1
|
Gennari F, Pagano M, Toncelli A, Lisanti MT, Paoletti R, Roversi PF, Tredicucci A, Giaccone M. Terahertz imaging for non-invasive classification of healthy and cimiciato-infected hazelnuts. Heliyon 2023; 9:e19891. [PMID: 37809509 PMCID: PMC10559270 DOI: 10.1016/j.heliyon.2023.e19891] [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] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/02/2023] [Revised: 09/04/2023] [Accepted: 09/05/2023] [Indexed: 10/10/2023] Open
Abstract
The development of new non-invasive approaches able to recognize defective food is currently a lively field of research. In particular, a simple and non-destructive method able to recognize defective hazelnuts, such as cimiciato-infected ones, in real-time is still missing. This study has been designed to detect the presence of such damaged hazelnuts. To this aim, a measurement setup based on terahertz (THz) radiation has been developed. Images of a sample of 150 hazelnuts have been acquired in the low THz range by a compact and portable active imaging system equipped with a 0.14 THz source and identified as Healthy Hazelnuts (HH) or Cimiciato Hazelnut (CH) after visual inspection. All images have been analyzed to find the average transmission of the THz radiation within the sample area. The differences in the distribution of the two populations have been used to set up a classification scheme aimed at the discrimination between healthy and injured samples. The performance of the classification scheme has been assessed through the use of the confusion matrix on 50 samples. The False Positive Rate (FPR) and True Negative Rate (TNR) are 0% and 100%, respectively. On the other hand, the True Positive Rate (TPR) and False Negative Rate (FNR) are 75% and 25%, respectively. These results are relevant from the perspective of the development of a simple, automatic, real-time method for the discrimination of cimiciato-infected hazelnuts in the processing industry.
Collapse
Affiliation(s)
- Fulvia Gennari
- Dipartimento di Fisica “E. Fermi”, Università di Pisa, Largo B. Pontecorvo 3, 56127, Pisa, Italy
| | - Mario Pagano
- Institute of Research on Terrestrial Ecosystems (IRET), National Research Council (CNR), Via Madonna del Piano 10, 50019, Sesto Fiorentino, Italy
| | - Alessandra Toncelli
- Dipartimento di Fisica “E. Fermi”, Università di Pisa, Largo B. Pontecorvo 3, 56127, Pisa, Italy
- Centro per l’Integrazione della Strumentazione dell’Università di Pisa (CISUP), Lungarno Pacinotti 43/44, 56126, Pisa, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Largo B. Pontecorvo 3, 56127, Pisa, Italy
- Istituto Nanoscienze – CNR, Piazza S. Silvestro 12, 56127, Pisa, Italy
| | - Maria Tiziana Lisanti
- Università degli Studi di Napoli Federico II, Dipartimento di Agraria, Sezione di Scienze della Vigna e del Vino, viale Italia 60, 83100, Avellino, Italy
| | - Riccardo Paoletti
- Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Largo B. Pontecorvo 3, 56127, Pisa, Italy
- Dipartimento di Scienze Fisiche, della Terra e dell’Ambiente, Sezione di Fisica, Università di Siena, via Roma 56, 53100, Siena, Italy
| | - Pio Federico Roversi
- CREA, Research Centre for Plant Protection and Certification, 50125, Firenze, Italy
| | - Alessandro Tredicucci
- Dipartimento di Fisica “E. Fermi”, Università di Pisa, Largo B. Pontecorvo 3, 56127, Pisa, Italy
- Centro per l’Integrazione della Strumentazione dell’Università di Pisa (CISUP), Lungarno Pacinotti 43/44, 56126, Pisa, Italy
- Istituto Nanoscienze – CNR, Piazza S. Silvestro 12, 56127, Pisa, Italy
| | - Matteo Giaccone
- Institute for Mediterranean Agricultural and Forestry Systems, National Research Council, 80055 P.le Enrico, Fermi 1 - Loc. Porto del Granatello, 80055, Portici, Naples, Italy
| |
Collapse
|
2
|
Zanotto S, Bonatti L, Pantano MF, Mišeikis V, Speranza G, Giovannini T, Coletti C, Cappelli C, Tredicucci A, Toncelli A. Strain-Induced Plasmon Confinement in Polycrystalline Graphene. ACS Photonics 2023; 10:394-400. [PMID: 36820323 PMCID: PMC9936574 DOI: 10.1021/acsphotonics.2c01157] [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] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 07/24/2022] [Indexed: 06/18/2023]
Abstract
Terahertz spectroscopy is a perfect tool to investigate the electronic intraband conductivity of graphene, but a phenomenological model (Drude-Smith) is often needed to describe disorder. By studying the THz response of isotropically strained polycrystalline graphene and using a fully atomistic computational approach to fit the results, we demonstrate here the connection between the Drude-Smith parameters and the microscopic behavior. Importantly, we clearly show that the strain-induced changes in the conductivity originate mainly from the increased separation between the single-crystal grains, leading to enchanced localization of the plasmon excitations. Only at the lowest strain values explored, a behavior consistent with the deformation of the individual grains can instead be observed.
Collapse
Affiliation(s)
- Simone Zanotto
- NEST, Istituto Nanoscienze − CNR and Scuola Normale
Superiore, Piazza S. Silvestro 12, Pisa, 56127, Italy
| | - Luca Bonatti
- Scuola
Normale Superiore, Piazza dei Cavalieri 7, Pisa, 56126, Italy
| | - Maria F. Pantano
- Department
of Civil, Environmental and Mechanical Engineering, University of Trento, Via Mesiano 77, Trento, 38123, Italy
| | - Vaidotas Mišeikis
- Center
for Nanotechnology Innovation @NEST - Istituto Italiano di Tecnologia, Piazza S. Silvestro 12, Pisa, 56127, Italy
| | - Giorgio Speranza
- Centre
for Materials and Microsystems, Fondazione
Bruno Kessler, via Sommarive 18, Trento, I-38123, Italy
| | | | - Camilla Coletti
- Center
for Nanotechnology Innovation @NEST - Istituto Italiano di Tecnologia, Piazza S. Silvestro 12, Pisa, 56127, Italy
| | - Chiara Cappelli
- Scuola
Normale Superiore, Piazza dei Cavalieri 7, Pisa, 56126, Italy
| | - Alessandro Tredicucci
- Dipartimento
di Fisica ”E. Fermi” and CISUP, Università di Pisa, and Istituto Nanoscienze - CNR, Largo Pontecorvo 3, Pisa, 56127, Italy
| | - Alessandra Toncelli
- Dipartimento
di Fisica ”E. Fermi” and CISUP, Università di Pisa, and Istituto Nanoscienze - CNR, Largo Pontecorvo 3, Pisa, 56127, Italy
| |
Collapse
|
3
|
Cammarata S, Fontana A, Kaplan AE, Cornia S, Dao TH, Lacava C, Demontis V, Iadanza S, Vitali V, De Matteis F, Pedreschi E, Magazzù G, Toncelli A, Spinella F, Saponara S, Gunnella R, Rossella F, Salamon A, Bellani V. Polarization Control in Integrated Graphene-Silicon Quantum Photonics Waveguides. Materials (Basel) 2022; 15:8739. [PMID: 36556545 PMCID: PMC9786119 DOI: 10.3390/ma15248739] [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] [Figures] [Subscribe] [Scholar Register] [Received: 11/11/2022] [Revised: 11/29/2022] [Accepted: 12/02/2022] [Indexed: 06/17/2023]
Abstract
We numerically investigated the use of graphene nanoribbons placed on top of silicon-on-insulator (SOI) strip waveguides for light polarization control in silicon photonic-integrated waveguides. We found that two factors mainly affected the polarization control: the graphene chemical potential and the geometrical parameters of the waveguide, such as the waveguide and nanoribbon widths and distance. We show that the graphene chemical potential influences both TE and TM polarizations almost in the same way, while the waveguide width tapering enables both TE-pass and TM-pass polarizing functionalities. Overall, by increasing the oxide spacer thickness between the silicon waveguide and the top graphene layer, the device insertion losses can be reduced, while preserving a high polarization extinction ratio.
Collapse
Affiliation(s)
- Simone Cammarata
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pisa, 56127 Pisa, Italy
- Dipartimento di Ingegneria dell’Informazione, Università di Pisa, 56122 Pisa, Italy
| | - Andrea Fontana
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pavia, 27100 Pavia, Italy
| | - Ali Emre Kaplan
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pavia, 27100 Pavia, Italy
- Dipartimento di Ingegneria Industriale e dell’Informazione, Università di Pavia, 27100 Pavia, Italy
| | - Samuele Cornia
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pavia, 27100 Pavia, Italy
- Dipartimento di Scienze Fisiche, Informatiche e Matematiche, Università di Modena e Reggio Emilia, 41125 Modena, Italy
| | - Thu Ha Dao
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Roma Tor Vergata, 00133 Roma, Italy
- Dipartimento di Ingegneria Industriale, Università di Roma Tor Vergata, 00133 Roma, Italy
| | - Cosimo Lacava
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pavia, 27100 Pavia, Italy
- Dipartimento di Ingegneria Industriale e dell’Informazione, Università di Pavia, 27100 Pavia, Italy
| | - Valeria Demontis
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pavia, 27100 Pavia, Italy
- NEST, Scuola Normale Superiore, Istituto Nanoscienze-CNR, 56127 Pisa, Italy
| | - Simone Iadanza
- Centre for Advanced Photonics and Process Analysis, Munster Technological University, Tyndall National Institute, T12 P928 Cork, Ireland
| | - Valerio Vitali
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pavia, 27100 Pavia, Italy
- Optoelectronics Research Center (ORC), University of Southampton, Southampton SO17 1BJ, UK
| | - Fabio De Matteis
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Roma Tor Vergata, 00133 Roma, Italy
- Dipartimento di Ingegneria Industriale, Università di Roma Tor Vergata, 00133 Roma, Italy
| | - Elena Pedreschi
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pisa, 56127 Pisa, Italy
| | - Guido Magazzù
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pisa, 56127 Pisa, Italy
| | - Alessandra Toncelli
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pisa, 56127 Pisa, Italy
- Dipartimento di Fisica, Università di Pisa, 56127 Pisa, Italy
| | - Franco Spinella
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pisa, 56127 Pisa, Italy
| | - Sergio Saponara
- Dipartimento di Ingegneria dell’Informazione, Università di Pisa, 56122 Pisa, Italy
| | - Roberto Gunnella
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Perugia, 06123 Perugia, Italy
- Scuola di Scienze e Tecnologie, Università di Camerino, 62032 Camerino, Italy
| | - Francesco Rossella
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pavia, 27100 Pavia, Italy
- Dipartimento di Scienze Fisiche, Informatiche e Matematiche, Università di Modena e Reggio Emilia, 41125 Modena, Italy
| | - Andrea Salamon
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Roma Tor Vergata, 00133 Roma, Italy
| | - Vittorio Bellani
- Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Pavia, 27100 Pavia, Italy
- Dipartimento di Fisica, Università di Pavia, 27100 Pavia, Italy
| |
Collapse
|
4
|
Brini L, Bennour I, Toncelli A, Maalej R, Abdelhedi M. Eu-Doped Pyrochlore Crystal Nano-Powders as Fluorescent Solid for Fingerprint Visualization and for Anti-Counterfeiting Applications. Materials (Basel) 2022; 15:ma15072423. [PMID: 35407757 PMCID: PMC8999860 DOI: 10.3390/ma15072423] [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] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 02/16/2022] [Revised: 03/12/2022] [Accepted: 03/22/2022] [Indexed: 11/30/2022]
Abstract
Undoped Y2Sn2O7 and Eu3+ doped Y2Sn2O7 samples with doping concentrations 7%, 8%, 9%, and 10% are successfully synthesized by the co-precipitation method. A complete structural, morphological, and spectroscopic characterization is carried out. XRD measurements reveal that samples crystallize in the pure single pyrochlore phase and Eu3+ ions occupy sites with D3d symmetry. After mechanical grinding, the average crystallite size is less than 100 nm for all compositions. Optical characterization shows emission from the 5D0 level towards the lower lying 7F0,1,2,3,4 levels. The CIE color coordinates of all the pyrochlore phosphors are very close to those of the ideal red light. For the visualization of latent fingerprints, different surfaces are tested, including difficult ones (wood and ceramic), with excellent results. All three levels of fingerprint ridge patterns are visualized: core (Level 1), bifurcation and termination (Level 2), and sweat pores (Level 3). Moreover, our nano-powders are used to prepare a stable fluorescent ink.
Collapse
Affiliation(s)
- Layla Brini
- Laboratory of Inorganic Chemistry, Faculty of Sciences of Sfax, Sfax University, Sfax 3018, Tunisia; (L.B.); (M.A.)
| | - Ines Bennour
- Laboratory of Dielectric and Photonic Materials, Faculty of Sciences of Sfax, Sfax University, Sfax 3018, Tunisia; (I.B.); (R.M.)
| | - Alessandra Toncelli
- Dipartimento di Fisica, Università di Pisa, Largo B. Pontecorvo 3, I-56127 Pisa, Italy
- Istituto Nanoscienze CNR, Piazza San Silvestro 12, I-56127 Pisa, Italy
- Istituto Nazionale di Fisica Nucleare-Sezione di Pisa, Largo B. Pontecorvo 3, I-56127 Pisa, Italy
- Correspondence: ; Tel.: +39-050-2214-556
| | - Ramzi Maalej
- Laboratory of Dielectric and Photonic Materials, Faculty of Sciences of Sfax, Sfax University, Sfax 3018, Tunisia; (I.B.); (R.M.)
| | - Mohamed Abdelhedi
- Laboratory of Inorganic Chemistry, Faculty of Sciences of Sfax, Sfax University, Sfax 3018, Tunisia; (L.B.); (M.A.)
| |
Collapse
|
5
|
Toncelli A. RE-Based Inorganic-Crystal Nanofibers Produced by Electrospinning for Photonic Applications. Materials (Basel) 2021; 14:ma14102679. [PMID: 34065324 PMCID: PMC8160682 DOI: 10.3390/ma14102679] [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] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 04/09/2021] [Revised: 05/08/2021] [Accepted: 05/15/2021] [Indexed: 11/29/2022]
Abstract
Electrospinning is an effective and inexpensive technique to grow polymer materials in nanofiber shape with exceptionally high surface-area-to-volume ratio. Although it has been known for about a century, it has gained much interest in the new millennium thanks to its low cost and versatility, which has permitted to obtain a large variety of multifunctional compositions with a rich collection of new possible applications. Rare-earth doped materials possess many remarkable features that have been exploited, for example, for diode pumped bulk solid-state lasers in the visible and near infrared regions, or for biomedical applications when grown in nanometric form. In the last few decades, electrospinning preparation of rare-earth-doped crystal nanofibers has been developed and many different materials have been successfully grown. Crystal host, crystal quality and nanosized shape can deeply influence the optical properties of embedded rare earth ions; therefore, a large number of papers has recently been devoted to the growth and characterization of rare earth doped nanofibers with the electrospinning technique and an up-to-date review of this rapidly developing topic is missing; This review paper is devoted to the presentation of the main results obtained in this field up to now with particular insight into the optical characterization of the various materials grown with this technique.
Collapse
Affiliation(s)
- Alessandra Toncelli
- Dipartimento di Fisica “E. Fermi”, Università di Pisa, Largo B, Pontecorvo 3, 56127 Pisa, Italy;
- Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Largo B, Pontecorvo 3, 56127 Pisa, Italy
- Istituto Nanoscienze—CNR, Piazza S. Silvestro 12, 56127 Pisa, Italy
| |
Collapse
|
6
|
Turri G, Webster S, Bass M, Toncelli A. Temperature-Dependent Stimulated Emission Cross-Section in Nd 3+:YLF Crystal. Materials (Basel) 2021; 14:431. [PMID: 33467181 PMCID: PMC7830701 DOI: 10.3390/ma14020431] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 11/30/2020] [Revised: 12/30/2020] [Accepted: 01/06/2021] [Indexed: 11/16/2022]
Abstract
Spectroscopic properties of neodymium-doped yttrium lithium fluoride were measured at different temperatures from 35 K to 350 K in specimens with 1 at% Nd3+ concentration. The absorption spectrum was measured at room temperature from 400 to 900 nm. The decay dynamics of the 4F3/2 multiplet was investigated by measuring the fluorescence lifetime as a function of the sample temperature, and the radiative decay time was derived by extrapolation to 0 K. The stimulated-emission cross-sections of the transitions from the 4F3/2 to the 4I9/2, 4I11/2, and 4I13/2 levels were obtained from the fluorescence spectrum measured at different temperatures, using the Aull-Jenssen technique. The results show consistency with most results previously published at room temperature, extending them over a broader range of temperatures. A semi-empirical formula for the magnitude of the stimulated-emission cross-section as a function of temperature in the 250 K to 350 K temperature range, is presented for the most intense transitions to the 4I11/2 and 4I13/2 levels.
Collapse
Affiliation(s)
- Giorgio Turri
- Mathematics and Science Department, Full Sail University, 3300 University Blvd, Winter Park, FL 32792, USA;
| | - Scott Webster
- CREOL, The College of Optics and Photonics, University of Central Florida, 4304 Scorpius St., Orlando, FL 32816, USA; (S.W.); (M.B.)
| | - Michael Bass
- CREOL, The College of Optics and Photonics, University of Central Florida, 4304 Scorpius St., Orlando, FL 32816, USA; (S.W.); (M.B.)
| | - Alessandra Toncelli
- Physics Department, University of Pisa, Largo B. Pontecorvo 3, 56127 Pisa, Italy
- Italian National Research Council (CNR), Institute of Nanoscience (NANO), 56127 Pisa, Italy
| |
Collapse
|
7
|
Szewczyk PK, Gradys A, Kim SK, Persano L, Marzec M, Kryshtal A, Busolo T, Toncelli A, Pisignano D, Bernasik A, Kar-Narayan S, Sajkiewicz P, Stachewicz U. Enhanced Piezoelectricity of Electrospun Polyvinylidene Fluoride Fibers for Energy Harvesting. ACS Appl Mater Interfaces 2020; 12:13575-13583. [PMID: 32090543 PMCID: PMC7497623 DOI: 10.1021/acsami.0c02578] [Citation(s) in RCA: 49] [Impact Index Per Article: 12.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/10/2020] [Accepted: 02/24/2020] [Indexed: 05/10/2023]
Abstract
Piezoelectric polymers are promising energy materials for wearable and implantable applications for replacing bulky batteries in small and flexible electronics. Therefore, many research studies are focused on understanding the behavior of polymers at a molecular level and designing new polymer-based generators using polyvinylidene fluoride (PVDF). In this work, we investigated the influence of voltage polarity and ambient relative humidity in electrospinning of PVDF for energy-harvesting applications. A multitechnique approach combining microscopy and spectroscopy was used to study the content of the β-phase and piezoelectric properties of PVDF fibers. We shed new light on β-phase crystallization in electrospun PVDF and showed the enhanced piezoelectric response of the PVDF fiber-based generator produced with the negative voltage polarity at a relative humidity of 60%. Above all, we proved that not only crystallinity but also surface chemistry is crucial for improving piezoelectric performance in PVDF fibers. Controlling relative humidity and voltage polarity increased the d33 piezoelectric coefficient for PVDF fibers by more than three times and allowed us to generate a power density of 0.6 μW·cm-2 from PVDF membranes. This study showed that the electrospinning technique can be used as a single-step process for obtaining a vast spectrum of PVDF fibers exhibiting different physicochemical properties with β-phase crystallinity reaching up to 74%. The humidity and voltage polarity are critical factors in respect of chemistry of the material on piezoelectricity of PVDF fibers, which establishes a novel route to engineer materials for energy-harvesting and sensing applications.
