - H Jang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | | | - Y Ji
- Tsinghua University, Beijing 100084, China
| | | | - W W Johnson
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D I Jones
- University of Southampton, Southampton SO17 1BJ, United Kingdom
| | - R Jones
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R J G Jonker
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - L Ju
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Haris
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - P Kalmus
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kalogera
- Northwestern University, Evanston, Illinois 60208, USA
| | - S Kandhasamy
- The University of Mississippi, University, Mississippi 38677, USA
| | - G Kang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - J B Kanner
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Karlen
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - M Kasprzack
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy and LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - E Katsavounidis
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - W Katzman
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - T Kaur
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Kawabe
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Kawazoe
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Kéfélian
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G M Keiser
- Stanford University, Stanford, California 94305, USA
| | - D Keitel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D B Kelley
- Syracuse University, Syracuse, New York 13244, USA
| | - W Kells
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D G Keppel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Khalaidovski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Y Khalili
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - E A Khazanov
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - C Kim
- Seoul National University, Seoul 151-742, Korea and Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - K Kim
- Hanyang University, Seoul 133-791, Korea
| | - N G Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - N Kim
- Stanford University, Stanford, California 94305, USA
| | - S Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - Y-M Kim
- Pusan National University, Busan 609-735, Korea
| | - E J King
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - P J King
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D L Kinzel
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J S Kissel
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Klimenko
- University of Florida, Gainesville, Florida 32611, USA
| | - J Kline
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Koehlenbeck
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Kokeyama
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - V Kondrashov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S Koranda
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - W Z Korth
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - I Kowalska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - D B Kozak
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kringel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Krishnan
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Królak
- NCBJ, 05-400 Świerk-Otwock, Poland and IM-PAN, 00-956 Warsaw, Poland
| | - G Kuehn
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Kumar
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - D Nanda Kumar
- University of Florida, Gainesville, Florida 32611, USA
| | - P Kumar
- Syracuse University, Syracuse, New York 13244, USA
| | - R Kumar
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Kuo
- National Tsing Hua University, Hsinchu 300, Taiwan
| | | | - P K Lam
- Australian National University, Canberra, ACT 0200, Australia
| | - M Landry
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - B Lantz
- Stanford University, Stanford, California 94305, USA
| | - S Larson
- Northwestern University, Evanston, Illinois 60208, USA
| | - P D Lasky
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - A Lazzarini
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Lazzaro
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Leaci
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - S Leavey
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | | | - C H Lee
- Pusan National University, Busan 609-735, Korea
| | - H K Lee
- Hanyang University, Seoul 133-791, Korea
| | - H M Lee
- Seoul National University, Seoul 151-742, Korea
| | - J Lee
- Hanyang University, Seoul 133-791, Korea
| | - P J Lee
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Leonardi
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - J R Leong
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - I Leonor
- University of Oregon, Eugene, Oregon 97403, USA
| | - A Le Roux
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - N Leroy
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - N Letendre
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - Y Levin
- Monash University, Victoria 3800, Australia
| | - B Levine
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Lewis
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T G F Li
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - K Libbrecht
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - A Libson
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A C Lin
- Stanford University, Stanford, California 94305, USA
| | | | - N A Lockerbie
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - V Lockett
- California State University Fullerton, Fullerton, California 92831, USA
| | - D Lodhia
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Loew
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J Logue
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A L Lombardi
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - E Lopez
- Louisiana Tech University, Ruston, Louisiana 71272, USA
| | - M Lorenzini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - M Lormand
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - G Losurdo
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J Lough
- Syracuse University, Syracuse, New York 13244, USA
| | - M J Lubinski
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - H Lück
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A P Lundgren
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Y Ma
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - E P Macdonald
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - T MacDonald
- Stanford University, Stanford, California 94305, USA
| | - B Machenschalk
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M MacInnis
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D M Macleod
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | | | - R Magee
- Washington State University, Pullman, Washington 99164, USA
| | - M Mageswaran
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Maglione
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - K Mailand
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E Majorana
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | | | - V Malvezzi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - N Man
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G M Manca
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - I Mandel
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - V Mandic
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Mangano
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - N M Mangini
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - G Mansell
- Australian National University, Canberra, ACT 0200, Australia
| | | | - F Marchesoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
| | - F Marion
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - S Márka
- Columbia University, New York, New York 10027, USA
| | - Z Márka
- Columbia University, New York, New York 10027, USA
| | - A Markosyan
- Stanford University, Stanford, California 94305, USA
| | - E Maros
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Marque
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Martelli
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - I W Martin
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R M Martin
- University of Florida, Gainesville, Florida 32611, USA
| | - L Martinelli
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - D Martynov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J N Marx
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - K Mason
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Masserot
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | | | - F Matichard
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - L Matone
- Columbia University, New York, New York 10027, USA
| | - N Mavalvala
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - G May
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Mazumder
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - G Mazzolo
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R McCarthy
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E McClelland
- Australian National University, Canberra, ACT 0200, Australia
| | - S C McGuire
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - G McIntyre
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J McIver
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - K McLin
- Sonoma State University, Rohnert Park, California 94928, USA
| | - D Meacher
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G D Meadors
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - M Mehmet
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Meidam
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - M Meinders
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Melatos
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - G Mendell
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R A Mercer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Meshkov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Messenger
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M S Meyer
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P M Meyers
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - F Mezzani
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - H Miao
- Caltech-CaRT, Pasadena, California 91125, USA
| | - C Michel
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - E E Mikhailov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - L Milano
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J Miller
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Y Minenkov
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - C Mishra
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - S Mitra
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - V P Mitrofanov
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | | | - R Mittleman
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - B Moe
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - A Moggi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - M Mohan
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | | | - D Moraru
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - G Moreno
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - N Morgado
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S R Morriss
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - K Mossavi
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Mours
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C M Mow-Lowry
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C L Mueller
- University of Florida, Gainesville, Florida 32611, USA
| | - G Mueller
- University of Florida, Gainesville, Florida 32611, USA
| | - S Mukherjee
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - A Mullavey
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - J Munch
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - D Murphy
- Columbia University, New York, New York 10027, USA
| | - P G Murray
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Mytidis
- University of Florida, Gainesville, Florida 32611, USA
| | - M F Nagy
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - I Nardecchia
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - L Naticchioni
