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Vanaja M, Sarkar B, Sathish P, Jyothi Lakshmi N, Yadav SK, Mohan C, Sushma A, Yashavanth BS, Srinivasa Rao M, Prabhakar M, Singh VK. Elevated CO 2 ameliorates the high temperature stress effects on physio-biochemical, growth, yield traits of maize hybrids. Sci Rep 2024; 14:2928. [PMID: 38316909 PMCID: PMC10844601 DOI: 10.1038/s41598-024-53343-2] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/20/2023] [Accepted: 01/31/2024] [Indexed: 02/07/2024] Open
Abstract
The rising temperatures and levels of carbon dioxide in the atmosphere are anticipated to have a significant impact on the productivity of agricultural crops. Although, the individual effects of elevated CO2 and temperature have been extensively studied in C3 and C4 crops, there remains a scarcity of research investigating their interactive effects specifically on maize hybrids. The impact of elevated temperature and its interaction with elevated CO2 on phenology, physiology, biomass, and grain yield of maize hybrids was assessed in a field experiment using Free Air Temperature Elevation (FATE) facility. The results showed that elevated temperature (eT) increased the anthesis silking interval (ASI), while the presence of elevated CO2 along with elevated temperature (eT + eCO2) mitigated this effect. The differential expression were observed between hybrids depending on their genetic potential. Furthermore, the net photosynthetic rate (Anet), stomatal conductance (gs), and transpiration rate (Tr) of hybrids decreased under elevated temperature but eT + eCO2 condition helped in reverting its impact to some extent. In term of leaf composition, the highest level of total soluble sugars (TSS) and starch was observed under eT + eCO2 conditions, possibly due to improved Anet in the presence of elevated eCO2. The negative impact of eT was also evident through increased proline and MDA content, but eT + eCO2 ameliorated the adverse effect of eT. The biomass and grain yield also responded similarly, among the hybrids 900M GOLD recorded superior performance for grain yield at eT condition exceeding 35 °C. On the other hand, DHM117 experienced a significant reduction in grain yield under eT, but performed better under eT + eCO2 due to its improved physiological response to eCO2. The study indicated that elevated levels of carbon dioxide can actually mitigate the detrimental effects of elevated temperature on maize crop. This positive impact on maize crop can be attributed to an enhanced physiological performance in the presence of eCO2 which enables the plants to maintain satisfactory yield levels despite the challenging environmental conditions.
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Affiliation(s)
- M Vanaja
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
| | - B Sarkar
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India.
| | - P Sathish
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
| | - N Jyothi Lakshmi
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
| | - S K Yadav
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
| | - Ch Mohan
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
| | - A Sushma
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
| | - B S Yashavanth
- ICAR-National Academy of Agricultural Research Management, Rajendranagar, Hyderabad, India
| | - M Srinivasa Rao
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
| | - M Prabhakar
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
| | - V K Singh
- ICAR-Central Research Institute for Dryland Agriculture, Santoshnagar, Hyderabad, TS, 500 059, India
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Haldar S, Sarkar B, Dixit A. Dose to Organ at Risk and its Characteristic Variation with the Clinically Used Different Prescription Levels for Early-stage Left-sided Breast Cancer. Clin Oncol (R Coll Radiol) 2024; 36:21-29. [PMID: 38040550 DOI: 10.1016/j.clon.2023.11.038] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/06/2023] [Revised: 05/27/2023] [Accepted: 11/22/2023] [Indexed: 12/03/2023]
Abstract
AIMS To evaluate the organ at risk (OAR) dose and its characteristic variation with different clinically usable prescription doses (RxD) for breast and chest wall radiotherapy in patients with early-stage left-sided breast cancer. MATERIALS AND METHODS In total, 145 patients with early-stage breast cancers (T1N0M0-T2N0M0) on the left side were treated with radiotherapy after a modified radical mastectomy or breast conservation surgery, with a mean age of 45.1 ± 21.6 years. The patient received 4050 cGy of field-in-field (three-dimensional conformal radiotherapy) treatment limited to the breast or chest wall, excluding the supraclavicular node, axillary node and internal mammary chain, over 15 fractions. Additional plans of 5000 cGy/25 fractions, 4500 cGy/20 fractions and 2600 cGy/5 fractions were created with no or minor changes to the original plan. Mathematical modelling was used to study the distinctive change in the dose-volume characteristics for various OARs