Collapse
Affiliation(s)
- Piotr K. Szewczyk
- International Centre
of Electron Microscopy for Materials Science and Faculty of Metals
Engineering and Industrial Computer Science, AGH University of Science and Technology, 30-059 Krakow, Poland
| | - Arkadiusz Gradys
- Polish Academy of Sciences, Institute of Fundamental Technological Research, 02-106 Warszawa, Poland
| | - Sung Kyun Kim
- Department of Materials Science and Metallurgy, University of Cambridge, CB3 0FS Cambridge, U.K.
| | - Luana Persano
- Nanoscience Institute NANO, Italian National Research Council (CNR), 56127 Pisa, Italy
| | - Mateusz Marzec
- Academic Centre for Materials and Nanotechnology, AGH University of Science and Technology, 30-059 Krakow, Poland
| | - Aleksandr Kryshtal
- International Centre
of Electron Microscopy for Materials Science and Faculty of Metals
Engineering and Industrial Computer Science, AGH University of Science and Technology, 30-059 Krakow, Poland
| | - Tommaso Busolo
- Department of Materials Science and Metallurgy, University of Cambridge, CB3 0FS Cambridge, U.K.
| | - Alessandra Toncelli
- Nanoscience Institute NANO, Italian National Research Council (CNR), 56127 Pisa, Italy
- Department of Physics, University of Pisa, 56127 Pisa, Italy
| | - Dario Pisignano
- Nanoscience Institute NANO, Italian National Research Council (CNR), 56127 Pisa, Italy
- Department of Physics, University of Pisa, 56127 Pisa, Italy
| | - Andrzej Bernasik
- Academic Centre for Materials and Nanotechnology, AGH University of Science and Technology, 30-059 Krakow, Poland
- Faculty of Physics and Applied Computer Science, AGH University of Science and Technology, 30-059 Krakow, Poland
| | - Sohini Kar-Narayan
- Department of Materials Science and Metallurgy, University of Cambridge, CB3 0FS Cambridge, U.K.
| | - Paweł Sajkiewicz
- Polish Academy of Sciences, Institute of Fundamental Technological Research, 02-106 Warszawa, Poland
| | - Urszula Stachewicz
- International Centre
of Electron Microscopy for Materials Science and Faculty of Metals
Engineering and Industrial Computer Science, AGH University of Science and Technology, 30-059 Krakow, Poland
| |
Collapse
|
8
|
Carrasco I, Laversenne L, Bigotta S, Toncelli A, Tonelli M, Zagumennyi AI, Pollnau M. Super-quadratic upconversion luminescence among lanthanide ions. Opt Express 2019; 27:33217-33232. [PMID: 31878395 DOI: 10.1364/oe.27.033217] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/08/2023]
Abstract
We explore the arguably most fundamental aspect of energy-transfer upconversion (ETU), namely the dependence of upconversion luminescence from a higher-energy level, following ETU excitation from a metastable lower-energy level, on direct luminescence from that metastable level. We investigate ETU among neighboring Nd3+ ions in single crystals of GdVO4 and LaSc3(BO3)4 with different doping concentrations by measuring, after short-pulse laser excitation with different pump energies, the infrared luminescence decay from the metastable 4F3/2 level and the yellow upconversion luminescence decay from the 4G7/2 level. We observe a highly super-quadratic dependence of upconversion on direct luminescence intensity. We conclude that the commonly assumed quadratic law of ETU, as proposed by Grant's model and frequently employed in rate-equation simulations, is inadequate to the description of ETU processes. Whereas Zubenko's model, which considers a finite migration rate, provides significantly better fits to the experimental luminescence-decay curves, also this model cannot accurately reproduce the measured decay curves, partly because it does not take the non-homogeneous distribution of active ions into account.
Collapse
|
9
|
Pagano M, Baldacci L, Ottomaniello A, de Dato G, Chianucci F, Masini L, Carelli G, Toncelli A, Storchi P, Tredicucci A, Corona P. THz Water Transmittance and Leaf Surface Area: An Effective Nondestructive Method for Determining Leaf Water Content. Sensors (Basel) 2019; 19:E4838. [PMID: 31698861 PMCID: PMC6891343 DOI: 10.3390/s19224838] [Citation(s) in RCA: 12] [Impact Index Per Article: 2.4] [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: 09/28/2019] [Revised: 10/27/2019] [Accepted: 10/29/2019] [Indexed: 02/07/2023]
Abstract
Water availability is a major limiting factor in plant productivity and plays a key role in plant species distribution over a given area. New technologies, such as terahertz quantum cascade lasers (THz-QCLs) have proven to be non-invasive, effective, and accurate tools for measuring and monitoring leaf water content. This study explores the feasibility of using an advanced THz-QCL device for measuring the absolute leaf water content in Corylus avellana L., Laurus nobilis L., Ostrya carpinifolia Scop., Quercus ilex L., Quercus suber L., and Vitis vinifera L. (cv. Sangiovese). A recently proposed, simple spectroscopic technique was used, consisting in determining the transmission of the THz light beam through the leaf combined with a photographic measurement of the leaf area. A significant correlation was found between the product of the leaf optical depth (τ) and the leaf surface area (LA) with the leaf water mass (Mw) for all the studied species (Pearson's r test, p ≤ 0.05). In all cases, the best fit regression line, in the graphs of τLA as a function of Mw, displayed R2 values always greater than 0.85. The method proposed can be combined with water stress indices of plants in order to gain a better understanding of the leaf water management processes or to indirectly monitor the kinetics of leaf invasion by pathogenic bacteria, possibly leading to the development of specific models to study and fight them.
Collapse
Affiliation(s)
- Mario Pagano
- CREA—Research Centre for Plant Protection and Certification, Via di Lanciola 12/A, 50125 Firenze, Italy
- CREA—Research Centre for Viticulture and Enology, Viale Santa Margherita 80, 52100 Arezzo, Italy;
| | - Lorenzo Baldacci
- NEST, CNR—Istituto Nanoscienze and Scuola Normale Superiore, Piazza San Silvestro 12, 56124 Pisa, Italy; (L.B.); (A.O.); (L.M.); (A.T.)
| | - Andrea Ottomaniello
- NEST, CNR—Istituto Nanoscienze and Scuola Normale Superiore, Piazza San Silvestro 12, 56124 Pisa, Italy; (L.B.); (A.O.); (L.M.); (A.T.)
- Dipartimento di Fisica “E. Fermi”, Università di Pisa, Largo Bruno Pontecorvo 3, 56127 Pisa, Italy; (G.C.); (A.T.)
| | - Giovanbattista de Dato
- CREA—Research Centre for Forestry and Wood, Viale Santa Margherita 80, 52100 Arezzo, Italy; (G.d.D.); (F.C.); (P.C.)
| | - Francesco Chianucci
- CREA—Research Centre for Forestry and Wood, Viale Santa Margherita 80, 52100 Arezzo, Italy; (G.d.D.); (F.C.); (P.C.)
| | - Luca Masini
- NEST, CNR—Istituto Nanoscienze and Scuola Normale Superiore, Piazza San Silvestro 12, 56124 Pisa, Italy; (L.B.); (A.O.); (L.M.); (A.T.)
| | - Giorgio Carelli
- Dipartimento di Fisica “E. Fermi”, Università di Pisa, Largo Bruno Pontecorvo 3, 56127 Pisa, Italy; (G.C.); (A.T.)
| | - Alessandra Toncelli
- Dipartimento di Fisica “E. Fermi”, Università di Pisa, Largo Bruno Pontecorvo 3, 56127 Pisa, Italy; (G.C.); (A.T.)
| | - Paolo Storchi
- CREA—Research Centre for Viticulture and Enology, Viale Santa Margherita 80, 52100 Arezzo, Italy;
| | - Alessandro Tredicucci
- NEST, CNR—Istituto Nanoscienze and Scuola Normale Superiore, Piazza San Silvestro 12, 56124 Pisa, Italy; (L.B.); (A.O.); (L.M.); (A.T.)
- Dipartimento di Fisica “E. Fermi”, Università di Pisa, Largo Bruno Pontecorvo 3, 56127 Pisa, Italy; (G.C.); (A.T.)
| | - Piermaria Corona
- CREA—Research Centre for Forestry and Wood, Viale Santa Margherita 80, 52100 Arezzo, Italy; (G.d.D.); (F.C.); (P.C.)
| |
Collapse
|
10
|
Guglielmero L, Guazzelli L, Toncelli A, Chiappe C, Tredicucci A, Pomelli CS. An insight into the intermolecular vibrational modes of dicationic ionic liquids through far-infrared spectroscopy and DFT calculations. RSC Adv 2019; 9:30269-30276. [PMID: 35530250 PMCID: PMC9072084 DOI: 10.1039/c9ra05735h] [Citation(s) in RCA: 6] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/24/2019] [Accepted: 09/18/2019] [Indexed: 12/03/2022] Open
Abstract
Dicationic ionic liquids (DILs) are a subclass of the ionic liquid (IL) family and are characterized by two cationic head groups linked by means of a spacer. While DILs are increasingly attracting interest due to their peculiar physico-chemical properties, there is still a lack of understanding of their intermolecular interactions. Herein, we report our investigations on the intermolecular vibrational modes of two bromide DILs and of a bistriflimide DIL. The minimal possible neutral cluster of ions was studied as a simplified model of these systems and was optimized at the DFT level. Normal modes of two sandwich-like conformers were then calculated using the harmonic approximation with analytical computation of the second derivatives of molecular energy with respect to the atomic coordinates. The calculated spectra were compared to far-infrared experimental spectra and two groups of peaks over three, for the two bromide DILs, and three over five, for the Tf2N− DIL, were described by the proposed neutral cluster model. Therefore, this model represents a reliable and computationally affordable model for the exploration of the intermolecular interactions of this kind of system. The minimal cluster of ions represents a reliable and computationally affordable model for the exploration of the intermolecular interactions of dicationic ionic liquids.![]()
Collapse
Affiliation(s)
| | | | - Alessandra Toncelli
- Dipartimento di Fisica “E. Fermi” and Istituto Nanoscienze CNR
- Università di Pisa
- 56127 Pisa
- Italy
| | | | - Alessandro Tredicucci
- Dipartimento di Fisica “E. Fermi” and Istituto Nanoscienze CNR
- Università di Pisa
- 56127 Pisa
- Italy
- Laboratorio NEST
| | | |
Collapse
|
11
|
Sghedoni R, Coniglio A, Mazzoni LN, Busoni S, Belli G, Tarducci R, Nocetti L, Fedeli L, Esposito M, Ciccarone A, Altabella L, Bellini A, Binotto L, Caivano R, Carnì M, Ricci A, Cimolai S, D'Urso D, Gasperi C, Levrero F, Mangili P, Morzenti S, Nitrosi A, Oberhofer N, Parruccini N, Toncelli A, Valastro LM, Gori C, Gobbi G, Giannelli M. A straightforward multiparametric quality control protocol for proton magnetic resonance spectroscopy: Validation and comparison of various 1.5 T and 3 T clinical scanner systems. Phys Med 2018; 54:49-55. [PMID: 30337010 DOI: 10.1016/j.ejmp.2018.08.013] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.7] [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: 04/06/2018] [Revised: 07/25/2018] [Accepted: 08/13/2018] [Indexed: 02/08/2023] Open
Abstract
PURPOSE The aim of this study was to propose and validate across various clinical scanner systems a straightforward multiparametric quality assurance procedure for proton magnetic resonance spectroscopy (MRS). METHODS Eighteen clinical 1.5 T and 3 T scanner systems for MRS, from 16 centres and 3 different manufacturers, were enrolled in the study. A standard spherical water phantom was employed by all centres. The acquisition protocol included 3 sets of single (isotropic) voxel (size 20 mm) PRESS acquisitions with unsuppressed water signal and acquisition voxel position at isocenter as well as off-center, repeated 4/5 times within approximately 2 months. Water peak linewidth (LW) and area under the water peak (AP) were estimated. RESULTS LW values [mean (standard deviation)] were 1.4 (1.0) Hz and 0.8 (0.3) Hz for 3 T and 1.5 T scanners, respectively. The mean (standard deviation) (across all scanners) coefficient of variation of LW and AP for different spatial positions of acquisition voxel were 43% (20%) and 11% (11%), respectively. The mean (standard deviation) phantom T2values were 1145 (50) ms and 1010 (95) ms for 1.5 T and 3 T scanners, respectively. The mean (standard deviation) (across all scanners) coefficients of variation for repeated measurements of LW, AP and T2 were 25% (20%), 10% (14%) and 5% (2%), respectively. CONCLUSIONS We proposed a straightforward multiparametric and not time consuming quality control protocol for MRS, which can be included in routine and periodic quality assurance procedures. The protocol has been validated and proven to be feasible in a multicentre comparison study of a fairly large number of clinical 1.5 T and 3 T scanner systems.
Collapse
Affiliation(s)
| | - Angela Coniglio
- Medical Physics Unit, Ospedale San Giovanni Calibita Fatebenefratelli, Roma, Italy.
| | | | | | | | - Roberto Tarducci
- Health Physics Unit, Azienda Ospedaliera di Perugia, Perugia, Italy
| | - Luca Nocetti
- Health Physics Unit, Azienda Ospedaliera di Modena, Modena, Italy
| | - Luca Fedeli
- Physics and Astronomy Department, University of Florence, Firenze, Italy
| | - Marco Esposito
- Health Physics Unit, Azienda USL Toscana Centro, Firenze, Italy
| | | | | | | | - Luca Binotto
- Medical Physics Unit, Azienda ULSS 3 Serenissima, Mestre, Italy
| | - Rocchina Caivano
- Radiotherapy and Health Physics Unit, IRCCS CROB, Rionero in Vulture - Potenza, Italy
| | - Marco Carnì
- Health Physics Unit, Policlinico Umberto I, Roma, Italy
| | | | - Sara Cimolai
- Health Physics Unit, Azienda ULSS 2 Marca Trevigiana, Treviso, Italy
| | - Davide D'Urso
- Health Physics Unit, Azienda ULSS 2 Marca Trevigiana, Treviso, Italy
| | - Chiara Gasperi
- Health Physics Unit, Azienda USL Toscana Sud Est, Arezzo, Italy
| | - Fabrizio Levrero
- Medical and Health Physics Unit, IRCCS AOU San Martino, Genova, Italy
| | - Paola Mangili
- Medical Physics Unit, IRCCS San Raffaele, Milano, Italy
| | | | - Andrea Nitrosi
- Medical Physics Unit, Arcispedale Santa Maria Nuova - IRCCS, Reggio Emilia, Italy
| | - Nadia Oberhofer
- Health Physics, Azienda Sanitaria della Provincia Autonoma di Bolzano, Bolzano, Italy
| | | | | | | | - Cesare Gori
- Health Physics Unit, AOU Careggi, Firenze, Italy
| | - Gianni Gobbi
- Health Physics Unit, Azienda Ospedaliera di Perugia, Perugia, Italy
| | - Marco Giannelli
- Unit of Medical Physics, Pisa University Hospital "Azienda Ospedaliero-Universitaria Pisana", Pisa, Italy
| | | |
Collapse
|
12
|
Baldacci L, Pagano M, Masini L, Toncelli A, Carelli G, Storchi P, Tredicucci A. Non-invasive absolute measurement of leaf water content using terahertz quantum cascade lasers. Plant Methods 2017; 13:51. [PMID: 28638439 PMCID: PMC5474302 DOI: 10.1186/s13007-017-0197-z] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/04/2023]
Abstract
BACKGROUND Plant water resource management is one of the main future challenges to fight recent climatic changes. The knowledge of the plant water content could be indispensable for water saving strategies. Terahertz spectroscopic techniques are particularly promising as a non-invasive tool for measuring leaf water content, thanks to the high predominance of the water contribution to the total leaf absorption. Terahertz quantum cascade lasers (THz QCL) are one of the most successful sources of THz radiation. RESULTS Here we present a new method which improves the precision of THz techniques by combining a transmission measurement performed using a THz QCL source, with simple pictures of leaves taken by an optical camera. As a proof of principle, we performed transmission measurements on six plants of Vitis vinifera L. (cv "Colorino"). We found a linear law which relates the leaf water mass to the product between the leaf optical depth in the THz and the projected area. Results are in optimal agreement with the proposed law, which reproduces the experimental data with 95% accuracy. CONCLUSIONS This method may overcome the issues related to intra-variety heterogeneities and retrieve the leaf water mass in a fast, simple, and non-invasive way. In the future this technique could highlight different behaviours in preserving the water status during drought stress.