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R K Nayak
- IISER-Kolkata, Mohanpur, West Bengal 741252, India
| | - V Necula
- University of Florida, Gainesville, Florida 32611, USA
| | - G Nelemans
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - I Neri
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - M Neri
- Università degli Studi di Genova, I-16146 Genova, Italy and INFN, Sezione di Genova, I-16146 Genova, Italy
| | - G Newton
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Nguyen
- Australian National University, Canberra, ACT 0200, Australia
| | - A B Nielsen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Nissanke
- Caltech-CaRT, Pasadena, California 91125, USA
| | - A H Nitz
- Syracuse University, Syracuse, New York 13244, USA
| | - F Nocera
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - D Nolting
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M E N Normandin
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - L K Nuttall
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - E Ochsner
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - J O'Dell
- Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom
| | - E Oelker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J J Oh
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - S H Oh
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - F Ohme
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - S Omar
- Stanford University, Stanford, California 94305, USA
| | - P Oppermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Oram
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B O'Reilly
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Ortega
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - R O'Shaughnessy
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - C Osthelder
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D J Ottaway
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - R S Ottens
- University of Florida, Gainesville, Florida 32611, USA
| | - H Overmier
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B J Owen
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - C Padilla
- California State University Fullerton, Fullerton, California 92831, USA
| | - A Pai
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - O Palashov
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - C Palomba
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - H Pan
- National Tsing Hua University, Hsinchu 300, Taiwan
| | - Y Pan
- University of Maryland, College Park, Maryland 20742, USA
| | - C Pankow
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M A Papa
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - H Paris
- Stanford University, Stanford, California 94305, USA
| | - A Pasqualetti
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Passaquieti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | | | - M Pedraza
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - A Pele
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Penn
- Hobart and William Smith Colleges, Geneva, New York 14456, USA
| | - A Perreca
- Syracuse University, Syracuse, New York 13244, USA
| | - M Phelps
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Pichot
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Pickenpack
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Piergiovanni
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - V Pierro
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - L Pinard
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - I M Pinto
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - M Pitkin
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Poeld
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Poggiani
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - A Poteomkin
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - J Powell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Prasad
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - V Predoi
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | | | - T Prestegard
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - L R Price
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Prijatelj
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S Privitera
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G A Prodi
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - L Prokhorov
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - O Puncken
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - M Punturo
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - P Puppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - M Pürrer
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Qin
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - V Quetschke
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - E Quintero
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | | | - F J Raab
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D S Rabeling
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | - I Rácz
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - H Radkins
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P Raffai
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - S Raja
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - G Rajalakshmi
- Tata Institute for Fundamental Research, Mumbai 400005, India
| | - M Rakhmanov
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - C Ramet
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Ramirez
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - P Rapagnani
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - V Raymond
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Razzano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - V Re
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Recchia
- Università di Roma Tor Vergata, I-00133 Roma, Italy and INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy
| | - C M Reed
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T Regimbau
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Reid
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - D H Reitze
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and University of Florida, Gainesville, Florida 32611, USA
| | - O Reula
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - E Rhoades
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - F Ricci
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R Riesen
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Riles
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - N A Robertson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F Robinet
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - A Rocchi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - S B Roddy
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L Rolland
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - J G Rollins
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Romano
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - G Romanov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - J H Romie
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D Rosińska
- CAMK-PAN, 00-716 Warsaw, Poland and Institute of Astronomy, 65-265 Zielona Góra, Poland
| | - S Rowan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Rüdiger
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Ruggi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Ryan
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Salemi
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - L Sammut
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - V Sandberg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J R Sanders
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - S Sankar
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V Sannibale
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | | | - E Saracco
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - B Sassolas
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | | | - P R Saulson
- Syracuse University, Syracuse, New York 13244, USA
| | - R Savage
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Scheuer
- Northwestern University, Evanston, Illinois 60208, USA
| | - R Schilling
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Schilman
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - P Schmidt
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - R Schnabel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | | | - E Schreiber
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Schuette
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B F Schutz
- Cardiff University, Cardiff CF24 3AA, United Kingdom and Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - J Scott
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S M Scott
- Australian National University, Canberra, ACT 0200, Australia
| | - D Sellers
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A S Sengupta
- Indian Institute of Technology, Gandhinagar, Ahmedabad, Gujarat 382424, India
| | - D Sentenac
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - V Sequino
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Sergeev
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - D A Shaddock
- Australian National University, Canberra, ACT 0200, Australia
| | - S Shah
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - M S Shahriar
- Northwestern University, Evanston, Illinois 60208, USA
| | - M Shaltev
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Z Shao
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B Shapiro
- Stanford University, Stanford, California 94305, USA
| | - P Shawhan
- University of Maryland, College Park, Maryland 20742, USA
| | - D H Shoemaker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T L Sidery
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Siellez
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - X Siemens
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - D Sigg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D Simakov
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Singer
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - L Singer
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Singh
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A M Sintes
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - B J J Slagmolen
- Australian National University, Canberra, ACT 0200, Australia
| | - J Slutsky
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - J R Smith
- California State University Fullerton, Fullerton, California 92831, USA
| | - M R Smith
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R J E Smith
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - N D Smith-Lefebvre
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E J Son
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - B Sorazu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Souradeep
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - A Staley
- Columbia University, New York, New York 10027, USA
| | - J Stebbins
- Stanford University, Stanford, California 94305, USA
| | - M Steinke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - B C Stephens
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Steplewski
- Washington State University, Pullman, Washington 99164, USA
| | - S Stevenson
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Stone
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - D Stops
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K A Strain
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Straniero
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S Strigin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - R Sturani
- Instituto de Física Teórica, Universidade Estadual Paulista/ICTP South American Institute for Fundamental Research, São Paulo, São Paulo 01140-070, Brazil
| | - A L Stuver
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - S Susmithan
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P J Sutton
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B Swinkels
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Tacca
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - D Talukder
- University of Oregon, Eugene, Oregon 97403, USA
| | - D B Tanner
- University of Florida, Gainesville, Florida 32611, USA
| | - J Tao