Collapse
Affiliation(s)
- Lorenzo Baldacci
- NEST, CNR Istituto Nanoscienze and Scuola Normale Superiore, Piazza San Silvestro 12, 56127 Pisa, Italy
| | - Mario Pagano
- Consiglio per la ricerca in agricoltura e l’analisi dell’economia agraria, Centro di ricerca per la Viticoltura e l’Enologia, Viale Santa Margherita 80, 52100 Arezzo, Italy
| | - Luca Masini
- NEST, CNR Istituto Nanoscienze and Scuola Normale Superiore, Piazza San Silvestro 12, 56127 Pisa, Italy
| | - Alessandra Toncelli
- NEST, CNR Istituto Nanoscienze and Dipartimento di Fisica, Università di Pisa, Largo Pontecorvo 3, 56127 Pisa, Italy
| | - Giorgio Carelli
- Dipartimento di Fisica, Università di Pisa, Largo Pontecorvo 3, 56127 Pisa, Italy
| | - Paolo Storchi
- Consiglio per la ricerca in agricoltura e l’analisi dell’economia agraria, Centro di ricerca per la Viticoltura e l’Enologia, Viale Santa Margherita 80, 52100 Arezzo, Italy
| | - Alessandro Tredicucci
- NEST, CNR Istituto Nanoscienze and Dipartimento di Fisica, Università di Pisa, Largo Pontecorvo 3, 56127 Pisa, Italy
| |
Collapse
|
13
|
Sghedoni R, Coniglio A, Belli G, Busoni S, Ciccarone A, Esposito M, Giannelli M, Mazzoni L, Nocetti L, Tarducci R, Altabella I, Anoja R, Berardi P, Bertolini N, Biagini C, Carnì M, Cesana P, Cimolai S, Clemente S, Fabbri E, Fedeli L, Filice S, Levrero F, Meliadò G, Mordini N, Morzenti S, Moscato A, Oberhofer N, Paruccini N, Ricci A, Romeo N, Scelfo D, Toncelli A, Torresin A, Tosetti M, Zucca I, Gori C. AIFM multicenter intercomparison of MR scanners for proton spectroscopy – preliminary results. Phys Med 2016. [DOI: 10.1016/j.ejmp.2016.01.459] [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] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/28/2022] Open
|
14
|
Toncelli A, Noeske R, Cosottini M, Costagli M, Domenici V, Tiberi G, Tosetti M. STEAM-MiTiS: An MR spectroscopy method for the detection of scalar-coupled metabolites and its application to glutamate at 7 T. Magn Reson Med 2014; 74:1515-22. [DOI: 10.1002/mrm.25556] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/03/2014] [Revised: 10/28/2014] [Accepted: 11/09/2014] [Indexed: 11/07/2022]
Affiliation(s)
| | - Ralph Noeske
- MR Applications and Workflow Development; GE Healthcare; Berlin Germany
| | - Mirco Cosottini
- Dipartimento di Ricerca Traslazionale e delle Nuove Tecnologie in Medicina e Chirurgia; University of Pisa; Pisa Italy
- Fondazione IMAGO7; Pisa Italy
| | - Mauro Costagli
- Fondazione IMAGO7; Pisa Italy
- Laboratorio di Fisica Medica e Biotecnologie per la Risonanza Magnetica IRCCS Fondazione Stella Maris; Pisa Italy
| | - Valentina Domenici
- Dipartimento di Chimica e Chimica Industriale; University of Pisa; Pisa Italy
| | - Gianluigi Tiberi
- Fondazione IMAGO7; Pisa Italy
- Laboratorio di Fisica Medica e Biotecnologie per la Risonanza Magnetica IRCCS Fondazione Stella Maris; Pisa Italy
| | - Michela Tosetti
- Fondazione IMAGO7; Pisa Italy
- Laboratorio di Fisica Medica e Biotecnologie per la Risonanza Magnetica IRCCS Fondazione Stella Maris; Pisa Italy
| |
Collapse
|
15
|
Aasi J, Abbott BP, Abbott R, Abbott T, Abernathy MR, Accadia T, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, Affeldt C, Agathos M, Aggarwal N, Aguiar OD, Ain A, Ajith P, Alemic A, Allen B, Allocca A, Amariutei D, Andersen M, Anderson R, Anderson SB, Anderson WG, Arai K, Araya MC, Arceneaux C, Areeda J, Aston SM, Astone P, Aufmuth P, Aulbert C, Austin L, 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, Behnke B, Bejger M, Beker MG, Belczynski C, Bell AS, Bell C, Bergmann G, Bersanetti D, Bertolini A, Betzwieser J, Beyersdorf PT, Bilenko IA, Billingsley G, Birch J, Biscans S, Bitossi M, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bloemen S, Blom M, 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, Bulik T, Bulten HJ, Buonanno A, Burman R, Buskulic D, Buy C, Cadonati L, Cagnoli G, Bustillo JC, Calloni E, Camp JB, Campsie P, Cannon KC, Canuel B, Cao J, Capano CD, Carbognani F, Carbone L, Caride S, Castiglia A, 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, Chow J, Christensen N, Chu Q, Chua SSY, Chung S, Ciani G, Clara F, Clark JA, Cleva F, Coccia E, Cohadon PF, Colla A, Collette C, Colombini M, Cominsky L, Constancio M, Conte A, Cook D, Corbitt TR, Cordier M, Cornish N, Corpuz A, Corsi A, Costa CA, Coughlin MW, Coughlin S, Coulon JP, Countryman S, Couvares P, Coward DM, Cowart M, Coyne DC, Coyne R, Craig K, Creighton JDE, Crowder SG, Cumming A, Cunningham L, Cuoco E, Dahl K, Canton TD, Damjanic M, Danilishin SL, D'Antonio S, Danzmann K, Dattilo V, Daveloza H, Davier M, Davies GS, Daw EJ, Day R, Dayanga T, 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, Di Fiore L, Di Lieto A, Di Palma I, Di Virgilio A, Donath A, Donovan F, Dooley KL, Doravari S, Dossa S, Douglas R, Downes TP, Drago M, Drever RWP, Driggers JC, Du Z, Dwyer S, Eberle T, Edo T, Edwards M, Effler A, Eggenstein H, Ehrens P, Eichholz J, Eikenberry SS, Endrőczi G, Essick R, Etzel T, Evans M, Evans T, Factourovich M, Fafone V, Fairhurst S, Fang Q, Farinon S, Farr B, Farr WM, Favata M, Fehrmann H, Fejer MM, Feldbaum D, Feroz F, Ferrante I, 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 J, Gammaitoni L, Gaonkar S, Garufi F, Gehrels N, Gemme G, Genin E, Gennai A, Ghosh S, Giaime JA, Giardina KD, Giazotto A, Gill C, 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 C, Gushwa K, Gustafson EK, Gustafson R, Hammer D, Hammond G, Hanke M, Hanks J, Hanna C, 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, Holt K, Hooper S, Hopkins P, Hosken DJ, Hough J, Howell EJ, Hu Y, Huerta E, Hughey B, Husa S, Huttner SH, Huynh M, Huynh-Dinh T, Ingram DR, Inta R, Isogai T, Ivanov A, Iyer BR, Izumi K, Jacobson M, James E, Jang H, Jaranowski P, Ji Y, Jiménez-Forteza F, Johnson WW, Jones DI, Jones R, Jonker RJG, Ju L, K H, Kalmus P, Kalogera V, Kandhasamy S, Kang G, Kanner JB, Karlen J, Kasprzack M, Katsavounidis E, Katzman W, Kaufer H, Kawabe K, Kawazoe F, Kéfélian F, Keiser GM, Keitel D, Kelley DB, Kells W, Khalaidovski A, Khalili FY, Khazanov EA, Kim C, Kim K, Kim N, Kim NG, 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, Kremin A, Kringel V, Królak A, Kuehn G, Kumar A, Kumar P, Kumar R, Kuo L, Kutynia A, Kwee P, Landry M, Lantz B, Larson S, Lasky PD, Lawrie C, Lazzarini A, Lazzaro C, Leaci P, Leavey S, Lebigot EO, Lee CH, Lee HK, Lee HM, Lee J, Leonardi M, Leong JR, Le Roux A, Leroy N, Letendre N, Levin Y, Levine B, Lewis J, Li TGF, Libbrecht K, Libson A, Lin AC, Littenberg TB, Litvine V, Lockerbie NA, Lockett V, Lodhia D, Loew K, Logue J, Lombardi AL, Lorenzini M, Loriette V, Lormand M, Losurdo G, Lough J, Lubinski MJ, Lück H, Luijten E, Lundgren AP, Lynch R, Ma Y, Macarthur J, Macdonald EP, MacDonald T, Machenschalk B, MacInnis M, Macleod DM, Magana-Sandoval F, Mageswaran M, Maglione C, Mailand K, Majorana E, Maksimovic I, Malvezzi V, Man N, Manca GM, Mandel I, Mandic V, Mangano V, Mangini N, 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, Matzner RA, Mavalvala N, 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, Meyers P, Miao H, Michel C, Mikhailov EE, Milano L, Milde S, Miller J, Minenkov Y, Mingarelli CMF, Mishra C, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Moe B, Moesta P, 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, Kumar DN, Nardecchia I, Naticchioni L, Nayak RK, Necula V, Nelemans G, Neri I, Neri M, Newton G, Nguyen T, Nitz A, Nocera F, Nolting D, Normandin MEN, Nuttall LK, Ochsner E, O'Dell J, Oelker E, Oh JJ, Oh SH, Ohme F, Oppermann P, O'Reilly B, 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, Paoletti R, Paris H, Pasqualetti A, Passaquieti R, Passuello D, Pedraza M, 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, Premachandra S, Prestegard T, Price LR, Prijatelj M, Privitera S, Prodi GA, Prokhorov L, Puncken O, Punturo M, Puppo P, Qin J, Quetschke V, Quintero E, Quiroga G, 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, Re V, Read J, Reed CM, Regimbau T, Reid S, Reitze DH, Rhoades E, Ricci F, Riles K, Robertson NA, Robinet F, Rocchi A, Rodruck M, Rolland L, Rollins JG, Romano JD, Romano R, Romanov G, Romie JH, Rosińska D, Rowan S, Rüdiger A, Ruggi P, Ryan K, Salemi F, Sammut L, Sandberg V, Sanders JR, Sannibale V, Santiago-Prieto I, Saracco E, Sassolas B, Sathyaprakash BS, Saulson PR, Savage R, Scheuer J, Schilling R, 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 D, Shah S, Shahriar MS, Shaltev M, 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 M, Smith RJE, Smith-Lefebvre ND, Son EJ, Sorazu B, Souradeep T, Sperandio L, Staley A, Stebbins J, 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, Tarabrin SP, Taylor R, Ter Braack APM, Thirugnanasambandam MP, Thomas M, Thomas P, Thorne KA, Thorne KS, Thrane E, Tiwari V, Tokmakov KV, Tomlinson C, Toncelli A, Tonelli M, Torre O, Torres CV, Torrie CI, Travasso F, Traylor G, Tse M, Ugolini D, Unnikrishnan CS, Urban AL, Urbanek K, Vahlbruch H, Vajente G, Valdes G, Vallisneri M, van den Brand JFJ, Van Den Broeck C, van der Putten S, 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, Verma SS, Vetrano F, Viceré A, Vincent-Finley R, Vinet JY, Vitale S, Vo T, Vocca H, Vorvick C, Vousden WD, Vyachanin SP, Wade A, Wade L, Wade M, Walker M, Wallace L, 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 T, Williamson AR, Willis JL, Willke B, Wimmer M, Winkler W, Wipf CC, Wiseman AG, Wittel H, Woan G, Worden J, Yablon J, Yakushin I, Yamamoto H, Yancey CC, Yang H, Yang Z, Yoshida S, Yvert M, Zadrożny A, Zanolin M, Zendri JP, Zhang F, Zhang L, Zhao C, Zhu XJ, Zucker ME, Zuraw S, Zweizig J. Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data. Phys Rev Lett 2014; 113:231101. [PMID: 25526109 DOI: 10.1103/physrevlett.113.231101] [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: 07/07/2014] [Indexed: 06/04/2023]
Abstract
Gravitational waves from a variety of sources are predicted to superpose to create a stochastic background. This background is expected to contain unique information from throughout the history of the Universe that is unavailable through standard electromagnetic observations, making its study of fundamental importance to understanding the evolution of the Universe. We carry out a search for the stochastic background with the latest data from the LIGO and Virgo detectors. Consistent with predictions from most stochastic gravitational-wave background models, the data display no evidence of a stochastic gravitational-wave signal. Assuming a gravitational-wave spectrum of Ω_{GW}(f)=Ω_{α}(f/f_{ref})^{α}, we place 95% confidence level upper limits on the energy density of the background in each of four frequency bands spanning 41.5-1726 Hz. In the frequency band of 41.5-169.25 Hz for a spectral index of α=0, we constrain the energy density of the stochastic background to be Ω_{GW}(f)<5.6×10^{-6}. For the 600-1000 Hz band, Ω_{GW}(f)<0.14(f/900 Hz)^{3}, a factor of 2.5 lower than the best previously reported upper limits. We find Ω_{GW}(f)<1.8×10^{-4} using a spectral index of zero for 170-600 Hz and Ω_{GW}(f)<1.0(f/1300 Hz)^{3} for 1000-1726 Hz, bands in which no previous direct limits have been placed. The limits in these four bands are the lowest direct measurements to date on the stochastic background. We discuss the implications of these results in light of the recent claim by the BICEP2 experiment of the possible evidence for inflationary gravitational waves.
Collapse
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
| | - T Accadia
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - F Acernese
- INFN, Sezione di Napoli, Complesso Universitario di Monte Sant'Angelo, I-80126 Napoli, Italy and Università di Salerno, Fisciano, I-84084 Salerno, Italy
| | - K Ackley
- University of Florida, Gainesville, Florida 32611, USA
| | - C Adams
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - T Adams
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - P Addesso
- Università di Salerno, Fisciano, I-84084 Salerno, 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
| | - A Ain
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - P Ajith
- Tata Institute for Fundamental Research, Mumbai 400005, 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
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Siena, I-53100 Siena, Italy
| | - D Amariutei
- University of Florida, Gainesville, Florida 32611, USA
| | - M Andersen
- Stanford University, Stanford, California 94305, USA
| | - R 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 Areeda
- California State University Fullerton, Fullerton, California 92831, USA
| | - S M Aston
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - P Astone
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - P Aufmuth
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - C Aulbert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - L Austin
- LIGO - California Institute of Technology, Pasadena, California 91125, USA
| | - 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
- INFN, Sezione di Napoli, Complesso Universitario di Monte Sant'Angelo, I-80126 Napoli, Italy and Università di Salerno, Fisciano, I-84084 Salerno, 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
| | - 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
- INFN, Sezione di Genova, I-16146 Genova, Italy and Università degli Studi di Genova, I-16146 Genova, Italy
| | - A Bertolini
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J Betzwieser
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - P T Beyersdorf
- San Jose State University, San Jose, California 95192, 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, Los Angeles 70754, USA
| | - S Biscans
- LIGO - Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - 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
| | - M Blom
- Nikhef, Science Park, 1098 XG Amsterdam, 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 des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, 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
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India and Washington State University, Pullman, Washington 99164, USA
| | - L Bosi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | | | - P R Brady
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - V B Braginsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - M Branchesi
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, 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, Los Angeles 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
| | - 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
- 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 Sant'Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte Sant'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
| | - A Castiglia
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - 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 Taiwan 300
| | - 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
| | - J Chow
- Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | | | - Q Chu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S S Y Chua
- Australian National University, Canberra, Australian Capital Territory 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
| | - J A Clark
- University of Massachusetts - Amherst, Amherst, Massachusetts 01003, USA
| | - F Cleva
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Coccia
- INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy and Università di Roma Tor Vergata, I-00133 Roma, 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
| | - M Cordier
- San Jose State University, San Jose, California 95192, USA
| | - N Cornish
- Montana State University, Bozeman, Montana 59717, USA
| | - A Corpuz
- Embry-Riddle Aeronautical University, Prescott, Azusa 86301, 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
| | - S Coughlin
- Northwestern University, Evanston, Illinois 60208, USA
| | - 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 Cowart
- LIGO - Livingston Observatory, Livingston, Los Angeles 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
| | - 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
| | - 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
| | - G Debreczeni
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklósút 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
| | - 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 Sant'Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte Sant'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
| | - S Dhurandhar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - M Díaz
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - L Di Fiore
- INFN, Sezione di Napoli, Complesso Universitario di Monte Sant'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
| | | | - A Donath
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - 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, Los Angeles 70754, USA
| | - S Dossa
- Carleton College, Northfield, Minnesota 55057, 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
- INFN, Gruppo Collegato di Trento, I-38050 Povo Trento, Italy and Università 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
| | - 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 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 Miklósút 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, Los Angeles 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
| | - 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
| | - 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, Los Angeles 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
| | - 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' Astrophysics Research Group, 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, Los Angeles 70754, USA
| | - P Fulda
- University of Florida, Gainesville, Florida 32611, USA
| | - M Fyffe
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - J 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 Sant'Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte Sant'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
| | - 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 and Washington State University, Pullman, Washington 99164, USA
| | - J A Giaime
- Louisiana State University, Baton Rouge, Louisiana 70803, USA and LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - K D Giardina
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - A Giazotto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Gill
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - 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' Astrophysics Research Group, 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, Azusa 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
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy
| | - C Guido
- LIGO - Livingston Observatory, Livingston, Los Angeles 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
| | - 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
- Perimeter Institute for Theoretical Physics, Ontario N2L 2Y5, Canada
| | - J Hanson
- LIGO - Livingston Observatory, Livingston, Los Angeles 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, Los Angeles 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
| | - K Holt
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - S Hooper
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P Hopkins
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - 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, Azusa 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, Los Angeles 70754, USA
| | - D R Ingram
- LIGO - Hanford Observatory, Richland, Washington 99352, USA
| | - R Inta
- The Pennsylvania State University, University Park, Pennsylvania 16802, 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
| | - E James
- LIGO - California Institute of Technology, Pasadena, California 91125, USA
| | - H Jang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - P Jaranowski
- Biał ystok University, 15-424 Biał ystok, Poland
| | - 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
| | - Haris K
- 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, Los Angeles 70754, USA
| | - H Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - 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
| | - 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
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea and Seoul National University, Seoul 151-742, Korea
| | - K Kim
- Hanyang University, Seoul 133-791, Korea
| | - N Kim
- Stanford University, Stanford, California 94305, USA
| | - N G 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, Los Angeles 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
| | - A Kremin
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Kringel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Królak
- IM-PAN, 00-956 Warsaw, Poland and NCBJ, 05-400 Świerk-Otwock, 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
| | - 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 Taiwan 300
| | | | - P Kwee
- LIGO - Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - 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, Victoria 3010, Australia
| | - C Lawrie
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - 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
- LIGO - Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Leonardi
- INFN, Gruppo Collegato di Trento, I-38050 Povo Trento, Italy and Università di Trento, I-38050 Povo, Trento, Italy
| | - J R Leong
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Le Roux
- LIGO - Livingston Observatory, Livingston, Los Angeles 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 and Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - 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
| | | | - V Litvine
- LIGO - California Institute of Technology, Pasadena, California 91125, 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, Azusa 86301, USA
| | - J Logue
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A L Lombardi
- University of Massachusetts - Amherst, Amherst, Massachusetts 01003, 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, Los Angeles 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
| | - E Luijten
- Northwestern University, Evanston, Illinois 60208, USA
| | - A P Lundgren
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Lynch
- LIGO - Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Y Ma
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J Macarthur
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - 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
| | | | - 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 Mangini
- University of Massachusetts - Amherst, Amherst, Massachusetts 01003, USA
| | | | - 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
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, 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
| | - R A Matzner
- The University of Texas at Austin, Austin, Texas 78712, USA
| | - N Mavalvala
- LIGO - Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, 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 and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - R McCarthy
- LIGO - Hanford Observatory, Richland, Washington 99352, USA
| | - D E McClelland
- Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - S C McGuire
- Southern University and A&M College, Baton Rouge, Los Angeles 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, Victoria 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
| | - P Meyers
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - 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 Sant'Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte Sant'Angelo, I-80126 Napoli, Italy
| | - S Milde
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - 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
| | - P Moesta
- Caltech-CaRT, Pasadena, California 91125, USA
| | - M Mohan
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S R P Mohapatra
- Syracuse University, Syracuse, New York 13244, USA and Rochester Institute of Technology, Rochester, New York 14623, USA
| | - 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 Miklósút 29-33, Hungary
| | - D Nanda Kumar
- University of Florida, Gainesville, Florida 32611, USA
| | - 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
- INFN, Sezione di Genova, I-16146 Genova, Italy and Università degli Studi di Genova, I-16146 Genova, Italy
| | - G Newton
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Nguyen
- Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A 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, Los Angeles 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
| | - P Oppermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B O'Reilly
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - 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, Los Angeles 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 Taiwan 300
| | - 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
| | - R Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Siena, I-53100 Siena, Italy
| | - H Paris
- LIGO - Hanford Observatory, Richland, Washington 99352, 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
| | - 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
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy
| | - V Pierro
- INFN, Sezione di Genova, I-16146 Genova, Italy and University of Sannio at Benevento, I-82100 Benevento, Italy
| | - L Pinard
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - I M Pinto
- INFN, Sezione di Genova, I-16146 Genova, Italy and University of Sannio at Benevento, I-82100 Benevento, 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
| | | | - 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
- INFN, Gruppo Collegato di Trento, I-38050 Povo Trento, Italy and Università 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
| | - 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
| | - G Quiroga
- Argentinian Gravitational Wave Group, Cordoba, Cordoba 5000, Argentina
| | | | - 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 Miklósút 29-33, Hungary
| | - H Radkins
- LIGO - Hanford Observatory, Richland, Washington 99352, USA
| | - P Raffai
- MTA Eötvös University, 'Lendulet' Astrophysics Research Group, 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, Los Angeles 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
| | - V Re
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - J Read
- California State University Fullerton, Fullerton, California 92831, USA
| | - 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
| | - E Rhoades
- Embry-Riddle Aeronautical University, Prescott, Azusa 86301, USA
| | - F Ricci
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - 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
| | - M Rodruck
- LIGO - Hanford Observatory, Richland, Washington 99352, 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
| | - J D Romano
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - R Romano
- INFN, Sezione di Napoli, Complesso Universitario di Monte Sant'Angelo, I-80126 Napoli, Italy and Università di Salerno, Fisciano, I-84084 Salerno, Italy
| | - G Romanov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - J H Romie
- LIGO - Livingston Observatory, Livingston, Los Angeles 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, Victoria 3010, Australia
| | - V Sandberg
- LIGO - Hanford Observatory, Richland, Washington 99352, USA
| | - J R Sanders
- University of Michigan, Ann Arbor, Michigan 48109, 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
| | - 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, Australian Capital Territory 0200, Australia
| | - D Sellers
- LIGO - Livingston Observatory, Livingston, Los Angeles 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 Shaddock
- Australian National University, Canberra, Australian Capital Territory 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
| | - 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, Australian Capital Territory 0200, Australia
| | - J Slutsky
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J R Smith
- California State University Fullerton, Fullerton, California 92831, USA
| | - M 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
| | - L Sperandio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Staley
- Columbia University, New York, New York 10027, USA
| | - J Stebbins
- Stanford University, Stanford, California 94305, USA
| | - J Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and Instituto de Física Teórica, Universidade Estadual Paulista/International Center for Theoretical Physics-South American Institue for Research, São Paulo, São Paulo 01140-070, Brazil
| | - A L Stuver
- LIGO - Livingston Observatory, Livingston, Los Angeles 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
| | - 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
| | | | | | - M Thomas
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, USA
| | - P Thomas
- LIGO - Hanford Observatory, Richland, Washington 99352, USA
| | - K A Thorne
- LIGO - Livingston Observatory, Livingston, Los Angeles 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
| | - A Toncelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - O Torre
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Siena, I-53100 Siena, 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, Los Angeles 70754, USA
| | - M Tse
- LIGO - Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA and Columbia University, New York, New York 10027, USA
| | - D Ugolini
- Trinity University, San Antonio, Texas 78212, USA
| | | | - A L Urban
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - K Urbanek
- Stanford University, Stanford, California 94305, 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
| | | | - 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 Miklósút 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
| | - S S Verma
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - F Vetrano
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy
| | - A Viceré
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy
| | - R Vincent-Finley
- Southern University and A&M College, Baton Rouge, Los Angeles 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 Wade
- Australian National University, Canberra, Australian Capital Territory 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
| | - M Wang
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - X Wang
- Tsinghua University, Beijing 100084, China
| | - R L Ward
- Australian National University, Canberra, Australian Capital Territory 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, Los Angeles 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, Los Angeles 70813, USA
| | - L Williams
- University of Florida, Gainesville, Florida 32611, USA
| | - R Williams
- LIGO - California Institute of Technology, Pasadena, California 91125, USA
| | - T Williams
- Southeastern Louisiana University, Hammond, Los Angeles 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
| | - J Worden
- LIGO - Hanford Observatory, Richland, Washington 99352, USA
| | - J Yablon
- Northwestern University, Evanston, Illinois 60208, USA
| | - I Yakushin
- LIGO - Livingston Observatory, Livingston, Los Angeles 70754, 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
| | - Z Yang
- Tsinghua University, Beijing 100084, China
| | - S Yoshida
- Southeastern Louisiana University, Hammond, Los Angeles 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, Azusa 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
| | - 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
| |
Collapse
|
16
|
Aasi J, Abadie J, Abbott BP, Abbott R, Abbott T, Abernathy MR, Accadia T, Acernese F, Adams C, Adams T, Adhikari RX, Affeldt C, Agathos M, Aggarwal N, Aguiar OD, Ajith P, Allen B, Allocca A, Amador Ceron E, Amariutei D, Anderson RA, Anderson SB, Anderson WG, Arai K, Araya MC, Arceneaux C, Areeda J, Ast S, Aston SM, Astone P, Aufmuth P, Aulbert C, Austin L, Aylott BE, Babak S, Baker PT, Ballardin G, Ballmer SW, Barayoga JC, Barker D, Barnum SH, Barone F, Barr B, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Basti A, Batch J, Bauchrowitz J, Bauer TS, Bebronne M, Behnke B, Bejger M, Beker MG, Bell AS, Bell C, Belopolski I, Bergmann G, Berliner JM, Bersanetti D, Bertolini A, Bessis D, Betzwieser J, Beyersdorf PT, Bhadbhade T, Bilenko IA, Billingsley G, Birch J, Bitossi M, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Blom M, Bock O, Bodiya TP, Boer M, Bogan C, Bond C, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Boschi V, Bose S, Bosi L, Bowers J, Bradaschia C, Brady PR, Braginsky VB, Branchesi M, Brannen CA, Brau JE, Breyer J, Briant T, Bridges DO, Brillet A, Brinkmann M, Brisson V, Britzger M, Brooks AF, Brown DA, Brown DD, Brückner F, Bulik T, Bulten HJ, Buonanno A, Buskulic D, Buy C, Byer RL, 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, Castiglia A, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Cella G, Cepeda C, Cesarini E, Chakraborty R, Chalermsongsak T, Chao S, Charlton P, Chassande-Mottin E, Chen X, Chen Y, Chincarini A, Chiummo A, Cho HS, Chow J, Christensen N, Chu Q, Chua SSY, Chung S, Ciani G, Clara F, Clark DE, Clark JA, Cleva F, Coccia E, Cohadon PF, Colla A, Colombini M, Constancio M, Conte A, Conte R, Cook D, Corbitt TR, Cordier M, Cornish N, Corsi A, Costa CA, Coughlin MW, Coulon JP, Countryman S, Couvares P, Coward DM, Cowart M, Coyne DC, Craig K, Creighton JDE, Creighton TD, Crowder SG, Cumming A, Cunningham L, Cuoco E, Dahl K, Dal Canton T, Damjanic M, Danilishin SL, D'Antonio S, Danzmann K, Dattilo V, Daudert B, Daveloza H, Davier M, Davies GS, Daw EJ, Day R, Dayanga T, De Rosa R, Debreczeni G, Degallaix J, Del Pozzo W, Deleeuw E, Deléglise S, Denker T, Dent T, Dereli H, Dergachev V, DeRosa R, DeSalvo R, Dhurandhar S, Di Fiore L, Di Lieto A, Di Palma I, Di Virgilio A, Díaz M, Dietz A, Dmitry K, Donovan F, Dooley KL, Doravari S, Drago M, Drever RWP, Driggers JC, Du Z, Dumas JC, Dwyer S, Eberle T, Edwards M, Effler A, Ehrens P, Eichholz J, Eikenberry SS, Endrőczi G, Essick R, Etzel T, Evans K, Evans M, Evans T, Factourovich M, Fafone V, Fairhurst S, Fang Q, Farinon S, Farr B, Farr W, Favata M, Fazi D, Fehrmann H, Feldbaum D, Ferrante I, Ferrini F, Fidecaro F, Finn LS, Fiori I, Fisher R, Flaminio R, Foley E, Foley S, Forsi E, Fotopoulos N, Fournier JD, Franco S, Frasca S, Frasconi F, Frede M, Frei M, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fujimoto MK, Fulda P, Fyffe M, Gair J, Gammaitoni L, Garcia J, Garufi F, Gehrels N, Gemme G, Genin E, Gennai A, Gergely L, Ghosh S, Giaime JA, Giampanis S, Giardina KD, Giazotto A, Gil-Casanova S, Gill C, Gleason J, Goetz E, Goetz R, Gondan L, González G, Gordon N, Gorodetsky ML, Gossan S, Goßler S, Gouaty R, Graef C, Graff PB, Granata M, Grant A, Gras S, Gray C, Greenhalgh RJS, Gretarsson AM, Griffo C, Groot P, Grote H, Grover K, Grunewald S, Guidi GM, Guido C, Gushwa KE, Gustafson EK, Gustafson R, Hall B, Hall E, Hammer D, Hammond G, Hanke M, Hanks J, Hanna C, Hanson J, Harms J, Harry GM, Harry IW, Harstad ED, Hartman MT, Haughian K, Hayama K, Heefner J, Heidmann A, Heintze M, Heitmann H, Hello P, Hemming G, Hendry M, Heng IS, Heptonstall AW, Heurs M, Hild S, Hoak D, Hodge KA, Holt K, Holtrop M, Hong T, Hooper S, Horrom T, Hosken DJ, Hough J, Howell EJ, Hu Y, Hua Z, Huang V, Huerta EA, Hughey B, Husa S, Huttner SH, Huynh M, Huynh-Dinh T, Iafrate J, Ingram DR, Inta R, Isogai T, Ivanov A, Iyer BR, Izumi K, Jacobson M, James E, Jang H, Jang YJ, Jaranowski P, Jiménez-Forteza F, Johnson WW, Jones D, Jones DI, Jones R, Jonker RJG, Ju L, K H, Kalmus P, Kalogera V, Kandhasamy S, Kang G, Kanner JB, Kasprzack M, Kasturi R, Katsavounidis E, Katzman W, Kaufer H, Kaufman K, Kawabe K, Kawamura S, Kawazoe F, Kéfélian F, Keitel D, Kelley DB, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khazanov EA, Kim BK, Kim C, Kim K, Kim N, Kim W, 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 D, Kremin A, Kringel V, Królak A, Kucharczyk C, Kudla S, Kuehn G, Kumar A, Kumar P, Kumar R, Kurdyumov R, Kwee P, Landry M, Lantz B, Larson S, Lasky PD, Lawrie C, Lazzarini A, Le Roux A, Leaci P, Lebigot EO, Lee CH, Lee HK, Lee HM, Lee J, Lee J, Leonardi M, Leong JR, Leroy N, Letendre N, Levine B, Lewis JB, Lhuillier V, Li TGF, Lin AC, Littenberg TB, Litvine V, Liu F, Liu H, Liu Y, Liu Z, Lloyd D, Lockerbie NA, Lockett V, Lodhia D, Loew K, Logue J, Lombardi AL, Lorenzini M, Loriette V, Lormand M, Losurdo G, Lough J, Luan J, Lubinski MJ, Lück H, Lundgren AP, Macarthur J, Macdonald E, Machenschalk B, MacInnis M, Macleod DM, Magana-Sandoval F, Mageswaran M, Mailand K, Majorana E, Maksimovic I, Malvezzi V, Man N, Manca GM, Mandel I, Mandic V, Mangano V, 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, Matzner RA, Mavalvala N, May G, Mazumder N, Mazzolo G, McCarthy R, McClelland DE, McGuire SC, McIntyre G, McIver J, Meacher D, Meadors GD, Mehmet M, Meidam J, Meier T, Melatos A, Mendell G, Mercer RA, Meshkov S, Messenger C, Meyer MS, Miao H, Michel C, Mikhailov EE, Milano L, Miller J, Minenkov Y, Mingarelli CMF, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Moe B, Mohan M, Mohapatra SRP, Mokler F, Moraru D, Moreno G, Morgado N, Mori T, 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, Nanda Kumar D, Nardecchia I, Nash T, Naticchioni L, Nayak R, Necula V, Nelemans G, Neri I, Neri M, Newton G, Nguyen T, Nishida E, Nishizawa A, Nitz A, Nocera F, Nolting D, Normandin ME, Nuttall LK, Ochsner E, O'Dell J, Oelker E, Ogin GH, Oh JJ, Oh SH, Ohme F, Oppermann P, O'Reilly B, Ortega Larcher W, O'Shaughnessy R, Osthelder C, Ott CD, Ottaway DJ, Ottens RS, Ou J, Overmier H, Owen BJ, Padilla C, Pai A, Palomba C, Pan Y, Pankow C, Paoletti F, Paoletti R, Papa MA, Paris H, Pasqualetti A, Passaquieti R, Passuello D, Pedraza M, Peiris P, Penn S, Perreca A, Phelps M, Pichot M, Pickenpack M, Piergiovanni F, Pierro V, Pinard L, Pindor B, Pinto IM, Pitkin M, Poeld J, Poggiani R, Poole V, Poux C, Predoi V, Prestegard T, Price LR, Prijatelj M, Principe M, Privitera S, Prix R, Prodi GA, Prokhorov L, Puncken O, Punturo M, Puppo P, 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, Rapagnani P, Raymond V, Re V, Reed CM, Reed T, Regimbau T, Reid S, Reitze DH, Ricci F, Riesen R, Riles K, Robertson NA, Robinet F, Rocchi A, Roddy S, Rodriguez C, Rodruck M, Roever C, 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 J, Sannibale V, Santiago-Prieto I, Saracco E, Sassolas B, Sathyaprakash BS, Saulson PR, Savage R, Schilling R, Schnabel R, Schofield RMS, Schreiber E, Schuette D, Schulz B, Schutz BF, Schwinberg P, Scott J, Scott SM, Seifert F, Sellers D, Sengupta AS, Sentenac D, Sergeev A, Shaddock D, Shah S, Shahriar MS, Shaltev M, Shapiro B, Shawhan P, Shoemaker DH, Sidery TL, Siellez K, Siemens X, Sigg D, Simakov D, Singer A, Singer L, Sintes AM, Skelton GR, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith RJE, Smith-Lefebvre ND, Soden K, Son EJ, Sorazu B, Souradeep T, Sperandio L, Staley A, Steinert E, Steinlechner J, Steinlechner S, Steplewski S, Stevens D, Stochino A, Stone R, Strain KA, Straniero N, Strigin S, Stroeer AS, Sturani R, Stuver AL, Summerscales TZ, Susmithan S, Sutton PJ, Swinkels B, Szeifert G, Tacca M, Talukder D, Tang L, Tanner DB, Tarabrin SP, Taylor R, ter Braack APM, Thirugnanasambandam MP, Thomas M, Thomas P, Thorne KA, Thorne KS, Thrane E, Tiwari V, Tokmakov KV, Tomlinson C, Toncelli A, Tonelli M, Torre O, Torres CV, Torrie CI, Travasso F, Traylor G, Tse M, Ugolini D, Unnikrishnan CS, Vahlbruch H, Vajente G, Vallisneri M, van den Brand JFJ, Van Den Broeck C, van der Putten S, 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, Verma S, Vetrano F, Viceré A, Vincent-Finley R, Vinet JY, Vitale S, Vlcek B, Vo T, Vocca H, Vorvick C, Vousden WD, Vrinceanu D, Vyachanin SP, Wade A, Wade L, Wade M, Waldman SJ, Walker M, Wallace L, Wan Y, Wang J, Wang M, Wang X, Wanner A, 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, Whitcomb SE, White DJ, Whiting BF, Wibowo S, Wiesner K, Wilkinson C, Williams L, Williams R, Williams T, Willis JL, Willke B, Wimmer M, Winkelmann L, Winkler W, Wipf CC, Wittel H, Woan G, Worden J, Yablon J, Yakushin I, Yamamoto H, Yancey CC, Yang H, Yeaton-Massey D, Yoshida S, Yum H, Yvert M, Zadrożny A, Zanolin M, Zendri JP, Zhang F, Zhang L, Zhao C, Zhu H, Zhu XJ, Zotov N, Zucker ME, Zweizig J. Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors. Phys Rev Lett 2014; 112:131101. [PMID: 24745400 DOI: 10.1103/physrevlett.112.131101] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/25/2013] [Indexed: 06/03/2023]
Abstract
Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising observational signature. In this Letter we present a search for GWs from cosmic string cusps in data collected by the LIGO and Virgo gravitational wave detectors between 2005 and 2010, with over 625 days of live time. We find no evidence of GW signals from cosmic strings. From this result, we derive new constraints on cosmic string parameters, which complement and improve existing limits from previous searches for a stochastic background of GWs from cosmic microwave background measurements and pulsar timing data. In particular, if the size of loops is given by the gravitational backreaction scale, we place upper limits on the string tension Gμ below 10(-8) in some regions of the cosmic string parameter space.