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S P Tarabrin
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Taylor
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G Tellez
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - M Thomas
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Thomas
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - K A Thorne
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K S Thorne
- Caltech-CaRT, Pasadena, California 91125, USA
| | - E Thrane
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Tiwari
- University of Florida, Gainesville, Florida 32611, USA
| | - K V Tokmakov
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - C Tomlinson
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - C V Torres
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - C I Torrie
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F Travasso
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - G Traylor
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Tse
- Columbia University, New York, New York 10027, USA
| | - D Tshilumba
- University of Brussels, Brussels 1050, Belgium
| | - H Tuennermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Ugolini
- Trinity University, San Antonio, Texas 78212, USA
| | | | - A L Urban
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S A Usman
- Syracuse University, Syracuse, New York 13244, USA
| | - H Vahlbruch
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Vajente
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - G Valdes
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - M van Beuzekom
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J F J van den Brand
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | | | - M V van der Sluys
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | | | - A A van Veggel
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Vass
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Vasúth
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - R Vaulin
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Vecchio
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - G Vedovato
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - J Veitch
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - P J Veitch
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - K Venkateswara
- University of Washington, Seattle, Washington 98195, USA
| | - D Verkindt
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - F Vetrano
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - A Viceré
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - R Vincent-Finley
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - J-Y Vinet
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Vitale
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Vo
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - H Vocca
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - C Vorvick
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - W D Vousden
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S P Vyachanin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - A R Wade
- Australian National University, Canberra, ACT 0200, Australia
| | - L Wade
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Wade
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Walker
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - L Wallace
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S Walsh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Wang
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - X Wang
- Tsinghua University, Beijing 100084, China
| | - R L Ward
- Australian National University, Canberra, ACT 0200, Australia
| | - M Was
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Weaver
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - L-W Wei
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Weinert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A J Weinstein
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Weiss
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Welborn
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L Wen
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P Wessels
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M West
- Syracuse University, Syracuse, New York 13244, USA
| | - T Westphal
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Wette
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J T Whelan
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - D J White
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - B F Whiting
- University of Florida, Gainesville, Florida 32611, USA
| | - K Wiesner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Wilkinson
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - K Williams
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - L Williams
- University of Florida, Gainesville, Florida 32611, USA
| | - R Williams
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T D Williams
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | | | - J L Willis
- Abilene Christian University, Abilene, Texas 79699, USA
| | - B Willke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M Wimmer
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - W Winkler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C C Wipf
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A G Wiseman
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - H Wittel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - G Woan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Wolovick
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - J Worden
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - Y Wu
- University of Florida, Gainesville, Florida 32611, USA
| | - J Yablon
- Northwestern University, Evanston, Illinois 60208, USA
| | - I Yakushin
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Yam
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - H Yamamoto
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C C Yancey
- University of Maryland, College Park, Maryland 20742, USA
| | - H Yang
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Yoshida
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | - M Yvert
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | | | - M Zanolin
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J-P Zendri
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - Fan Zhang
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA and Tsinghua University, Beijing 100084, China
| | - L Zhang
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Zhao
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - H Zhu
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - X J Zhu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M E Zucker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S Zuraw
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - J Zweizig
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R L Aptekar
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - J L Atteia
- Université de Toulouse, UPS-OMP, IRAP, Toulouse, France and CNRS, IRAP, 14, Avenue Edouard Belin, F-31400 Toulouse, France
| | - T Cline
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - V Connaughton
- CSPAR, University of Alabama in Huntsville, Huntsville, Alabama 35899, USA
| | - D D Frederiks
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - S V Golenetskii
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - K Hurley
- University of California-Berkeley, Space Sciences Lab, 7 Gauss Way, Berkeley, California 94720, USA
| | - H A Krimm
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA and Universities Space Research Association, 7178 Columbia Gateway Drive Columbia, Maryland 21046, USA
| | - M Marisaldi
- INAF-IASF Bologna, Via Piero Gobetti 101, 40129 Bologna, Italy
| | - V D Pal'shin
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation and Saint Petersburg State Polytechnical University, 195251, Saint Petersburg, Russia
| | - D Palmer
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - D S Svinkin
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - Y Terada
- Graduate School of Science and Engineering, Saitama University, Saitama City, Japan
| | - A von Kienlin
- Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany
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Palm EC, Esler D, Anderson EM, Williams TD, Love OP, Wilson MT. Baseline corticosterone in wintering marine birds: methodological considerations and ecological patterns. Physiol Biochem Zool 2013; 86:346-53. [PMID: 23629884 DOI: 10.1086/670156] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/03/2022]
Abstract
Previous studies have related levels of plasma corticosterone (CORT) of seabirds to variation in foraging conditions during the breeding period, but it is unclear whether similar relationships between foraging conditions and baseline CORT exist during other life stages. We validated methods for identifying baseline CORT of lethally sampled birds and assessed variation in baseline CORT relative to winter habitat conditions. We collected free-living white-winged scoters (Melanitta fusca) at four wintering sites during December and February. We found increasing CORT values beyond 3 min after time since flush (the duration between initial flush and death), presumably reflecting acute stress responses. Our results demonstrate that it is possible to obtain baseline CORT from lethally sampled birds if the time from initial flush until death is measured. Our study sites varied appreciably in exposure to wind and waves, predation danger, diving depths, and the fraction of preferred foods in scoter diets. Despite these habitat differences, baseline CORT did not vary across sites or winter periods. We interpret this lack of variation as evidence that birds select wintering areas where they can successfully manage site-specific costs and maintain physiological homeostasis.
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Affiliation(s)
- E C Palm
- Centre for Wildlife Ecology, Simon Fraser University, Burnaby, British Columbia, Canada.
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Winter V, Elliott JE, Letcher RJ, Williams TD. Validation of an egg-injection method for embryotoxicity studies in a small, model songbird, the zebra finch (Taeniopygia guttata). Chemosphere 2013; 90:125-131. [PMID: 22959718 DOI: 10.1016/j.chemosphere.2012.08.017] [Citation(s) in RCA: 11] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/10/2012] [Revised: 08/02/2012] [Accepted: 08/07/2012] [Indexed: 06/01/2023]
Abstract
Female birds deposit or 'excrete' lipophilic contaminants to their eggs during egg formation. Concentrations of xenobiotics in bird eggs can therefore accurately indicate levels of contamination in the environment and sampling of bird eggs is commonly used as a bio-monitoring tool. It is widely assumed that maternally transferred contaminants cause adverse effects on embryos but there has been relatively little experimental work confirming direct developmental effects (cf. behaviorally-mediated effects). We validated the use of egg injection for studies of in ovo exposure to xenobiotics for a small songbird model species, the zebra finch (Taeniopygia guttata), where egg weight averages only 1 g. We investigated a) the effect of puncturing eggs with or without vehicle (DMSO) injection on egg fate (embryo development), chick hatching success and subsequent growth to 90 days (sexual maturity), and b) effects of two vehicle solutions (DMSO and safflower oil) on embryo and chick growth. PBDE-99 and -47 were measured in in ovo PBDE-treated eggs, chicks and adults to investigate relationships between putative injection amounts and the time course of metabolism (debromination) of PBDE-99 during early development. We successfully injected a small volume (5 μL) of vehicle into eggs, at incubation day 0, with no effects on egg or embryo fate and with hatchability similar to that for non-manipulated eggs in our captive-breeding colony (43% vs. 48%). We did find some evidence for an inhibitory effect of DMSO vehicle on post-hatching chick growth, in male chicks only. This method can be used to treat eggs in a dose-dependent, and ecologically-relevant, manner with PBDE-99, based on chemical analysis of eggs, hatchling and adults.