Collapse
Affiliation(s)
- J Aasi
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - J Abadie
- 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
| | - T Accadia
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - F Acernese
- INFN, Sezione di Napoli, Complesso Universitario di Monte S.Angelo, I-80126 Napoli, Italy and Università di Salerno, Fisciano, I-84084 Salerno, Italy
| | - C Adams
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Adams
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - 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, SP, Brazil
| | - P Ajith
- LIGO-California Institute of Technology, Pasadena, California 91125, 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
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Siena, I-53100 Siena, Italy
| | - E Amador Ceron
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - D Amariutei
- University of Florida, Gainesville, Florida 32611, 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 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
| | - C Aulbert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - L Austin
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - 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
| | - D Barker
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - S H Barnum
- LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - F Barone
- INFN, Sezione di Napoli, Complesso Universitario di Monte S.Angelo, I-80126 Napoli, Italy and Università di Salerno, Fisciano, I-84084 Salerno, 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
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom and 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 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
| | - M Bebronne
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - 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
| | - A S Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - I Belopolski
- Columbia University, New York, New York 10027, USA
| | - G Bergmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J M Berliner
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - D Bersanetti
- INFN, Sezione di Genova, I-16146 Genova, Italy and Università degli Studi di Genova, I-16146 Genova, Italy
| | - A Bertolini
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - D Bessis
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - J Betzwieser
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P T Beyersdorf
- San Jose State University, San Jose, California 95192, USA
| | - T Bhadbhade
- Stanford University, Stanford, California 94305, USA
| | - I A Bilenko
- Moscow State University, Moscow 119992, Russia
| | - G Billingsley
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - J Birch
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - 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, WA 6009, Australia
| | - M Blom
- Nikhef, Science Park, 1098 XG Amsterdam, 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
| | - 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 des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, 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
| | - S Bose
- Washington State University, Pullman, Washington 99164, USA
| | - L Bosi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - J Bowers
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | | | - P R Brady
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | | | - M Branchesi
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
| | - C A Brannen
- Washington State University, Pullman, Washington 99164, USA
| | - J E Brau
- University of Oregon, Eugene, Oregon 97403, USA
| | - J Breyer
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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
| | - M Britzger
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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
| | - 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
| | - 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
| | - R L Byer
- Stanford University, Stanford, California 94305, USA
| | - L Cadonati
- 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 M5 S 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
| | - A Castiglia
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - 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
| | - 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 Chao
- National Tsing Hua University, Hsinchu Taiwan 300
| | - P Charlton
- Charles Sturt University, Wagga Wagga, NSW 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, WA 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
| | - J Chow
- Australian National University, Canberra, ACT 0200, Australia
| | | | - Q Chu
- University of Western Australia, Crawley, WA 6009, Australia
| | - S S Y Chua
- Australian National University, Canberra, ACT 0200, Australia
| | - S Chung
- University of Western Australia, Crawley, WA 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
| | - F Cleva
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Coccia
- INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy and Università di Roma Tor Vergata, I-00133 Roma, 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
| | - M Colombini
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - M Constancio
- Instituto Nacional de Pesquisas Espaciais, 12227-010, São José dos Campos, SP, Brazil
| | - A Conte
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R Conte
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN (Sezione di Napoli), Italy
| | - D Cook
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - T R Corbitt
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - M Cordier
- San Jose State University, San Jose, California 95192, 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, SP, 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, WA 6009, Australia
| | - M Cowart
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D C Coyne
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - K Craig
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J D E Creighton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T D Creighton
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - 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
| | - 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, WA 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
| | - B Daudert
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - 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
| | - 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
| | - 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
| | - W Del Pozzo
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - E Deleeuw
- University of Florida, Gainesville, Florida 32611, USA
| | - S Deléglise
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - 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 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), Italy
| | - S Dhurandhar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - 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
| | | | - M Díaz
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - A Dietz
- The University of Mississippi, University, Mississippi 38677, USA
| | - K Dmitry
- Moscow State University, Moscow 119992, Russia
| | - 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
| | - M Drago
- INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy and Università di Trento, I-38050 Povo, Trento, Italy
| | - R W P Drever
- 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
| | - J-C Dumas
- University of Western Australia, Crawley, WA 6009, Australia
| | - S Dwyer
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - T Eberle
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Edwards
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Effler
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - 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
| | - K Evans
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - 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
| | - Q Fang
- University of Western Australia, Crawley, WA 6009, Australia
| | - S Farinon
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Farr
- Northwestern University, Evanston, Illinois 60208, USA
| | - W Farr
- Northwestern University, Evanston, Illinois 60208, USA
| | - 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
| | - D Feldbaum
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA and University of Florida, Gainesville, Florida 32611, USA
| | - I Ferrante
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - 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 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
| | - E Foley
- California State University Fullerton, Fullerton, California 92831, USA
| | - S Foley
- LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - E Forsi
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - N Fotopoulos
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - 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
| | - M Frei
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - Z Frei
- MTA-Eotvos 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
| | - M-K Fujimoto
- National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
| | - P Fulda
- University of Florida, Gainesville, Florida 32611, USA
| | - M Fyffe
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J 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
| | - J Garcia
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - 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
| | - E Genin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Gennai
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - L Gergely
- MTA-Eotvos University, "Lendulet" A. R. G., Budapest 1117, Hungary
| | - S Ghosh
- Washington State University, Pullman, Washington 99164, USA
| | - J A Giaime
- Louisiana State University, Baton Rouge, Louisiana 70803, USA and LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Giampanis
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - K D Giardina
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Giazotto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - S Gil-Casanova
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - C Gill
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - 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-Eotvos 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
| | | | - 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 Graef
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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
| | - C Griffo
- California State University Fullerton, Fullerton, California 92831, 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
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
| | - C Guido
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K E 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
| | - B Hall
- Washington State University, Pullman, Washington 99164, USA
| | - E Hall
- LIGO-California Institute of Technology, Pasadena, California 91125, 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
- Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada
| | - 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 T Hartman
- University of Florida, Gainesville, Florida 32611, USA
| | - K Haughian
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - K Hayama
- National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
| | - J Heefner
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - A Heidmann
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - M Heintze
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA and University of Florida, Gainesville, Florida 32611, 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
| | - 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
| | - K Holt
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Holtrop
- University of New Hampshire, Durham, New Hampshire 03824, USA
| | - T Hong
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Hooper
- University of Western Australia, Crawley, WA 6009, Australia
| | - T Horrom
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - D J Hosken
- University of Adelaide, Adelaide, SA 5005, Australia
| | - J Hough
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Howell
- University of Western Australia, Crawley, WA 6009, Australia
| | - Y Hu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - Z Hua
- Tsinghua University, Beijing 100084, China
| | - V Huang
- National Tsing Hua University, Hsinchu Taiwan 300
| | - E A 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
| | - J Iafrate
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D R Ingram
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - R Inta
- Australian National University, Canberra, ACT 0200, Australia
| | - 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
| | - E James
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - H Jang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - Y J Jang
- Northwestern University, Evanston, Illinois 60208, USA
| | | | | | - W W Johnson
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D Jones
- LIGO-Hanford Observatory, Richland, Washington 99352, 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, WA 6009, Australia
| | - Haris K
- 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
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - G Kang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - J B Kanner
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - M Kasprzack
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy and LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - R Kasturi
- Hobart and William Smith Colleges, Geneva, New York 14456, USA
| | - 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
| | - K Kaufman
- Caltech-CaRT, Pasadena, California 91125, USA
| | - K Kawabe
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - S Kawamura
- National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
| | - 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
| | - 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
- Moscow State University, Moscow 119992, Russia
| | - E A Khazanov
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - B K Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - C Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea and Seoul National University, Seoul 151-742, Korea
| | - K Kim
- Hanyang University, Seoul 133-791, Korea
| | - N Kim
- Stanford University, Stanford, California 94305, USA
| | - W Kim
- University of Adelaide, Adelaide, SA 5005, Australia
| | - Y-M Kim
- Pusan National University, Busan 609-735, Korea
| | - E J King
- University of Adelaide, Adelaide, SA 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-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, 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 Kozak
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - A Kremin
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Kringel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Królak
- IM-PAN, 00-956 Warsaw, Poland and NCBJ, 05-400 Świerk-Otwock, Poland
| | - C Kucharczyk
- Stanford University, Stanford, California 94305, USA
| | - S Kudla
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - G Kuehn
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Kumar
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - P Kumar
- Syracuse University, Syracuse, New York 13244, USA
| | - R Kumar
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Kurdyumov
- Stanford University, Stanford, California 94305, USA
| | - P Kwee
- LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Landry
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - B Lantz
- Stanford University, Stanford, California 94305, USA
| | - S Larson
- Utah State University, Logan, Utah 84322, USA
| | - P D Lasky
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - C Lawrie
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Lazzarini
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - A Le Roux
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Leaci
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | | | - 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
- LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J Lee
- California State University Fullerton, Fullerton, California 92831, USA
| | - M Leonardi
- INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy and Università di Trento, I-38050 Povo, Trento, Italy
| | - J R Leong
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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
| | - B Levine
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - J B Lewis
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - V Lhuillier
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - T G F Li
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - A C Lin
- Stanford University, Stanford, California 94305, USA
| | | | - V Litvine
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - F Liu
- University of Brussels, Brussels 1050 Belgium
| | - H Liu
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - Y Liu
- Tsinghua University, Beijing 100084, China
| | - Z Liu
- University of Florida, Gainesville, Florida 32611, USA
| | - D Lloyd
- LIGO-California Institute of Technology, Pasadena, California 91125, 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
| | - M Lorenzini
- INFN, Sezione 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
| | - J Luan
- Caltech-CaRT, Pasadena, California 91125, 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
| | - J Macarthur
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Macdonald
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - 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
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - F Magana-Sandoval
- California State University Fullerton, Fullerton, California 92831, USA
| | - M Mageswaran
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - 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
| | - 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
| | | | - 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
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, 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
| | - R A Matzner
- The University of Texas at Austin, Austin, Texas 78712, 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
| | - 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
| | - T Meier
- 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
| | - 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
- Australian National University, Canberra, ACT 0200, Australia
| | - Y Minenkov
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - S Mitra
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | | | | | - R Mittleman
- LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - B Moe
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Mohan
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S R P Mohapatra
- Syracuse University, Syracuse, New York 13244, USA and Rochester Institute of Technology, Rochester, New York 14623, USA
| | - F Mokler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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
| | - T Mori
- National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
| | - 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, SA 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
| | - D Nanda Kumar
- University of Florida, Gainesville, Florida 32611, USA
| | - I Nardecchia
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - T Nash
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - L Naticchioni
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R 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
- INFN, Sezione di Genova, I-16146 Genova, Italy and Università degli Studi 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
| | - E Nishida
- National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
| | - A Nishizawa
- National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
| | - A 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 Normandin
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - L K Nuttall
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - 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
| | - G H Ogin
- LIGO-California Institute of Technology, Pasadena, California 91125, 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
| | - P Oppermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B O'Reilly
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Ortega Larcher
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - R O'Shaughnessy
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - C Osthelder
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - C D Ott
- Caltech-CaRT, Pasadena, California 91125, USA
| | - D J Ottaway
- University of Adelaide, Adelaide, SA 5005, Australia
| | - R S Ottens
- University of Florida, Gainesville, Florida 32611, USA
| | - J Ou
- National Tsing Hua University, Hsinchu Taiwan 300
| | - 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
| | - C Palomba
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - 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
| | - R Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Siena, I-53100 Siena, 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
- LIGO-Hanford Observatory, Richland, Washington 99352, 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
| | - P Peiris
- Rochester Institute of Technology, Rochester, New York 14623, 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
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
| | - V Pierro
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN (Sezione di Napoli), Italy
| | - L Pinard
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - B Pindor
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - I M Pinto
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN (Sezione di 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
| | - V Poole
- Washington State University, Pullman, Washington 99164, USA
| | - C Poux
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - 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
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Principe
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN (Sezione di Napoli), Italy
| | - S Privitera
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - R Prix
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - G A Prodi
- INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy and Università di Trento, I-38050 Povo, Trento, Italy
| | - L Prokhorov
- Moscow State University, Moscow 119992, 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
| | - 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
- Columbia University, New York, New York 10027, USA and MTA-Eotvos University, "Lendulet" A. R. G., Budapest 1117, Hungary
| | - S Raja
- RRCAT, Indore, MP 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
| | - 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
| | - V Re
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - C M Reed
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - T Reed
- Louisiana Tech University, Ruston, Louisiana 71272, 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
| | - 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 Roddy
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | - C Rodriguez
- Northwestern University, Evanston, Illinois 60208, USA
| | - M Rodruck
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - C Roever
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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
- INFN, Sezione di Napoli, Complesso Universitario di Monte S.Angelo, I-80126 Napoli, Italy and Università di Salerno, Fisciano, I-84084 Salerno, 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 Sanders
- University of Michigan, Ann Arbor, Michigan 48109, 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
| | - R Schilling
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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 Schulz
- 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
| | - P Schwinberg
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - J Scott
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S M Scott
- Australian National University, Canberra, ACT 0200, Australia
| | - F Seifert
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - 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
| | - A Sergeev
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - D 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
| | - 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
| | - A M Sintes
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - G R Skelton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - B J J Slagmolen
- Australian National University, Canberra, ACT 0200, Australia
| | - J Slutsky
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - N D Smith-Lefebvre
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - K Soden
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, 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
| | - L Sperandio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Staley
- Columbia University, New York, New York 10027, USA
| | - E Steinert
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - J Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Steplewski
- Washington State University, Pullman, Washington 99164, USA
| | - D Stevens
- Northwestern University, Evanston, Illinois 60208, USA
| | - A Stochino
- Australian National University, Canberra, ACT 0200, Australia
| | - R Stone
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - 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
- Moscow State University, Moscow 119992, Russia
| | - A S Stroeer
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - R Sturani
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
| | - A L Stuver
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - S Susmithan
- University of Western Australia, Crawley, WA 6009, Australia
| | - P J Sutton
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B Swinkels
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - G Szeifert
- MTA-Eotvos University, "Lendulet" A. R. G., Budapest 1117, Hungary
| | - 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
| | - L Tang
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - D B Tanner
- University of Florida, Gainesville, Florida 32611, 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
| | | | | | - 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
| | - A Toncelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - O Torre
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Siena, I-53100 Siena, 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 Ugolini
- Trinity University, San Antonio, Texas 78212, 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
| | | | - 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, SA 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
| | - S Verma
- University of Western Australia, Crawley, WA 6009, Australia
| | - F Vetrano
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
| | - A Viceré
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy and Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, 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
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - B Vlcek
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, 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
| | - D Vrinceanu
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - A 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
| | - S J Waldman
- LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Walker
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - L Wallace
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - Y Wan
- Tsinghua University, Beijing 100084, China
| | - J Wang
- National Tsing Hua University, Hsinchu Taiwan 300
| | - M Wang
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - X Wang
- Tsinghua University, Beijing 100084, China
| | - A Wanner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - 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, WA 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
| | - S E Whitcomb
- LIGO-California Institute of Technology, Pasadena, California 91125, USA and University of Western Australia, Crawley, WA 6009, Australia
| | - D J White
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - B F Whiting
- University of Florida, Gainesville, Florida 32611, USA
| | - S Wibowo
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - K Wiesner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Wilkinson
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - L Williams
- University of Florida, Gainesville, Florida 32611, USA
| | - R Williams
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - T 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
| | - L Winkelmann
- 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
| | - 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
| | - J Worden
- LIGO-Hanford Observatory, Richland, Washington 99352, USA
| | - J Yablon
- Northwestern University, Evanston, Illinois 60208, USA
| | - I Yakushin
- LIGO-Livingston Observatory, Livingston, Louisiana 70754, 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
| | - D Yeaton-Massey
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - S Yoshida
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | - H Yum
- Northwestern University, Evanston, Illinois 60208, 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
| | - F Zhang
- LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - L Zhang
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | - C Zhao
- University of Western Australia, Crawley, WA 6009, Australia
| | - H Zhu
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - X J Zhu
- University of Western Australia, Crawley, WA 6009, Australia
| | - N Zotov
- Louisiana Tech University, Ruston, Louisiana 71272, USA
| | - M E Zucker
- LIGO-Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J Zweizig
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| |
Collapse
|
17
|
Abadie J, Abbott BP, Abbott R, Abernathy M, Accadia T, Acernese F, Adams C, Adhikari R, Ajith P, Allen B, Allen G, Amador Ceron E, Amin RS, Anderson SB, Anderson WG, Antonucci F, Arain MA, Araya M, Aronsson M, Arun KG, Aso Y, Aston S, Astone P, Atkinson DE, Aufmuth P, Aulbert C, Babak S, Baker P, Ballardin G, Ballinger T, Ballmer S, Barker D, Barnum S, Barone F, Barr B, Barriga P, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Bastarrika M, Bauchrowitz J, Bauer TS, Behnke B, Beker MG, Belletoile A, Benacquista M, Bertolini A, Betzwieser J, Beveridge N, Beyersdorf PT, Bigotta S, Bilenko IA, Billingsley G, Birch J, Birindelli S, Biswas R, Bitossi M, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Blom M, Boccara C, Bock O, Bodiya TP, Bondarescu R, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Bose S, Bosi L, Bouhou B, Boyle M, Braccini S, Bradaschia C, Brady PR, Braginsky VB, Brau JE, Breyer J, Bridges DO, Brillet A, Brinkmann M, Brisson V, Britzger M, Brooks AF, Brown DA, Budzyński R, Bulik T, Bulten HJ, Buonanno A, Burguet-Castell J, Burmeister O, Buskulic D, Buy C, Byer RL, Cadonati L, Cagnoli G, Cain J, Calloni E, Camp JB, Campagna E, Campsie P, Cannizzo J, Cannon KC, Canuel B, Cao J, Capano C, Carbognani F, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Cella G, Cepeda C, Cesarini E, Chalermsongsak T, Chalkley E, Charlton P, Chassande-Mottin E, Chelkowski S, Chen Y, Chincarini A, Christensen N, Chua SSY, Chung CTY, Clark D, Clark J, Clayton JH, Cleva F, Coccia E, Colacino CN, Colas J, Colla A, Colombini M, Conte R, Cook D, Corbitt TR, Cornish N, Corsi A, Costa CA, Coulon JP, Coward D, Coyne DC, Creighton JDE, Creighton TD, Cruise AM, Culter RM, Cumming A, Cunningham L, Cuoco E, Dahl K, Danilishin SL, Dannenberg R, D’Antonio S, Danzmann K, Das K, Dattilo V, Daudert B, Davier M, Davies G, Davis A, Daw EJ, Day R, Dayanga T, De Rosa R, DeBra D, Degallaix J, del Prete M, Dergachev V, DeRosa R, DeSalvo R, Devanka P, Dhurandhar S, Di Fiore L, Di Lieto A, Di Palma I, Di Paolo Emilio M, Di Virgilio A, Díaz M, Dietz A, Donovan F, Dooley KL, Doomes EE, Dorsher S, Douglas ESD, Drago M, Drever RWP, Driggers JC, Dueck J, Dumas JC, Dwyer S, Eberle T, Edgar M, Edwards M, Effler A, Ehrens P, Ely G, Engel R, Etzel T, Evans M, Evans T, Fafone V, Fairhurst S, Fan Y, Farr BF, Fazi D, Fehrmann H, Feldbaum D, Ferrante I, Fidecaro F, Finn LS, Fiori I, Flaminio R, Flanigan M, Flasch K, Foley S, Forrest C, Forsi E, Fotopoulos N, Fournier JD, Franc J, Frasca S, Frasconi F, Frede M, Frei M, Frei Z, Freise A, Frey R, Fricke TT, Friedrich D, Fritschel P, Frolov VV, Fulda P, Fyffe M, Galimberti M, Gammaitoni L, Garofoli JA, Garufi F, Gemme G, Genin E, Gennai A, Ghosh S, Giaime JA, Giampanis S, Giardina KD, Giazotto A, Gill C, Goetz E, Goggin LM, González G, Goßler S, Gouaty R, Graef C, Granata M, Grant A, Gras S, Gray C, Greenhalgh RJS, Gretarsson AM, Greverie C, Grosso R, Grote H, Grunewald S, Guidi GM, Gustafson EK, Gustafson R, Hage B, Hall P, Hallam JM, Hammer D, Hammond G, Hanks J, Hanna C, Hanson J, Harms J, Harry GM, Harry IW, Harstad ED, Haughian K, Hayama K, Hayau JF, Hayler T, Heefner J, Heitmann H, Hello P, Heng IS, Heptonstall A, Hewitson M, Hild S, Hirose E, Hoak D, Hodge KA, Holt K, Hosken DJ, Hough J, Howell E, Hoyland D, Huet D, Hughey B, Husa S, Huttner SH, Huynh-Dinh T, Ingram DR, Inta R, Isogai T, Ivanov A, Jaranowski P, Johnson WW, Jones DI, Jones G, Jones R, Ju L, Kalmus P, Kalogera V, Kandhasamy S, Kanner J, Katsavounidis E, Kawabe K, Kawamura S, Kawazoe F, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khazanov EA, Kim H, King PJ, Kinzel DL, Kissel JS, Klimenko S, Kondrashov V, Kopparapu R, Koranda S, Kowalska I, Kozak D, Krause T, Kringel V, Krishnamurthy S, Krishnan B, Królak A, Kuehn G, Kullman J, Kumar R, Kwee P, Landry M, Lang M, Lantz B, Lastzka N, Lazzarini A, Leaci P, Leong J, Leonor I, Leroy N, Letendre N, Li J, Li TGF, Lin H, Lindquist PE, Lockerbie NA, Lodhia D, Lorenzini M, Loriette V, Lormand M, Losurdo G, Lu P, Luan J, Lubinski M, Lucianetti A, Lück H, Lundgren A, Machenschalk B, MacInnis M, Mageswaran M, Mailand K, Majorana E, Mak C, Maksimovic I, Man N, Mandel I, Mandic V, Mantovani M, Marchesoni F, Marion F, Márka S, Márka Z, Maros E, Marque J, Martelli F, Martin IW, Martin RM, Marx JN, Mason K, Masserot A, Matichard F, Matone L, Matzner RA, Mavalvala N, McCarthy R, McClelland DE, McGuire SC, McIntyre G, McIvor G, McKechan DJA, Meadors G, Mehmet M, Meier T, Melatos A, Melissinos AC, Mendell G, Menéndez DF, Mercer RA, Merill L, Meshkov S, Messenger C, Meyer MS, Miao H, Michel C, Milano L, Miller J, Minenkov Y, Mino Y, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Moe B, Mohan M, Mohanty SD, Mohapatra SRP, Moraru D, Moreau J, Moreno G, Morgado N, Morgia A, Mors K, Mosca S, Moscatelli V, Mossavi K, Mours B, MowLowry C, Mueller G, Mukherjee S, Mullavey A, Müller-Ebhardt H, Munch J, Murray PG, Nash T, Nawrodt R, Nelson J, Neri I, Newton G, Nishida E, Nishizawa A, Nocera F, Nolting D, Ochsner E, O’Dell J, Ogin GH, Oldenburg RG, O’Reilly B, O’Shaughnessy R, Osthelder C, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Page A, Pagliaroli G, Palladino L, Palomba C, Pan Y, Pankow C, Paoletti F, Papa MA, Pardi S, Pareja M, Parisi M, Pasqualetti A, Passaquieti R, Passuello D, Patel P, Pathak D, Pedraza M, Pekowsky L, Penn S, Peralta C, Perreca A, Persichetti G, Pichot M, Pickenpack M, Piergiovanni F, Pietka M, Pinard L, Pinto IM, Pitkin M, Pletsch HJ, Plissi MV, Poggiani R, Postiglione F, Prato M, Predoi V, Price LR, Prijatelj M, Principe M, Prix R, Prodi GA, Prokhorov L, Puncken O, Punturo M, Puppo P, Quetschke V, Raab FJ, Rabeling DS, Radke T, Radkins H, Raffai P, Rakhmanov M, Rankins B, Rapagnani P, Raymond V, Re V, Reed CM, Reed T, Regimbau T, Reid S, Reitze DH, Ricci F, Riesen R, Riles K, Roberts P, Robertson NA, Robinet F, Robinson C, Robinson EL, Rocchi A, Roddy S, Röver C, Rolland L, Rollins J, Romano JD, Romano R, Romie JH, Rosińska D, Rowan S, Rüdiger A, Ruggi P, Ryan K, Sakata S, Sakosky M, Salemi F, Sammut L, Sancho de la Jordana L, Sandberg V, Sannibale V, Santamaría L, Santostasi G, Saraf S, Sassolas B, Sathyaprakash BS, Sato S, Satterthwaite M, Saulson PR, Savage R, Schilling R, Schnabel R, Schofield R, Schulz B, Schutz BF, Schwinberg P, Scott J, Scott SM, Searle AC, Seifert F, Sellers D, Sengupta AS, Sentenac D, Sergeev A, Shaddock D, Shapiro B, Shawhan P, Shoemaker DH, Sibley A, Siemens X, Sigg D, Singer A, Sintes AM, Skelton G, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith ND, Somiya K, Sorazu B, Speirits FC, Sperandio L, Stein AJ, Stein LC, Steinlechner S, Steplewski S, Stochino A, Stone R, Strain KA, Strigin S, Stroeer A, Sturani R, Stuver AL, Summerscales TZ, Sung M, Susmithan S, Sutton PJ, Swinkels B, Talukder D, Tanner DB, Tarabrin SP, Taylor JR, Taylor R, Thomas P, Thorne KA, Thorne KS, Thrane E, Thüring A, Titsler C, Tokmakov KV, Toncelli A, Tonelli M, Torre O, Torres C, Torrie CI, Tournefier E, Travasso F, Traylor G, Trias M, Trummer J, Tseng K, Turner L, Ugolini D, Urbanek K, Vahlbruch H, Vaishnav B, Vajente G, Vallisneri M, van den Brand JFJ, Van Den Broeck C, van der Putten S, van der Sluys MV, van Veggel AA, Vass S, Vaulin R, Vavoulidis M, Vecchio A, Vedovato G, Veitch J, Veitch PJ, Veltkamp C, Verkindt D, Vetrano F, Viceré A, Villar A, Vinet JY, Vocca H, Vorvick C, Vyachanin SP, Waldman SJ, Wallace L, Wanner A, Ward RL, Was M, Wei P, Weinert M, Weinstein AJ, Weiss R, Wen L, Wen S, Wessels P, West M, Westphal T, Wette K, Whelan JT, Whitcomb SE, White DJ, Whiting BF, Wilkinson C, Willems PA, Williams L, Willke B, Winkelmann L, Winkler W, Wipf CC, Wiseman AG, Woan G, Wooley R, Worden J, Yakushin I, Yamamoto H, Yamamoto K, Yeaton-Massey D, Yoshida S, Yu PP, Yvert M, Zanolin M, Zhang L, Zhang Z, Zhao C, Zotov N, Zucker ME, Zweizig J. Publisher’s Note: Search for gravitational waves from compact binary coalescence in LIGO and Virgo data from S5 and VSR1 [Phys. Rev. D82, 102001 (2010)]. Int J Clin Exp Med 2012. [DOI: 10.1103/physrevd.85.089903] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
|
18
|
Abadie J, Abbott BP, Abbott R, Abernathy M, Accadia T, Acernese F, Adams C, Adhikari R, Ajith P, Allen B, Allen GS, Ceron EA, Amin RS, Anderson SB, Anderson WG, Antonucci F, Arain MA, Araya MC, Aronsson M, Arun KG, Aso Y, Aston SM, Astone P, Atkinson D, Aufmuth P, Aulbert C, Babak S, Baker P, Ballardin G, Ballmer S, Barker D, Barnum S, Barone F, Barr B, Barriga P, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Bastarrika M, Bauchrowitz J, Bauer TS, Behnke B, Beker MG, Belletoile A, Benacquista M, Bertolini A, Betzwieser J, Beveridge N, Beyersdorf PT, Bigotta S, Bilenko IA, Billingsley G, Birch J, Birindelli S, Biswas R, Bitossi M, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bland B, Blom M, Boccara C, Bock O, Bodiya TP, Bondarescu R, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Bose S, Bosi L, Bouhou B, Boyle M, Braccini S, Bradaschia C, Brady PR, Braginsky VB, Brau JE, Breyer J, Bridges DO, Brillet A, Brinkmann M, Brisson V, Britzger M, Brooks AF, Brown DA, Budzyński R, Bulik T, Bulten HJ, Buonanno A, Burguet-Castell J, Burmeister O, Buskulic D, Buy C, Byer RL, Cadonati L, Cagnoli G, Cain J, Calloni E, Camp JB, Campagna E, Campsie P, Cannizzo J, Cannon K, Canuel B, Cao J, Capano C, Carbognani F, Caride S, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Cella G, Cepeda C, Cesarini E, Chalermsongsak T, Chalkley E, Charlton P, Chassande-Mottin E, Chelkowski S, Chen Y, Chincarini A, Christensen N, Chua SSY, Chung CTY, Clark D, Clark J, Clayton JH, Cleva F, Coccia E, Colacino CN, Colas J, Colla A, Colombini M, Conte R, Cook D, Corbitt TR, Cornish N, Corsi A, Costa CA, Coulon JP, Coward DM, Coyne DC, Creighton JDE, Creighton TD, Cruise AM, Culter RM, Cumming A, Cunningham L, Cuoco E, Dahl K, Danilishin SL, Dannenberg R, D'Antonio S, Danzmann K, Das K, Dattilo V, Daudert B, Davier M, Davies G, Davis A, Daw EJ, Day R, Dayanga T, De Rosa R, DeBra D, Degallaix J, del Prete M, Dergachev V, DeRosa R, DeSalvo R, Devanka P, Dhurandhar S, Di Fiore L, Di Lieto A, Di Palma I, Di Paolo Emilio M, Di Virgilio A, Díaz M, Dietz A, Donovan F, Dooley KL, Doomes EE, Dorsher S, Douglas ESD, Drago M, Drever RWP, Driggers JC, Dueck J, Dumas JC, Eberle T, Edgar M, Edwards M, Effler A, Ehrens P, Engel R, Etzel T, Evans M, Evans T, Fafone V, Fairhurst S, Fan Y, Farr BF, Fazi D, Fehrmann H, Feldbaum D, Ferrante I, Fidecaro F, Finn LS, Fiori I, Flaminio R, Flanigan M, Flasch K, Foley S, Forrest C, Forsi E, Fotopoulos N, Fournier JD, Franc J, Frasca S, Frasconi F, Frede M, Frei M, Frei Z, Freise A, Frey R, Fricke TT, Friedrich D, Fritschel P, Frolov VV, Fulda P, Fyffe M, Galimberti M, Gammaitoni L, Garofoli JA, Garufi F, Gemme G, Genin E, Gennai A, Gholami I, Ghosh S, Giaime JA, Giampanis S, Giardina KD, Giazotto A, Gill C, Goetz E, Goggin LM, González G, Gorodetsky ML, Gossler S, Gouaty R, Graef C, Granata M, Grant A, Gras S, Gray C, Greenhalgh RJS, Gretarsson AM, Greverie C, Grosso R, Grote H, Grunewald S, Guidi GM, Gustafson EK, Gustafson R, Hage B, Hall P, Hallam JM, Hammer D, Hammond G, Hanks J, Hanna C, Hanson J, Harms J, Harry GM, Harry IW, Harstad ED, Haughian K, Hayama K, Hayau JF, Hayler T, Heefner J, Heitmann H, Hello P, Heng IS, Heptonstall AW, Hewitson M, Hild S, Hirose E, Hoak D, Hodge KA, Holt K, Hosken DJ, Hough J, Howell EJ, Hoyland D, Huet D, Hughey B, Husa S, Huttner SH, Huynh-Dinh T, Ingram DR, Inta R, Isogai T, Ivanov A, Jaranowski P, Johnson WW, Jones DI, Jones G, Jones R, Ju L, Kalmus P, Kalogera V, Kandhasamy S, Kanner JB, Katsavounidis E, Kawabe K, Kawamura S, Kawazoe F, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khazanov EA, Kim H, King PJ, Kinzel DL, Kissel JS, Klimenko S, Kondrashov V, Kopparapu R, Koranda S, Kowalska I, Kozak D, Krause T, Kringel V, Krishnamurthy S, Krishnan B, Królak A, Kuehn G, Kullman J, Kumar R, Kwee P, Landry M, Lang M, Lantz B, Lastzka N, Lazzarini A, Leaci P, Leong J, Leonor I, Leroy N, Letendre N, Li J, Li TGF, Liguori N, Lin H, Lindquist PE, Lockerbie NA, Lodhia D, Lorenzini M, Loriette V, Lormand M, Losurdo G, Lu P, Luan J, Lubinski M, Lucianetti A, Lück H, Lundgren AD, Machenschalk B, MacInnis M, Mageswaran M, Mailand K, Majorana E, Mak C, Maksimovic I, Man N, Mandel I, Mandic V, Mantovani M, Marchesoni F, Marion F, Márka S, Márka Z, Maros E, Marque J, Martelli F, Martin IW, Martin RM, Marx JN, Mason K, Masserot A, Matichard F, Matone L, Matzner RA, Mavalvala N, McCarthy R, McClelland DE, McGuire SC, McIntyre G, McIvor G, McKechan DJA, Meadors G, Mehmet M, Meier T, Melatos A, Melissinos AC, Mendell G, Menéndez DF, Mercer RA, Merill L, Meshkov S, Messenger C, Meyer MS, Miao H, Michel C, Milano L, Miller J, Minenkov Y, Mino Y, Mitra S, Mitrofanov VP, Mitselmakher G, Mittleman R, Moe B, Mohan M, Mohanty SD, Mohapatra SRP, Moraru D, Moreau J, Moreno G, Morgado N, Morgia A, Morioka T, Mors K, Mosca S, Moscatelli V, Mossavi K, Mours B, Mow-Lowry CM, Mueller G, Mukherjee S, Mullavey A, Müller-Ebhardt H, Munch J, Murray PG, Nash T, Nawrodt R, Nelson J, Neri I, Newton G, Nishizawa A, Nocera F, Nolting D, Ochsner E, O'Dell J, Ogin GH, Oldenburg RG, O'Reilly B, O'Shaughnessy R, Osthelder C, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Page A, Pagliaroli G, Palladino L, Palomba C, Pan Y, Pankow C, Paoletti F, Papa MA, Pardi S, Pareja M, Parisi M, Pasqualetti A, Passaquieti R, Passuello D, Patel P, Pathak D, Pedraza M, Pekowsky L, Penn S, Peralta C, Perreca A, Persichetti G, Pichot M, Pickenpack M, Piergiovanni F, Pietka M, Pinard L, Pinto IM, Pitkin M, Pletsch HJ, Plissi MV, Poggiani R, Postiglione F, Prato M, Predoi V, Price LR, Prijatelj M, Principe M, Prix R, Prodi GA, Prokhorov L, Puncken O, Punturo M, Puppo P, Quetschke V, Raab FJ, Rabeling DS, Radke T, Radkins H, Raffai P, Rakhmanov M, Rankins B, Rapagnani P, Raymond V, Re V, Reed CM, Reed T, Regimbau T, Reid S, Reitze DH, Ricci F, Riesen R, Riles K, Roberts P, Robertson NA, Robinet F, Robinson C, Robinson EL, Rocchi A, Roddy S, Röver C, Rolland L, Rollins J, Romano JD, Romano R, Romie JH, Rosińska D, Rowan S, Rüdiger A, Ruggi P, Ryan K, Sakata S, Sakosky M, Salemi F, Sammut L, de la Jordana LS, Sandberg V, Sannibale V, Santamaría L, Santostasi G, Saraf S, Sassolas B, Sathyaprakash BS, Sato S, Satterthwaite M, Saulson PR, Savage R, Schilling R, Schnabel R, Schofield RMS, Schulz B, Schutz BF, Schwinberg P, Scott J, Scott SM, Searle AC, Seifert F, Sellers D, Sengupta AS, Sentenac D, Sergeev A, Shaddock DA, Shapiro B, Shawhan P, Shoemaker DH, Sibley A, Siemens X, Sigg D, Singer A, Sintes AM, Skelton G, Slagmolen BJJ, Slutsky J, Smith JR, Smith MR, Smith ND, Somiya K, Sorazu B, Speirits FC, Sperandio L, Stein AJ, Stein LC, Steinlechner S, Steplewski S, Stochino A, Stone R, Strain KA, Strigin S, Stroeer AS, Sturani R, Stuver AL, Summerscales TZ, Sung M, Susmithan S, Sutton PJ, Swinkels B, Szokoly GP, Talukder D, Tanner DB, Tarabrin SP, Taylor JR, Taylor R, Thomas P, Thorne KA, Thorne KS, Thrane E, Thüring A, Titsler C, Tokmakov KV, Toncelli A, Tonelli M, Torre O, Torres C, Torrie CI, Tournefier E, Travasso F, Traylor G, Trias M, Trummer J, Tseng K, Turner L, Ugolini D, Urbanek K, Vahlbruch H, Vaishnav B, Vajente G, Vallisneri M, van den Brand JFJ, Van Den Broeck C, van der Putten S, van der Sluys MV, van Veggel AA, Vass S, Vaulin R, Vavoulidis M, Vecchio A, Vedovato G, Veitch J, Veitch PJ, Veltkamp C, Verkindt D, Vetrano F, Viceré A, Villar AE, Vinet JY, Vocca H, Vorvick C, Vyachanin SP, Waldman SJ, Wallace L, Wanner A, Ward RL, Was M, Wei P, Weinert M, Weinstein AJ, Weiss R, Wen L, Wen S, Wessels P, West M, Westphal T, Wette K, Whelan JT, Whitcomb SE, White D, Whiting BF, Wilkinson C, Willems PA, Williams L, Willke B, Winkelmann L, Winkler W, Wipf CC, Wiseman AG, Woan G, Wooley R, Worden J, Yakushin I, Yamamoto H, Yamamoto K, Yeaton-Massey D, Yoshida S, Yu P, Yvert M, Zanolin M, Zhang L, Zhang Z, Zhao C, Zotov N, Zucker ME, Zweizig J. Directional limits on persistent gravitational waves using LIGO S5 science data. Phys Rev Lett 2011; 107:271102. [PMID: 22243300 DOI: 10.1103/physrevlett.107.271102] [Citation(s) in RCA: 19] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/09/2011] [Indexed: 05/31/2023]
Abstract
The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgrounds. We perform two directional searches for persistent GWs using data from the LIGO S5 science run: one optimized for pointlike sources and one for arbitrary extended sources. Finding no evidence to support the detection of GWs, we present 90% confidence level (C.L.) upper-limit maps of GW strain power with typical values between 2-20×10(-50) strain(2) Hz(-1) and 5-35×10(-49) strain(2) Hz(-1) sr(-1) for pointlike and extended sources, respectively. The latter result is the first of its kind. We also set 90% C.L. limits on the narrow-band root-mean-square GW strain from interesting targets including Sco X-1, SN 1987A and the Galactic center as low as ≈7×10(-25) in the most sensitive frequency range near 160 Hz.