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Affiliation(s)
- V Winter
- Department of Biological Sciences, Simon Fraser University, Burnaby, British Columbia, Canada V5A 1S6
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Abstract
Levels of antibodies in sera from patients with diagnoses of subclinical or established psittacosis infections were determined by the serum neutralization anti-IgG test and by conventional tests. Relatively high levels of serum neutralizing anti-bodies were detected in tests in which anti-IgG was used, whereas conventional tests disclosed only marginal levels of antibody. Use of the serum neutralization anti-IgG test in conjunction with the fluorescent cell-counting technique permitted serum antibody determinations within 24 hr.
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Affiliation(s)
- T D Williams
- Aerobiology & Evaluation Laboratories, Fort Detrick, Frederick, Maryland 21701
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Love OP, Gilchrist HG, Bêty J, Wynne-Edwards KE, Berzins L, Williams TD. Using life-histories to predict and interpret variability in yolk hormones. Gen Comp Endocrinol 2009; 163:169-74. [PMID: 18952089 DOI: 10.1016/j.ygcen.2008.10.001] [Citation(s) in RCA: 25] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 07/31/2008] [Revised: 10/01/2008] [Accepted: 10/03/2008] [Indexed: 10/21/2022]
Abstract
Variation in yolk hormones is assumed to provide the plasticity necessary for mothers to individually optimize reproductive decisions via changes in offspring phenotype, the benefit being to maximise fitness. However, rather than routinely expecting adaptive variation within all species, the pattern and magnitude of yolk hormone deposition should theoretically relate to variation in life-histories. Here we present data on intra-clutch variation in yolk corticosterone in three species along a developmental continuum (European starling (Sturnus vulgaris): fully altricial; black guillemot (Cepphus grylle): semi-precocial; common eider (Somateria mollissima): fully precocial) to examine how and why variation in life-histories might relate to the evolution of variation in yolk steroids. Starlings and guillemots showed a significant increase in yolk corticosterone across the laying sequence; however, we found no pattern within eider clutches. Moreover, starlings showed the largest difference (94.6%) in yolk corticosterone between first- and last-laid eggs, whereas guillemots showed a moderate difference (58.9%). Despite these general species-specific patterns, individuals showed marked variation in the intra-clutch patterns of yolk corticosterone within each species indicating potential differences in intra-clutch flexibility among females. It is well documented that exposure to elevated yolk glucocorticoids reduces offspring quality at birth/hatching in many taxa and it has therefore been proposed that elevated yolk levels may modulate offspring competition and/or facilitate brood reduction under harsh conditions in birds. Our data suggests that intra-clutch variation in yolk corticosterone has the potential to act as an adaptive maternal effect in species where modulation of competition between nest-bound offspring would benefit mothers (starlings and guillemots). However, in precocial species where mothers would not benefit from a modulation of offspring quality, intra-clutch variation in yolk hormones may play little or no adaptive role. While future phylogenetically-controlled studies will be helpful in examining questions of adaptive mechanisms once more data on yolk corticosterone becomes available, our results nonetheless suggest that research on the evolutionary role of yolk hormones can benefit by a priori incorporating species-specific life-history-driven hypotheses.
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Affiliation(s)
- O P Love
- Department of Biological Sciences, Simon Fraser University, 8888 University Drive, Burnaby, BC, Canada.
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Abstract
An improved knowledge and understanding of the fundamental biological requirements is needed for many of the species of fish held in captivity and, without this knowledge it is difficult to determine the optimal conditions for laboratory culture. The aim of this paper is to review the key issues concerning environmental enrichment for laboratory-held fish species and identify where improvements are required. It provides background information on environmental enrichment, describes enrichment techniques currently used in aquatic ecotoxicology studies, identifies potential restrictions in their use and discusses why more detailed and species-specific guidance is needed.
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Affiliation(s)
- T D Williams
- AstraZeneca, Safety, Health and Environment, Brixham Environmental Laboratory, Freshwater Quarry, Brixham, Devon TQ5 8BA, UK.
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Falciani F, Diab AM, Sabine V, Williams TD, Ortega F, George SG, Chipman JK. Hepatic transcriptomic profiles of European flounder (Platichthys flesus) from field sites and computational approaches to predict site from stress gene responses following exposure to model toxicants. Aquat Toxicol 2008; 90:92-101. [PMID: 18823667 DOI: 10.1016/j.aquatox.2008.07.020] [Citation(s) in RCA: 22] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/03/2008] [Revised: 07/24/2008] [Accepted: 07/31/2008] [Indexed: 05/26/2023]
Abstract
Genomic technologies offer opportunities to gain a more global assessment of the health status of an organism through an understanding of the functional pathways that are responding to pollutant exposure. We have developed a 13,000 clone cDNA toxicogenomics microarray for Platichthys flesus, the European flounder (EU-GENIPOL Project). We aimed to distinguish the origins of flounder taken from six sampling sites of different pollution status in Northern Europe according to their hepatic gene expression profile using bioinformatic approaches. To determine which gene expression differences may relate to pollutant impact, we have completed complementary laboratory exposures of flounder to selected toxicants and determined the associated gene expression profiles. Using multivariate variable selection coupled with a statistical modelling procedure (GALGO) we can predict geographical site but the accuracy is limited to specific sites. The search space for a combination of genes that effectively predicts class membership is very large, however, by combining the signatures derived from acute laboratory exposure to individual chemicals to limit the search space, a very accurate model for classification of all the different environmental sites was achieved. The final model utilised the expression profiles of 16 clones and validation with a qPCR array comprising these genes correctly assigned the site of origin for fish obtained from three of the sites in an independent sampling. These data would imply that the gene expression fingerprints obtained with these arrays are primarily attributable to variations in chemical pollutant responses at the different sites, indicating their potential utility in environmental impact assessment.