Collapse
Affiliation(s)
- J Abadie
- LIGO-California Institute of Technology, Pasadena, California 91125, USA
| | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | |
Collapse
|
19
|
Accadia T, Acernese F, Astone P, Ballardin G, Barone F, Barsuglia M, Basti A, Bauer TS, Bebronne M, Beker MG, Belletoile A, Bitossi M, Bizouard MA, Blom M, Bondu F, Bonelli L, Bonnand R, Boschi V, Bosi L, Bouhou B, Braccini S, Bradaschia C, Branchesi M, Briant T, Brillet A, Brisson V, Bulik T, Bulten HJ, Buskulic D, Buy C, Cagnoli G, Calloni E, Canuel B, Carbognani F, Cavalier F, Cavalieri R, Cella G, Cesarini E, Chaibi O, Chassande-Mottin E, Chincarini A, Chiummo A, Cleva F, Coccia E, Cohadon PF, Colacino CN, Colas J, Colla A, Colombini M, Conte A, Corsi A, Coulon JP, Cuoco E, D' Antonio S, Dattilo V, Davier M, Day R, De Rosa R, Debreczeni G, Del Pozzo W, del Prete M, Di Fiore L, Di Lieto A, Di Paolo Emilio M, Di Virgilio A, Dietz A, Drago M, Endroczi G, Fafone V, Ferrante I, Fidecaro F, Fiori I, Flaminio R, Forte LA, Fournier JD, Franc J, Frasca S, Frasconi F, Galimberti M, Gammaitoni L, Garufi F, Gáspár ME, Gemme G, Genin E, Gennai A, Giazotto A, Gouaty R, Granata M, Greverie C, Guidi GM, Hayau JF, Heidmann A, Heitmann H, Hello P, Jaranowski P, Kowalska I, Królak A, Leroy N, Letendre N, Li TGF, Liguori N, Lorenzini M, Loriette V, Losurdo G, Majorana E, Maksimovic I, Man N, Mantovani M, Marchesoni F, Marion F, Marque J, Martelli F, Masserot A, Michel C, Milano L, Minenkov Y, Mohan M, Morgado N, Morgia A, Mours B, Naticchioni L, Nocera F, Pagliaroli G, Palladino L, Palomba C, Paoletti F, Parisi M, Pasqualetti A, Passaquieti R, Passuello D, Persichetti G, Piergiovanni F, Pietka M, Pinard L, Poggiani R, Prato M, Prodi GA, Punturo M, Puppo P, Rabeling DS, Rácz I, Rapagnani P, Re V, Regimbau T, Ricci F, Robinet F, Rocchi A, Rolland L, Romano R, Rosińska D, Ruggi P, Sassolas B, Sentenac D, Sperandio L, Sturani R, Swinkels B, Tacca M, Taffarello L, Toncelli A, Tonelli M, Torre O, Tournefier E, Travasso F, Vajente G, van den Brand JFJ, Van den Broeck C, van der Putten S, Vasuth M, Vavoulidis M, Vedovato G, Verkindt D, Vetrano F, Viceré A, Vinet JY, Vitale S, Vocca H, Ward RL, Was M, Yvert M, Zadroźny A, Zendri JP. A state observer for the Virgo inverted pendulum. Rev Sci Instrum 2011; 82:094502. [PMID: 21974605 DOI: 10.1063/1.3637466] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/31/2023]
Abstract
We report an application of Kalman filtering to the inverted pendulum (IP) of the Virgo gravitational wave interferometer. Using subspace method system identification techniques, we calculated a linear mechanical model of Virgo IP from experimental transfer functions. We then developed a Kalman filter, based on the obtained state space representation, that estimates from open loop time domain data, the state variables of the system. This allows the observation (and eventually control) of every resonance mode of the IP mechanical structure independently.
Collapse
Affiliation(s)
- T Accadia
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-Le-Vieux, France
| | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | |
Collapse
|
20
|
Pellé F, Dhaouadi M, Michely L, Aschehoug P, Toncelli A, Veronesi S, Tonelli M. Spectroscopic properties and upconversion in Pr3+:YF3 nanoparticles. Phys Chem Chem Phys 2011; 13:17453-60. [DOI: 10.1039/c1cp20725c] [Citation(s) in RCA: 39] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/21/2022]
|
21
|
Accadia T, Acernese F, Antonucci F, Aoudia S, Arun KG, Astone P, Ballardin G, Barone F, Barsuglia M, Bauer TS, Beker MG, Bigotta S, Birindelli S, Bitossi M, Bizouard MA, Blom M, Boccara C, Bondu F, Bonelli L, Bosi L, Braccini S, Bradaschia C, Brillet A, Budzynski R, Bulik T, Bulten HJ, Buskulic D, Cagnoli G, Calloni E, Campagna E, Canuel B, Carbognani F, Cavalier F, Cavalieri R, Cella G, Cesarini E, Chassande-Mottin E, Chincarini A, Cleva F, Coccia E, Colacino CN, Colas J, Colla A, Colombini M, Corda C, Corsi A, Coulon JP, Cuoco E, D'Antonio S, Dari A, Dattilo V, Davier M, Day R, De Rosa R, del Prete M, Di Fiore L, Di Lieto A, Emilio MDP, Di Virgilio A, Dietz A, Drago M, Fafone V, Ferrante I, Fidecaro F, Fiori I, Flaminio R, Fournier JD, Franc J, Frasca S, Frasconi F, Freise A, Gammaitoni L, Garufi F, Gemme G, Genin E, Gennai A, Giazotto A, Gouaty R, Granata M, Greverie C, Guidi GM, Heitmann H, Hello P, Hild S, Huet D, Jaranowski P, Kowalska I, Królak A, La Penna P, Leroy N, Letendre N, Li TGF, Lorenzini M, Loriette V, Losurdo G, Mackowski JM, Majorana E, Man N, Mantovani M, Marchesoni F, Marion F, Marque J, Martelli F, Masserot A, Michel C, Milano L, Minenkov Y, Mohan M, Moreau J, Morgado N, Morgia A, Mosca S, Moscatelli V, Mours B, Neri I, Nocera F, Pagliaroli G, Palladino L, Palomba C, Paoletti F, Pardi S, Parisi M, Pasqualetti A, Passaquieti R, Passuello D, Persichetti G, Pichot M, Piergiovanni F, Pietka M, Pinard L, Poggiani R, Prato M, Prodi GA, Punturo M, Puppo P, Rabaste O, Rabeling DS, Rapagnani P, Re V, Regimbau T, Ricci F, Robinet F, Rocchi A, Rolland L, Romano R, Rosińska D, Ruggi P, Sassolas B, Sentenac D, Sturani R, Swinkels B, Toncelli A, Tonelli M, Tournefier E, Travasso F, Trummer J, Vajentei G, van den Brand JFJ, van der Putten S, Vavoulidis M, Vedovato G, Verkindt D, Vetrano F, Viceré A, Vinet JY, Vocca H, Was M, Yvert M. In-vacuum Faraday isolation remote tuning. Appl Opt 2010; 49:4780-4790. [PMID: 20842804 DOI: 10.1364/ao.49.004780] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/29/2023]
Abstract
In-vacuum Faraday isolators (FIs) are used in gravitational wave interferometers to prevent the disturbance caused by light reflected back to the input port from the interferometer itself. The efficiency of the optical isolation is becoming more critical with the increase of laser input power. An in-vacuum FI, used in a gravitational wave experiment (Virgo), has a 20 mm clear aperture and is illuminated by an almost 20 W incoming beam, having a diameter of about 5 mm. When going in vacuum at 10(-6) mbar, a degradation of the isolation exceeding 10 dB was observed. A remotely controlled system using a motorized lambda=2 waveplate inserted between the first polarizer and the Faraday rotator has proven its capability to restore the optical isolation to a value close to the one set up in air.
Collapse
|
22
|
Accadia T, Acernese F, Antonucci F, Aoudia S, Arun KG, Astone P, Ballardin G, Barone F, Barsuglia M, Bauer TS, Beker MG, Belletoile A, Bigotta S, Birindelli S, Bitossi M, Bizouard MA, Blom M, Boccara C, Bondu F, Bonelli L, Bonnand R, Bosi L, Braccini S, Bradaschia C, Brillet A, Brisson V, Budzyński R, Bulik T, Bulten HJ, Buskulic D, Buy C, Cagnoli G, Calloni E, Campagna E, Canuel B, Carbognani F, Cavalier F, Cavalieri R, Cella G, Cesarini E, Chassande-Mottin E, Chincarini A, Cleva F, Coccia E, Colacino CN, Colas J, Colla A, Colombini M, Corsi A, Coulon JP, Cuoco E, D'Antonio S, Dari A, Dattilo V, Davier M, Day R, Rosa RD, Prete MD, Fiore LD, Lieto AD, Emilio MDP, Virgilio AD, Dietz A, Drago M, Fafone V, Ferrante I, Fidecaro F, Fiori I, Flaminio R, Fournier JD, Franc J, Frasca S, Frasconi F, Freise A, Galimberti M, Gammaitoni L, Garufi F, Gemme G, Genin E, Gennai A, Giazotto A, Gouaty R, Granata M, Greverie C, Guidi GM, Heitmann H, Hello P, Hild S, Huet D, Jaranowski P, Kowalska I, Królak A, Leroy N, Letendre N, Li TGF, Lorenzini M, Loriette V, Losurdo G, Mackowski JM, Majorana E, Maksimovic I, Man N, Mantovani M, Marchesoni F, Marion F, Marque J, Martelli F, Masserot A, Michel C, Milano L, Minenkov Y, Mohan M, Moreau J, Morgado N, Morgia A, Mosca S, Moscatelli V, Mours B, Neri I, Nocera F, Pagliaroli G, Palladino L, Palomba C, Paoletti F, Pardi S, Parisi M, Pasqualetti A, Passaquieti R, Passuello D, Persichetti G, Pichot M, Piergiovanni F, Pietka M, Pinard L, Poggiani R, Prato M, Prodi GA, Punturo M, Puppo P, Rabaste O, Rabeling DS, Rapagnani P, Re V, Regimbau T, Ricci F, Robinet F, Rocchi A, Rolland L, Romano R, Rosińska D, Ruggi P, Sassolas B, Sentenac D, Sturani R, Swinkels B, Toncelli A, Tonelli M, Torre O, Tournefier E, Travasso F, Trummer J, Vajente G, Brand JFJVD, Putten SVD, Vavoulidis M, Vedovato G, Verkindt D, Vetrano F, Viceré A, Vinet JY, Vocca H, Was M, Yvert M. Virgo calibration and reconstruction of the gravitationnal wave strain during VSR1. ACTA ACUST UNITED AC 2010. [DOI: 10.1088/1742-6596/228/1/012015] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
|
23
|
Accadia T, Acernese F, Antonucci F, Aoudia S, Arun KG, Astone P, Ballardin G, Barone F, Barsuglia M, Bauer TS, Beker MG, Belletoile A, Bigotta S, Birindelli S, Bizouard MA, Blom M, Boccara C, Bondu F, Bonelli L, Bonnand R, Bosi L, Braccini S, Bradaschia C, Brillet A, Brisson V, Budzyński R, Bulik T, Bulten HJ, Buskulic D, Buy C, Cagnoli G, Calloni E, Campagna E, Canuel B, Carbognani F, Cavalier F, Cavalieri R, Cella G, Cesarini E, Chassande-Mottin E, Chincarini A, Cleva F, Coccia E, Colacino CN, Colas J, Colla A, Colombini M, Corsi A, Coulon JP, Cuoco E, D'Antonio S, Dari A, Dattilo V, Davier M, Day R, Rosa RD, Prete MD, Fiore LD, Lieto AD, Emilio MDP, Virgilio AD, Dietz A, Drago M, Fafone V, Ferrante I, Fidecaro F, Fiori I, Flaminio R, Fournier JD, Franc J, Frasca S, Frasconi F, Freise A, Galimberti M, Gammaitoni L, Garufi F, Gemme G, Genin E, Gennai A, Giazotto A, Gouaty R, Granata M, Greverie C, Guidi G, Heitmann H, Hello P, Hild S, Huet D, Jaranowski P, Kowalska I, Królak A, Penna PL, Leroy N, Letendre N, Li TGF, Lorenzini M, Loriette V, Losurdo G, Mackowski JM, Majorana E, Man N, Mantovani M, Marchesoni F, Marion F, Marque J, Martelli F, Masserot A, Menzinger F, Michel C, Milano L, Minenkov Y, Mohan M, Moreau J, Morgado N, Morgia A, Mosca S, Moscatelli V, Mours B, Neri I, Nocera F, Pagliaroli G, Palomba C, Paoletti F, Pardi S, Parisi M, Pasqualetti A, Passaquieti R, Passuello D, Persichetti G, Pichot M, Piergiovanni F, Pietka M, Pinard L, Poggiani R, Prato M, Prodi GA, Punturo M, Puppo P, Rabaste O, Rabeling DS, Rapagnani P, Re V, Regimbau T, Ricci F, Robinet F, Rocchi A, Rolland L, Romano R, Rosińska D, Ruggi P, Sassolas B, Sentenac D, Sturani R, Swinkels B, Toncelli A, Tonelli M, Tournefier E, Travasso F, Trummer J, Vajente G, Brand JFJVD, Putten SVD, Vavoulidis M, Vedovato G, Verkindt D, Vetrano F, Viceré A, Vinet JY, Vocca H, Was M, Yvert M. Status and perspectives of the Virgo gravitational wave detector. ACTA ACUST UNITED AC 2010. [DOI: 10.1088/1742-6596/203/1/012074] [Citation(s) in RCA: 24] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
|
24
|
Acernese F, Alshourbagy M, Amico P, Antonucci F, Aoudia S, Astone P, Avino S, Ballardin G, Baggio L, Barone F, Barsotti L, Barsuglia M, Bauer TS, Bigotta S, Birindelli S, Bizouard MA, Boccara AC, Bondu F, Bosi L, Braccini S, Bradaschia C, Brillet A, Brisson V, Buskulic D, Cagnoli G, Calloni E, Campagna E, Carbognani F, Carbone L, Cavalier F, Cavalieri R, Cella G, Cesarini E, Chassande-Mottin E, Chatterji S, Cleva F, Coccia E, Corda C, Corsi A, Cottone F, Coulon JP, Cuoco E, D'Antonio S, Dari A, Dattilo V, Davier M, De Rosa R, Del Prete M, Di Fiore L, Di Lieto A, Di Paolo Emilio M, Di Virgilio A, Evans M, Fafone V, Ferrante I, Fidecaro F, Fiori I, Flaminio R, Fournier JD, Frasca S, Frasconi F, Gammaitoni L, Garufi F, Genin E, Gennai A, Giazotto A, Giordano L, Granata V, Greverie C, Grosjean D, Guidi G, Hamdani S, Hebri S, Heitmann H, Hello P, Huet D, La Penna P, Laval M, Leroy N, Letendre N, Lopez B, Lorenzini M, Loriette V, Losurdo G, Mackowski JM, Majorana E, Man N, Mantovani M, Marchesoni F, Marion F, Marque J, Martelli F, Masserot A, Menzinger F, Milano L, Minenkov Y, Moins C, Morgado N, Mosca S, Mours B, Neri I, Nocera F, Pagliaroli G, Palomba C, Paoletti F, Pardi S, Pasqualetti A, Passaquieti R, Passuello D, Persichetti G, Piergiovanni F, Pinard L, Poggiani R, Punturo M, Puppo P, Rabaste O, Rapagnani P, Regimbau T, Remillieux A, Ricci F, Ricciardi I, Rocchi A, Rolland L, Romano R, Ruggi P, Russo G, Sentenac D, Solimeno S, Swinkels BL, Tarallo M, Terenzi R, Toncelli A, Tonelli M, Tournefier E, Travasso F, Vajente G, van den Brand JFJ, van der Putten S, Verkindt D, Vetrano F, Viceré A, Vinet JY, Vocca H, Yvert M. In-vacuum optical isolation changes by heating in a Faraday isolator. Appl Opt 2008; 47:5853-5861. [PMID: 19122727 DOI: 10.1364/ao.47.005853] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
We describe a model evaluating changes in the optical isolation of a Faraday isolator when passing from air to vacuum in terms of different thermal effects in the crystal. The changes are particularly significant in the crystal thermal lensing (refraction index and thermal expansion) and in its Verdet constant and can be ascribed to the less efficient convection cooling of the magneto-optic crystal of the Faraday isolator. An isolation decrease by a factor of 10 is experimentally observed in a Faraday isolator that is used in a gravitational wave experiment (Virgo) with a 10 W input laser when going from air to vacuum. A finite element model simulation reproduces with a great accuracy the experimental data measured on Virgo and on a test bench. A first set of measurements of the thermal lensing has been used to characterize the losses of the crystal, which depend on the sample. The isolation factor measured on Virgo confirms the simulation model and the absorption losses of 0.0016 +/- 0.0002/cm for the TGG magneto-optic crystal used in the Faraday isolator.