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Affiliation(s)
- F Falciani
- School of Biosciences, The University of Birmingham, Birmingham B15 2TT, UK.
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Larsen PF, Nielsen EE, Williams TD, Loeschcke V. Intraspecific variation in expression of candidate genes for osmoregulation, heme biosynthesis and stress resistance suggests local adaptation in European flounder (Platichthys flesus). Heredity (Edinb) 2008; 101:247-59. [PMID: 18560442 DOI: 10.1038/hdy.2008.54] [Citation(s) in RCA: 50] [Impact Index Per Article: 3.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022] Open
Abstract
Despite the recent discovery of significant genetic structuring in a large number of marine organisms, the evolutionary significance of these often minute genetic differences are still poorly understood. To elucidate the adaptive relevance of low genetic differentiation among marine fish populations, we studied expression differences of osmoregulatory and stress genes in genetically weakly differentiated populations of the European flounder (Platichthys flesus), distributed across a natural salinity gradient. Flounders were maintained in a long-term reciprocal transplantation experiment mimicking natural salinities in the North Sea and the Baltic Sea. Applying real-time quantitative PCR and microarray analysis we studied expression of four candidate genes (hsp70, angiotensinogen, Na/K-ATPase-alpha and 5-aminolevulinic acid synthase (ALAS)) in gill, kidney and liver tissues. Genes involved in osmoregulative processes (Na/K-ATPases-alpha and angiotensinogen) showed highly plastic but similar expression in the two populations dependent on environmental salinity. However, we observed a unique sixfold up-regulation of hsp70 in kidney tissue of flounder from the North Sea following long-term acclimation to Baltic salinities. Similarly, significant differences between North Sea and Baltic flounders in expression of ALAS in response to different salinities were found in gill and liver tissue. These findings strongly suggest that gene expression in flounders is shaped by adaptation to local environmental conditions. This identification of adaptive differences in high gene flow marine organisms adds a new dimension to our current understanding of evolutionary processes in the sea and is of paramount importance for identification, protection and sustainable management of marine biodiversity.
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Affiliation(s)
- P F Larsen
- Department of Inland Fisheries, Danish Institute for Fisheries Research, Technical University of Denmark, Silkeborg, Denmark.
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Love OP, Wynne-Edwards KE, Bond L, Williams TD. Determinants of within- and among-clutch variation in yolk corticosterone in the European starling. Horm Behav 2008; 53:104-11. [PMID: 17961563 DOI: 10.1016/j.yhbeh.2007.09.007] [Citation(s) in RCA: 73] [Impact Index Per Article: 4.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 07/19/2007] [Revised: 08/28/2007] [Accepted: 09/04/2007] [Indexed: 11/28/2022]
Abstract
Maternal glucocorticoids are known to affect offspring phenotype in numerous vertebrate taxa. In birds, the maternal transfer of corticosterone to eggs was recently proposed as a hormonal mechanism by which offspring phenotype is matched to the relative quality of the maternal environment. However, current hypotheses lack supporting information on both intra- and inter-clutch variation in yolk corticosterone for wild birds. As such, we examined variation in yolk corticosterone levels in a wild population of European starlings (Sturnus vulgaris). Maternal condition, clutch size and nesting density were all negatively related to yolk corticosterone deposition; females with high condition indices, those laying larger clutches and those nesting in high-density associations deposited lower amounts of the hormone into eggs than those with low condition indices, laying small clutches and nesting in isolation. Alternatively, we found no effects of maternal age or human disturbance on yolk corticosterone deposition. Intra-clutch variation of yolk corticosterone was significant, with levels increasing across the laying sequence in all clutch sizes examined, with the difference between first and last-laid eggs being greater in large versus small clutches. Given the reported effects of yolk corticosterone on offspring size and growth, intra-clutch variation in yolk corticosterone has the potential to alter the competitive environment within a brood. Furthermore, our results indicate that variation in yolk corticosterone can originate from variation in both the mother's quality as well as the quality of her breeding environment. The presence of inter-female variation in particular is an important pre-requisite in testing whether the exposure of offspring to maternally-derived corticosterone is a mechanistic link between offspring phenotypic plasticity and maternal quality.
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Affiliation(s)
- O P Love
- Department of Biological Sciences, Simon Fraser University, Burnaby, British, Columbia, Canada V5A 1S6.
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Abstract
Recent studies on hormone-mediated maternal effects in birds have highlighted the influence of variable maternal yolk androgen concentration on offspring phenotype, particularly in terms of early development. If genetic differences between laying females regulate variation in yolk hormone concentration, then this physiological maternal effect is an indirect genetic effect which can provide a basis for the co-evolution of maternal and offspring phenotypes. Thus, we investigated the evolutionary associations between maternally derived yolk testosterone (T) and early developmental traits in passerine birds via a comparative, phylogenetic analysis. Our results from species-correlation and independent contrasts analyses provide convergent evidence for the correlated evolution of maternal yolk T concentration and length of the prenatal developmental period in passerines. Here, we show these traits are significantly negatively associated (species-correlation: p<0.001, r2=0.85; independent contrasts: p=0.005). Our results highlight the need for more studies investigating the role of yolk hormones in evolutionary processes concerning maternal effects.
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Affiliation(s)
- K B Gorman
- Department of Biological Sciences, Simon Fraser University, 8888 University Drive, Burnaby, British Columbia, Canada V5A 1S6.
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Seaman DA, Guglielmo CG, Williams TD. Effects of physiological state, mass change and diet on plasma metabolite profiles in the western sandpiper Calidris mauri. ACTA ACUST UNITED AC 2005; 208:761-9. [PMID: 15695767 DOI: 10.1242/jeb.01451] [Citation(s) in RCA: 46] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022]
Abstract
We used a food restriction/refeeding protocol to put birds through a controlled cycle of mass loss and mass gain to investigate the effects of rate and phase of mass change on plasma metabolite levels in relation to diet. Despite marked differences in fat content of the two diets (18% vs 4%) mean rate of mass loss or mass gain was independent of diet. There was also no effect of diet on plasma levels of any of the four measured metabolite (triglyceride, glycerol, uric acid and beta-OH-butyrate) during mass loss. However, during mass gain birds on the low fat diet had higher plasma levels of triglyceride and uric acid and lower beta-OH-butyrate than birds gaining mass on the high-fat diet. Thus, diet composition can affect plasma metabolite profiles independently of differences in rates of mass change. Nevertheless, certain plasma metabolites were related to variation in rates of mass change across physiological states. Glycerol levels were negatively related to the rate of mass change (independent of diet), and butyrate was negatively related to the rate of mass change on both diets (though the slope of this relationship was diet dependent). Uric acid was positively related to the rate of mass change but only for birds on the low-fat diet. Our study therefore confirms that measurement of plasma metabolites can provide robust information on physiological state (gain, loss) and the rate of mass change (e.g. in free-living birds caught only once) although researchers should be cogniscent of potential confounding effects of diet composition for certain metabolites, both for field studies and for future experimental validations of this technique.
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Affiliation(s)
- D A Seaman
- Department of Biological Sciences, Simon Fraser University, 8888 University Drive, Burnaby, V5A 1S6, Canada
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Gill H, Williams TD, Bishop CA, Cheng KM, Elliott JE. Effects of azinphos-methyl on cholinergic responses and general health in zebra finches (Taeniopygia guttata) after previous treatment with p,p'-DDE. Arch Environ Contam Toxicol 2005; 48:118-126. [PMID: 15657813 DOI: 10.1007/s00244-004-0229-8] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/02/2003] [Accepted: 07/15/2004] [Indexed: 05/24/2023]
Abstract
Although organochlorine (OC) pesticides were replaced with organophosphates (OPs) in the early 1970s, they continue to persist in orchard environments today. Extensive research has been conducted to determine the effects of currently used OPs on cholinesterase (ChE) activity; however, although OCs continue to be prevalent in areas of previous use, few studies have looked at the toxicity of a combination of residual OC compounds with currently used OP pesticides. The focus of our study was to determine the effects of azinphos-methyl (a common OP used in apple orchards today) on ChE activity and general health in zebra finches (Taeniopygia guttata) previously exposed to p,p'-DDE (a commonly detected metabolite of DDT). The main results of our study were as follows: (1) azinphos-methyl alone caused a dose-dependent inhibition of plasma and brain ChE activity; (2) p,p'-DDE in combination with azinphos-methyl did not change azinphos-methyl inhibition of ChE activity; and (3) there were suggestions of immunostimulation in birds dosed 1 year previously to p,p'-DDE and of anemia when p,p'-DDE was combined with azinphos-methyl; however, there was no dose-response for these parameters in birds subsequently dosed with p,p'-DDE.
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Affiliation(s)
- H Gill
- Agroecology Group, Faculty of Agricultural Sciences, University of British Columbia, 2357 Main Mall, Vancouver, British Columbia, V6T 1Z4, Canada
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Abstract
The purpose of the review is to highlight the influences of ambient temperature (T(a)) and caloric restriction (CR) on metabolism, cardiovascular function and behavior in mice. Standard vivarium ambient temperatures (T(a)?23 degrees C) are a mild cold stress for mice requiring elevated metabolic rate and food intake. Increasing T(a) into the zone of thermoneutrality (TMN?29-33 degrees C) markedly reduces food intake, metabolic rate, heart rate (HR) and blood pressure in mice. Mice are members of a diverse, yet unique group of homeothermic animals that respond to thermal and energetic challenges by allowing body temperature (T(b)) to fall to less than 31 degrees C, a condition known as torpor. In mice housed at standard T(a), torpor is induced by a single night of fasting or a few days of CR. The mechanisms responsible for initiating torpor are related to reduced caloric availability, but do not require leptin. Mice housed at TMN and subjected to CR exhibit physiologic reductions in metabolic rate and HR, but do not appear to enter torpor. Finally, mice exhibit differential locomotor activity responses during CR that depends on T(a). At standard T(a), mice display increased light-phase home-cage activity with CR. This response is virtually eliminated when CR is performed at TMN. We suggest that researchers using mice to investigate energy homeostasis and cardiovascular physiology carefully consider the influence of T(a) on physiology and behavior.
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Affiliation(s)
- J M Overton
- Department of Nutrition, Program in Neuroscience, 236 Biomedical Research Facility, Florida State University, Tallahassee, FL 32306-4340, USA.
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Abstract
1. In the present study, we determined the effect of diet-induced obesity on cardiovascular and metabolic regulation in mice at standard laboratory temperatures (ambient temperature (Ta) = 22 degrees C) and during exposure to thermoneutrality (Ta = 30 degrees C). 2. Male C57BL/6J (B6) mice fed a high-fat diet (HFF; n = 17) or chow (CHW; n = 14) for 15 weeks were surgically instrumented with telemetry devices, housed in metabolic chambers and assigned to either control or atenolol treatment (25 mg/kg per day in drinking water) to determine the effects of obesity on baseline cardiovascular function and on the responses to thermoneutrality and 24 h fasting. Mean arterial pressure (MAP), heart rate (HR), arterial pressure and HR variability (time and frequency domain), oxygen consumption (VO2) and locomotor activity were determined. 3. The HFF mice exhibited increased bodyweight (+10.6 +/- 4.1 g), moderate light period hypertension (+8.6 +/- 2.6 mmHg), no difference in HR and increased HR variability at standard laboratory temperature compared with CHW controls. Atenolol produced less of a decrease in HR in HFF mice (-42 +/- 10 b.p.m.) compared with CHW controls (-73 +/- 15 b.p.m.). Acute exposure to thermoneutrality (Ta = 30 degrees C) reduced HR similarly in both HFF and CHW mice (approximately 175 b.p.m.), but reduced MAP less in HFF than in CHW mice (-7.3 +/- 2.5 and -15.2 +/- 1.0 mmHg), respectively. Atenolol treatment had only minor effects on the HR response to thermonuetrality (-114 +/- 13 and -129 +/- 8 b.p.m. in HFF and CHW mice, respectively). The HFF mice displayed greater fasting-induced reductions in light period MAP than did CHW mice (-10.0 +/- 1.1 vs-3.1 +/- 3.5 mmHg, respectively), whereas HR was decreased equally in both groups. Fasting-induced increases in HR variability were attenuated in HFF mice. 4. We conclude that diet-induced obesity produced generally minor changes in cardiovascular regulation in B6 mice at baseline, some of which are distinct from the effects of diet-induced obesity in larger animal models. In contrast, acute variations in Ta or caloric availability produce pronounced alterations in cardiovascular function in either lean or obese mice, which are generally evident after atenolol and, thus, presumably not due exclusively to variation in cardiac sympathetic activity. Interestingly, the degree of obesity induced hypertension was augmented when mice were studied at thermonuetrality. The results suggest an important unrecognized role for vagal tone in the regulation of cardiovascular function in mice and support the need for considerable caution when using mouse models of obesity to examine regulation of cardiovascular function. We argue that mouse physiology studies should be performed in thermoneutral conditions.