Collapse
|
25
|
Acernese F, Amico P, Alshourbagy M, Antonucci F, Aoudia S, Astone P, Avino S, Baggio L, Ballardin G, Barone F, Barsotti L, Barsuglia M, Bauer TS, Bigotta S, Bizouard MA, Boccara C, Bondu F, Bosi L, Bradaschia C, van den Brand JFJ, Birindelli S, Braccini S, Brillet A, Brisson V, Buskulic D, Cagnoli G, Calloni E, Campagna E, Carbognani F, Cavalier F, Cavalieri R, Cella G, Cesarini E, Chassande-Mottin E, Clapson AC, Cleva F, Coccia E, Corda C, Corsi A, Cottone F, Coulon JP, Cuoco E, D’Antonio S, Dari A, Dattilo V, Davier M, del Prete M, De Rosa R, Di Fiore L, Di Lieto A, Di Virgilio A, Dujardin B, Evans M, Fafone V, Ferrante I, Fidecaro F, Fiori I, Flaminio R, Fournier JD, Frasca S, Frasconi F, Gammaitoni L, Garufi F, Genin E, Gennai A, Giazotto A, Giordano L, Granata V, Greverie C, Grosjean D, Guidi G, Hamdani S, Hebri S, Heitmann H, Hello P, Huet D, Kreckelbergh S, La Penna P, Laval M, Leroy N, Letendre N, Lopez B, Lorenzini M, Loriette V, Losurdo G, Mackowski JM, Majorana E, Man CN, Mantovani M, Marchesoni F, Marion F, Marque J, Martelli F, Masserot A, Menzinger F, Milano L, Minenkov Y, Moins C, Moreau J, Morgado N, Mosca S, Mours B, Neri I, Nocera F, Pagliaroli G, Pallottino GV, Palomba C, Paoletti F, Pardi S, Pasqualetti A, Passaquieti R, Passuello D, Piergiovanni F, Pinard L, Poggiani R, Punturo M, Puppo P, van der Putten S, Rapagnani P, Regimbau T, Reita V, Remillieux A, Ricci F, Ricciardi I, Rocchi A, Romano R, Ruggi P, Russo G, Solimeno S, Spallicci A, Tarallo M, Terenzi R, Tonelli M, Toncelli A, Tournefier E, Travasso F, Tremola C, Vajente G, Verkindt D, Vetrano F, Viceré A, Vinet JY, Vocca H, Yvert M. The Virgo 3 km interferometer for gravitational wave detection. ACTA ACUST UNITED AC 2008. [DOI: 10.1088/1464-4258/10/6/064009] [Citation(s) in RCA: 30] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
|
26
|
Alshourbagy M, Toncelli A, Tonelli M, Marchetti F. Silicon crystal fibers: difficulties and progress. Cryst Res Technol 2007. [DOI: 10.1002/crat.200610881] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/05/2022]
|
27
|
Acernese F, Alshourbagy M, Amico P, Aoudia S, Antonucci F, Astone P, Avino S, Babusci D, Ballardin G, Barone F, Barsuglia M, Barsotti L, Beauville F, Bigotta S, Birindelli S, Bizouard MA, Boccara AC, Bondu F, Bosi L, Braccini S, Bradaschia C, Brillet A, Brisson V, Brocco L, Buskulic D, Calloni E, Campagna E, Cavalier F, Carbognani F, Cavalieri R, Cella G, Cesarini E, Chassande-Motin E, Christensen N, Clapson AC, Frédéric C, Corda C, Corsi A, Cottone F, Coulon JP, Cuoco E, Dari A, Datillo V, Davier M, del Prete M, De Rosa R, Di Fiore L, Di Virgilio A, Dujardin B, Eleuteri A, Ferrante I, Fidecaro F, Fiori I, Flaminio R, Fourier JD, Frasca S, Frasconi F, Francois O, Gammaitoni L, Garufi F, Genin E, Gennai A, Giazotto A, Giordano G, Giordano L, Gouaty R, Grosjean D, Guidi GM, Hebri S, Heitmann H, Hello P, Karkar S, Kreckelbergh S, La Penna P, Laval M, Leroy N, Letendre N, Lopez B, Lorenzini M, Loriette V, Losurdo G, Mackowski JM, Majorana E, Mantovani M, Marchesoni F, Marion F, Marque J, Martelli F, Masserot A, Mazzoni M, Menzinger F, Moreau J, Milano L, Moins C, Morgado N, Mours B, Nary-Man C, Nocera F, Pai A, Palomba C, Paoletti F, Pardi S, Pasqualetti A, Passaquieti R, Passuello D, Perniola B, Piergiovanni F, Pinard L, Poggiani R, Punturo M, Puppo P, Qipiani K, Rapagnani P, Ricci F, Reita V, Remillieux A, Ricciardi I, Ruggi P, Russo G, Solimeno S, Spallicci A, Stanga R, Tarallo M, Toncelli A, Tonelli M, Tournefier E, Travasso F, Tremola C, Vajente G, Verkindt D, Vetrano F, Viceré A, Vinet JY, Vocca H, Yvert M. Measurement of the optical parameters of the Virgo interferometer. Appl Opt 2007; 46:3466-84. [PMID: 17514306 DOI: 10.1364/ao.46.003466] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/15/2023]
Abstract
The Virgo interferometer, aimed at detecting gravitational waves, is now in a commissioning phase. Measurements of its optical properties are needed for the understanding of the instrument. We present the techniques developed for the measurement of the optical parameters of Virgo. These parameters are compared with the Virgo specifications.
Collapse
|
28
|
Galzerano G, Laporta P, Bonelli L, Toncelli A, Tonelli M. Single-frequency diode-pumped Yb:KYF(4) laser around 1030 nm. Opt Express 2007; 15:3257-3264. [PMID: 19532566 DOI: 10.1364/oe.15.003257] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
Widely-tunable cw laser action has been demonstrated in a diode-pumped Yb:KYF(4) crystal. A comprehensive characterization of the active material and laser performance are reported, with particular attention to single-frequency laser operation. Single longitudinal-mode operation is achieved in the tuning range from 1020 to 1045 nm with a maximum output power of 150 mW. The relative intensity noise of the single-frequency laser is limited by quantum noise contribution for Fourier frequencies larger than 1 MHz.
Collapse
|
29
|
Alshourbagy M, Parisi D, Toncelli A, Tonelli M, Marchetti F. Growth and characterization of LiF single crystal fibers. Cryst Res Technol 2006. [DOI: 10.1002/crat.200610741] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
|
30
|
Galzerano G, Laporta P, Sani E, Bonelli L, Toncelli A, Tonelli M, Pesatori A, Svelto C. Room-temperature diode-pumped Yb:KYF(4) laser. Opt Lett 2006; 31:3291-3. [PMID: 17072400 DOI: 10.1364/ol.31.003291] [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] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/12/2023]
Abstract
Continuous-wave laser action has been demonstrated in a diode-pumped Yb:KYF(4) crystal. Crystal growth, spectroscopic measurements, and laser results are presented. A maximum output power of 505 mW, a slope efficiency of 43%, and a continuous wavelength tunability range of 65nm, from 1013 to 1078 nm, have been obtained at room temperature.
Collapse
Affiliation(s)
- Gianluca Galzerano
- Istituto di Fotonica e nanotecnologie-Consiglio Nazionale delle Richerche and Dipartimento di Fisica del Politecnico di Milano, Italy.
| | | | | | | | | | | | | | | |
Collapse
|
31
|
Richter A, Pavel N, Heumann E, Huber G, Parisi D, Toncelli A, Tonelli M, Diening A, Seelert W. Continuous-wave ultraviolet generation at 320 nm by intracavity frequency doubling of red-emitting Praseodymium lasers. Opt Express 2006; 14:3282-3287. [PMID: 19516470 DOI: 10.1364/oe.14.003282] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
We describe a new approach for the generation of coherent ultraviolet radiation. Continuous-wave ultraviolet light at 320 nm has been obtained by intracavity frequency doubling of red-emitting Praseodymium lasers. Lasing at the 640-nm fundamental wavelength in Pr:LiYF(4) and Pr:BaY(2)F(8) was realized by employing an optically pumped semiconductor laser at 480 nm as pump source.Using LiB(3)O(5) as nonlinear medium, ~19 mW of ultraviolet radiation with ~9% optical efficiency with respect to absorbed power was reached for both laser crystals; the visible-to-ultraviolet conversion efficiency was 26% and 35% for Pr:LiYF(4) and Pr:BaY(2)F(8), respectively.
Collapse
|
32
|
Coluccelli N, Galzerano G, Laporta P, Parisi D, Toncelli A, Tonelli M. Room-temperature Q-switched Tm:BaY(2)F(8) laser pumped by CW diode laser. Opt Express 2006; 14:1518-1523. [PMID: 19503477 DOI: 10.1364/oe.14.001518] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
We report on the realization of CW diode-pumped Tm:BaY(2)F(8) Q-switched laser at 1.93 microm. Active Q-switching was obtained by means of an intracavity Pockels cell. A functional characterization of the laser performance is presented with particular attention to output energy, pulse duration, pulse stability, and wavelength tunability. Pulses with time duration as short as 170 ns were demonstrated at the minimum repetition rate of 5 Hz with an energy of 3.2 mJ (corresponding to a peak power of 19 kW). A wavelength tunability range from 1905 nm to 1990 nm has been observed.
Collapse
|
33
|
Abstract
We report on the spectroscopic characterization of Tm :KYF(4) and Ho :KYF(4) single crystals. The energy level splittings are given, as well as the Judd-Ofelt parameters, the polarized absorption and emission cross sections and the energy transfer coefficients. This allows to have a deeper understanding of the Tm-Ho-codoped KYF(4) system and shows KYF(4) to be a promising material for widely tunable and efficient 2 µm laser operation.
Collapse
|
34
|
Abstract
We present the Erbium (4)I(11/2) and (4)I(13/2) complete polarized spectroscopic investigation on a series of Er(3+),Ce(3+):BaY(2)F(8) single crystals as a function of Cerium concentration. The main results of room temperature lifetime investigation show that the (4)I(13/2) lifetime reduces from 15.6 ms to 10 ms, the (4)I(11/2) lifetime reduces from 8.3 ms to 0.2 ms and (4)S(3/2) lifetime reduces from 420 to 110 micros when adding 4% Ce-codoping. Moreover, in the same experimental conditions, the fluorescence intensity from (4)I(13/2) increases by four times when adding 4%Ce, and the intensity of the 3 microm (4)I(11/2) ?(4)I(13/2) transition becomes undetectable. The experimental data are interpreted with a rate equation model. The obtained results could be interesting in perspective of obtaining a low-threshold 1.5 microm Er laser.
Collapse
|
35
|
Galzerano G, Cornacchia F, Parisi D, Toncelli A, Tonelli M, Laporta P. Widely tunable 1.94-microm Tm:BaY2F8 laser. Opt Lett 2005; 30:854-6. [PMID: 15865377 DOI: 10.1364/ol.30.000854] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/02/2023]
Abstract
A novel BaY2F8 crystal doped with thulium ions is grown and extensively investigated. Owing to the large number of vibronic levels and to a favorable electron-phonon coupling, extremely wide absorption and emission bands around 1.9 microm are observed. A room-temperature Tm:BaY2F8 laser tunable over a 210-nm interval, from 1849 to 2059 nm, is demonstrated.
Collapse
Affiliation(s)
- Gianluca Galzerano
- Istituto di Fotonica e Nanotecnologie, Consiglio Nazionale delle Ricerche, Dipartimento di Fisica del Politecnico di Milano, Piazza Leonardo da Vinci 32, Milano 20133, Italy.
| | | | | | | | | | | |
Collapse
|
36
|
Agnesi A, Carraro G, Guandalini A, Reali G, Sani E, Toncelli A, Tonelli M. 1-mJ Q-switched diode-pumped Nd:BaY(2)F(8) laser. Opt Express 2004; 12:3765-3769. [PMID: 19483908 DOI: 10.1364/opex.12.003765] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
We report what is to our knowledge the first high repetition rate Q-switched Nd:BaY(2)F(8) (Nd:BaYF) laser pumped with a multiwatt fiber-coupled diode array tuned at 806 nm. As much as 2.42 W of average power and up to 1.05 mJ of pulse energy were obtained with 6.1 W of absorbed pump power, with excellent beam quality (M(2)<1.2) and linear polarization.
Collapse
|
37
|
Agnesi A, Guandalini A, Tomaselli A, Sani E, Toncelli A, Tonelli M. Diode-pumped passively mode-locked and passively stabilized Nd3+:BaY2F8 laser. Opt Lett 2004; 29:1638-1640. [PMID: 15309844 DOI: 10.1364/ol.29.001638] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/24/2023]
Abstract
Continuous-wave mode locking (CW-ML) of a diode-pumped Nd3+:BaY2F8 laser is reported for the first time to our knowledge. Pulses as short as 4.8 ps were measured with a total output power of approximately 1 W at 1049 nm, corresponding to 3.4 W of absorbed power from the pump diode at 806 nm. A novel technique for passive stabilization of CW-ML has been demonstrated.
Collapse
Affiliation(s)
- Antonio Agnesi
- Istituto Nazionale di Fisica della Materia e Dipartimento di Elettronica dell'Universitá di Pavia, Via Ferrata, Pavia, Italy
| | | | | | | | | | | |
Collapse
|
38
|
Cornacchia F, Parisi D, Bernardini C, Toncelli A, Tonelli M. Efficient, diode-pumped Tm(3)+:BaY(2)F(8) vibronic laser. Opt Express 2004; 12:1982-1989. [PMID: 19475032 DOI: 10.1364/opex.12.001982] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
In this work we report the spectroscopy and laser results of several Thulium doped BaY(2)F(8) single crystals grown using the Czochralski technique. The doping concentration is between 2at.% and 18at.%. We performed room temperature laser experiments pumping the samples with a laser diode at 789 nm obtaining 61% as maximum optical-to-optical efficiency with a maximum output power of 290 mW and a minimum lasing threshold of 26 mW. The lasing wavelength changed with the dopant concentration from 1927 nm up to 2030 nm and the nature of the transition changed from purely electronic to vibronic, accordingly.
Collapse
|
39
|
Galzerano G, Sani E, Toncelli A, Della Valle G, Taccheo S, Tonelli M, Laporta P. Widely tunable continuous-wave diode-pumped 2-microm Tm-Ho:KYF4 laser. Opt Lett 2004; 29:715-717. [PMID: 15072368 DOI: 10.1364/ol.29.000715] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/24/2023]
Abstract
Continuous-wave laser action at approximately 2 microm is demonstrated in a Tm-Ho:KYF4 single crystal at room temperature. Crystal growth, spectroscopic measurements, and laser results are presented. An output power in excess of 250 mW is obtained with a tuning range of 99 nm, the largest ever published, to our knowledge, for Tm-Ho in any crystalline host.
Collapse
Affiliation(s)
- Gianluca Galzerano
- Istituto di Fotonica e Nanotecnologie, Consiglio Nazionale delle Ricerche, Dipartimento di Fisica del Politecnico di Milano, Piazza L. da Vinci 32, Milano 20133, Italy.
| | | | | | | | | | | | | |
Collapse
|
40
|
Galzerano G, Marano M, Longhi S, Sani E, Toncelli A, Tonelli M, Laporta P. Sub-100-ps amplitude-modulation mode-locked Tm-Ho:BaY2F8 laser at 2.06 microm. Opt Lett 2003; 28:2085-2087. [PMID: 14587823 DOI: 10.1364/ol.28.002085] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/24/2023]
Abstract
We report the generation of sub-100-ps pulse trains near the 2.06-microm wavelength in an actively mode-locked diode-pumped Tm-Ho:BaYF laser operating at room temperature. Transform-limited, 97-ps Gaussian pulses at a 100-MHz repetition rate with an average power in excess of 20 mW and with a carrier wavelength tunable by approximately 50 nm near 2.066 microm are demonstrated.
Collapse
Affiliation(s)
- G Galzerano
- Istituto di Fotonica e Nanotecnologie--Consiglio Nazionale delle Ricerche and Istituto Nazionale per la Fisica della Materia, Dipartimento di Fisica del Politecnico di Milano, Piazza L. da Vinci 32, Milano 20133, Italy.
| | | | | | | | | | | | | |
Collapse
|
41
|
Agnesi A, Guandalini A, Lucca A, Sani E, Toncelli A, Tonelli M, Dell'acqua S. Medium-power diode-pumped Nd:BaY2F8 laser. Opt Express 2003; 11:1149-1155. [PMID: 19465981 DOI: 10.1364/oe.11.001149] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
We report what is to our knowledge the first Nd:BaY2F8 (Nd:BaYF) laser pumped with a multiwatt fiber-coupled diode array tuned at approximately 804 nm. As much as 2.4 W were obtained with 6.2 W of absorbed pump power, showing efficient operation (51% slope efficiency), excellent beam quality (M2=1.1), and weak thermal lensing. Small intracavity losses (<1%) were measured, indicating both reduced thermally induced aberrations and good optical quality of the laser crystal.
Collapse
|
42
|
Abstract
We demonstrate a new technique for discovering the main mechanisms of energy transfer inside the active crystal of a solid-state laser. It consists of measuring the harmonic content of fluorescence when the pump has a sinusoidal modulation. In particular we discuss excited-state absorption and upconversion and present the equations for the fundamental and the second harmonic for both of these processes. We measured the fluorescence from the (4)S(3/2) multiplet of Er(3+) in three hosts, YLF, YAG, and CaSGG, with different doping. The results of the new method show that we are able to identify which multiplets transfer their energy to the observed one and through which process.
Collapse
|