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Affiliation(s)
- T D Williams
- Department of Nutrition, Food and Exercise Sciences, The Program in Neuroscience, Florida State University, Tallahassee, Florida 32306-4340, USA
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Williams TD, Kitaysky AS, Vézina F. Individual variation in plasma estradiol-17beta and androgen levels during egg formation in the European starling Sturnus vulgaris: implications for regulation of yolk steroids. Gen Comp Endocrinol 2004; 136:346-52. [PMID: 15081834 DOI: 10.1016/j.ygcen.2004.01.010] [Citation(s) in RCA: 73] [Impact Index Per Article: 3.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 10/02/2003] [Revised: 01/21/2004] [Accepted: 01/26/2004] [Indexed: 11/21/2022]
Abstract
While it is clear that maternal transfer of steroids to egg yolk can have significant effects on offspring phenotype, an unresolved question is whether females can facultatively adjust yolk hormone levels independently of their own plasma levels or whether yolk steroid levels are simply a direct consequence of temporal variation in the female's hormonal status. In part, this is because we lack detailed information about the day-to-day pattern of changes in plasma hormone levels during the laying cycle for non-domesticated birds. Here, we describe changes in plasma estradiol-17beta (E2) and androgens, throughout laying in relation to specific stages of ovarian follicular development in the European starling (Sturnus vulgaris). Plasma E2 levels increased rapidly from the onset of rapid yolk development (RYD) to reach maximum levels in birds with a complete follicle hierarchy (> or = 4 yolky follicles). However, levels decreased linearly throughout the later stages of follicle development returning to pre-breeding values before the final yolky follicle was ovulated. In females with > or = 4 yolky follicles there was 10-fold variation in plasma E2 levels among individual females, but this was not related to plasma levels of the main yolk precursor vitellogenin or to the total mass of yolky follicles developing at the time of blood sampling. In contrast to E2, plasma androgen levels showed only a very gradual linear decline throughout the laying cycle from pre-RYD to clutch completion. Furthermore, androgen levels showed less individual variability: 4-fold variation among females with > or = 4 yolky follicles, although this was also independent of our measures of reproductive function. Data on inter- and intra-individual variation in female hormone levels are important to set-up a priori predictions for, and interpretation of, studies of yolk hormone levels.
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Affiliation(s)
- T D Williams
- Department of Biological Sciences, Simon Fraser University, 8888 University Drive, Burnaby, BC, Canada.
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Abstract
SUMMARYEgg production in oviparous vertebrates is assumed to be costly but the physiological basis of any costs remains unknown. The avian oviduct is a highly differentiated linear organ, with five functionally specific regions. Here we show that the oviduct regresses rapidly `from the top down' as soon as the more proximal regions have completed their function but while the distal regions still retain an oviductal egg. In zebra finches Taeniopygia guttata, oviduct mass did not differ between early laying birds at the 1-egg stage compared with late-laying birds (with one remaining yolky follicle; dry mass, 151-167 mg). However, in birds with no remaining yolky follicles but with an oviductal egg, oviduct mass decreased to 94 mg (44%). Regression occurred unequally among different regions of the oviduct, with significant decreases in the proximal infundibulum/magnum and isthmus regions(59% and 40%, respectively), but no change in distal shell gland/vagina mass. The shell gland did not regress until after the last oviposition. Thus, the avian oviduct has a highly regulated size-function relationship consistent with a high maintenance energy cost for this organ. We suggest that oviduct function is a significant contributor to the physiological costs of egg production and might mediate individual variation in maternal effects associated with non-yolk components of egg quality (e.g. immunoglobulins,lysozyme).
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Affiliation(s)
- T D Williams
- Department of Biological Sciences, Simon Fraser University, 8888 University Drive, Burnaby, British Columbia V5A 1S6, Canada.
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Williams TD, Gensberg K, Minchin SD, Chipman JK. A DNA expression array to detect toxic stress response in European flounder (Platichthys flesus). Aquat Toxicol 2003; 65:141-57. [PMID: 12946615 DOI: 10.1016/s0166-445x(03)00119-x] [Citation(s) in RCA: 93] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/18/2023]
Abstract
As a first stage in developing a DNA array-based approach to investigating the effects of pollutants on an environmentally relevant European fish species, we have constructed a 160-gene custom microarray for European flounder. Degenerate primers were used to amplify 110 different fragments of stress-related and other genes from European flounder cDNA and genomic DNA. Additionally, 22 fragments were obtained by suppressive subtractive hybridisation (SSH). These fragments were cloned and sequenced, then, with additional control genes, used to create a cDNA microarray for flounder. After optimisation of the arraying process, hepatic mRNA was isolated from flounder caught in the polluted Tyne and relatively unpolluted Alde estuaries. Fluorescent cDNA probes were synthesised from the mRNA and used in dual-colour hybridisations to the microarray. A number of transcripts were differentially expressed between Tyne and Alde female flounder but these changes were not significant, due to high inter-individual variation. However, in comparisons between Tyne and Alde male flounder, 11 transcripts were found to significantly differ in expression (P<0.05). Seven transcripts were more highly expressed in the Tyne male fish (CYP1A, UDPGT, alpha-2HS-glycoprotein, dihydropyrimidine dehydrogenase, Cu/Zn SOD, aldehyde dehydrogenase and paraoxonase). Four transcripts (Elongation factor 1 (EF1), EF2, Int-6 and complement component C3) were found to be significantly less abundant in the Tyne male fish. Selected genes were assayed by real-time PCR, then normalised to alpha-tubulin. These assays confirmed the significance of the array results for CYP1A, UDPGT and EF1, but not for Cu/Zn SOD. This study provides a link between traditional single-gene biomarker studies and the emerging field of eco-toxicogenomics, demonstrating the utility of microarray studies on environmentally sampled, non-model organisms.
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Affiliation(s)
- T D Williams
- School of Biosciences, The University of Birmingham, Edgbaston, Birmingham B15 2TT, UK.
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Schöneich C, Williams TD. CU(II)-catalyzed oxidation of Alzheimer's disease beta-amyloid peptide and related sequences: remarkably different selectivities of neurotoxic betaAP1-40 and non-toxic betaAP40-1. Cell Mol Biol (Noisy-le-grand) 2003; 49:753-61. [PMID: 14528912] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 04/27/2023]
Abstract
We investigated the CuII-catalyzed oxidation of beta-amyloid peptides betaAP10-20 and betaAP40-1 by tandem mass spectrometry and compared oxidation yields and selectivities to those for betaAP1-16, betaAP1-28 and betaAP1-40, which were obtained earlier (26). While betaAP1-16, betaAP1-28 and betaAP1-40 showed an almost exclusive oxidation of His residues to 2-oxo-histidine, the selectivity pattern is changed for betaAP10-20,which shows oxidation of His but also hydroxylation of Tyr and Phe. In contrast to betaAP1-40, the reverse sequence betaAP40-1 shows a strong selectivity for the hydroxylation of Tyr31 while only negligible His oxidation is observed at early time points. These selectivity patterns show the importance of the geometry of the metal-binding site for peptide/protein oxidation. The significantly different characteristic of betaAP1-40 and betaAP40-1 with regard to metal catalyzed processes may be related to the differences in the neurotoxic properties of these sequences.
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Affiliation(s)
- C Schöneich
- Department of Pharmaceutical Chemistry, The University of Kansas, 2095 Constant Avenue, Lawrence, KS 66047, USA.
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Esch SW, Williams TD, Biswas S, Chakrabarty A, LeVine SM. Sphingolipid profile in the CNS of the twitcher (globoid cell leukodystrophy) mouse: a lipidomics approach. Cell Mol Biol (Noisy-le-grand) 2003; 49:779-87. [PMID: 14528915] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 04/27/2023]
Abstract
Globoid cell leukodystrophy (Krabbe disease) is caused by mutations in galactosylceramidase, a lysosomal enzyme that acts to digest galactosylceramide, a glycolipid concentrated in myelin, and psychosine (galactosylsphingosine). Globoid cell leukodystrophy has been identified in many species including humans and twitcher mice. Several studies on human tissue have examined the lipid profile in this disease by gas, liquid or thin layer chromatography. Electrospray ionization tandem mass spectrometry combined with reverse phase HPLC has become a powerful alternative strategy, used here to compare the sphingolipid profile of pons/medulla tissue from twitcher mice with control tissue. In this lipidomics LC-MS approach, we scanned for precursors of m/z 264 to obtain a semi-quantitative profile of ceramides and galactosylceramides. Sphingosine-1-phosphate, C18:0 ceramide, C22:0 ceramide and C24:0 ceramide levels were reduced in the pons/medulla of twitcher mice compared to levels in control mice at 31 and 35-37 days of age. The levels of C22:0 and C24:0 galactosylceramide were similar between twitcher and control specimens and there was a trend toward reduced levels of C24:1 galactosylceramide and C24:1 hydroxy-galactosylceramide in twitcher specimens. Psychosine, C 16:0 ceramide and C 18:0 galactosylceramide levels were increased in the CNS of twitcher mice compared to levels in control mice. These data indicate that there is a trend toward decreased levels of long chain fatty acids and increased levels of shorter chain fatty acids in galactosylceramides and ceramides from twitcher mice compared with control mice, and such changes may be due to demyelination characteristic of acute pathology.
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Affiliation(s)
- S W Esch
- Mass Spectrometry Laboratory, University of Kansas, Lawrence, Kansas 66045, USA
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Williams TD, Chambers JB, Gagnon SP, Roberts LM, Henderson RP, Overton JM. Cardiovascular and metabolic responses to fasting and thermoneutrality in Ay mice. Physiol Behav 2003; 78:615-23. [PMID: 12782216 DOI: 10.1016/s0031-9384(03)00049-0] [Citation(s) in RCA: 24] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/28/2023]
Abstract
Several lines of evidence support a role for reduced melanocortin signaling in the regulation of metabolic rate and cardiovascular function during negative energy balance. We tested the hypothesis that agouti yellow (B6.Cg-A(y)) mice would exhibit blunted physiologic responses to fasting and thermoneutrality. Male B6.Cg-A(y) mice (A(y); n=11, 34+/-2 g) and lean B6 littermates (B6; n=7, 26+/-2 g) were implanted with telemetry devices and housed in metabolic chambers (T(a)=23 degrees C) to determine the effects of a 24-h fasting and exposure to thermoneutrality (T(a)=30 degrees C) on mean arterial pressure (MAP), heart rate (HR), AP and HR variability (time and frequency domain), oxygen consumption (VO(2)), and locomotor activity. A(y) mice exhibited elevated baseline light-period MAP (A(y): 113+/-4; B6: 99+/-3 mm Hg) and VO(2) (A(y): 1.82+/-0.08 vs. B6: 1.45+/-0.13 ml/min) with no difference in HR (A(y): 530+/-12 vs. B6: 548+/-19 bpm). At 12-24 h after food removal, A(y) mice displayed normal fasting-induced bradycardia (A(y): -106+/-12; B6: -117+/-19 bpm) and reduction in VO(2) (A(y): -0.19+/-0.04 vs. B6: -0.28+/-0.05 ml/min), but with augmented hypotension (A(y): -9+/-2 vs. B6: -0.5+/-2 mm Hg) and blunted hyperactivity (A(y): 27+/-23 vs. B6: 122+/-42 m/11 h). Fasting was associated with increased HR variability in both time and frequency domain in B6 but not A(y) mice. Exposure to thermoneutrality produced comparable reductions in MAP, HR, and VO(2) in both strains. We conclude that inhibition of melanocortin signaling is not requisite for, but participates in, the metabolic and cardiovascular responses to negative energy balance.
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Affiliation(s)
- T D Williams
- Department of Nutrition, Food, and Exercise Sciences, Florida State University, 236 Biomedical Research Facility, Tallahassee, FL 32306-4340, USA
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