as a function of the RxD. OAR dosages, both absolute and normalised, were expressed in terms of the RxD. The mathematical (functional) relationship between OAR doses and different prescription levels was deduced by the least squares fit method. RESULT The left lung mean dose, V5Gy (%), V10Gy (%) and V20Gy (%) and the heart mean dose, V10Gy (%) and V20Gy (%) were evaluated. The dose-volume parameters showed a parabolic variation (x2) with the RxD. Prescription normalised OAR doses showed a linear relationship with the RxD; relative dose increased with diminishing RxD. Normalised lung and heart mean doses exhibited saturation (linear relationship) with RxD variation. Paired sample t-test results between RxD versus all evaluated parameters were found to be statistically significant (P = 0.004). The Pearson correlation coefficient between different prescription levels for left lung mean dose (range 0.942-1.0), heart mean dose (range 1.0-1.0), left lung V5Gy (%) (range 0.987-1.0), left lung V10Gy (%) (range 0.991-0.999), heart V10Gy (%) (range 0.998-1.0). CONCLUSION The functional form of absolute OAR dose-volume parameters versus RxD is parabolic and the RxD normalised OAR dose-volume parameter versus RxD is a straight line with a negative slope as RxD increases. This indicates an increase in the relative OAR dose-volume parameters if the RxD is reduced. This study is the first of its kind to compare the OAR doses as a function of clinically used degenerate prescription levels. These data will help to comprehend the OAR doses while adopting a new dose fractionation regimen and reviewing the radiotherapy treatment plans.
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Affiliation(s)
- S Haldar
- Department of Radiation Oncology, Saroj Gupta Cancer Centre and Research Institute, Kolkata, India; Department of Physics, Institute of Applied Science and Humanities, GLA University, Mathura, India
| | - B Sarkar
- Department of Radiation Oncology, Apollo Multispeciality Hospital, Kolkata, India.
| | - A Dixit
- Department of Mathematics, Institute of Applied Science and Humanities, GLA University, Mathura, India
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Sarkar B, Shahid T, Bhattacharya J, Chatterjee P, Biswas LN, Goswami S, Ghosh T, Ghosh SK, Pradhan A. A General Assessment of India's Extremely Low Number of Transgender Cancer Patients. Int J Radiat Oncol Biol Phys 2023; 117:e54. [PMID: 37785667 DOI: 10.1016/j.ijrobp.2023.06.766] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/04/2023]
Abstract
PURPOSE/OBJECTIVE(S) Physiological transgender (TJ) is one of the most marginalized and oppressed community in the Indian subcontinent. The observable percentage of physiological transgender (TJ) cancer patients is extremely low. This concise report aims to assess the factors that contribute to the scarcity of transgender cancer patients. MATERIALS/METHODS The hospital database (2012-2021) of 2 centers in New Delhi (population 32 million) & 1 in Kolkata (15 million) were evaluated. In addition, 28 senior oncologists (ONC) and 17 trans women (TWs) completed a six-point questionnaire. ONC was asked how many TJ patients they had seen in their career, as well as histopathology/site. Furthermore, the data was extrapolated to account for all clinicians' cumulative years of experience. The questions for TWs were age and where they go if you have a disease or illness. And, do they know any TJ cancer patients? RESULTS India's last census (2011) revealed a half-million TJ population. TJ density must be at least 1 million to be comparable to the rest of the world. Hospital databases counted 10,486 patients, with no patient identified as TJ. A total of 37 TJ cancer patients were reported by 28 ONC with an average and collective years of their medical service of 23.1±4.1 and 646 years; distributed in 3 metropolis of 67 million (combined) population (Kolkata, New Delhi, and Mumbai). The average lifetime number of TJ cancer patients/oncologist was 1.3±1.1. Total 12 cases were head neck cancers, with 4 caused by human papillomavirus. The remaining 25 patients have 5 lung, 5 gynecological, 4 breast, 3 brain cancers, 2 soft tissue sarcomas, and 6 cases of unknown origin. The density of 5-year prevalent cancer cases in India is 0.2%, with an estimated 0.007% of TJ cancer patients. TW could not identify any cancer patients in their community. CONCLUSION Being transgender is a social taboo in this part of the world. Their legal rights and classification as the third gender are uncommon. TJs are denied access to standard education, mainstream occupations, and social respect. Although the exact number has never been determined, it is estimated that a large proportion (≈90%) of TJ people are forced to choose roadside begging and working as cheap sex workers. There is no clinical reason why TJs should have fewer cancer incidents, they should be more susceptible to cancer due to unhealthy living conditions, unprotected sex, lack of medical care, proper nutrition, and all other factors associated with their very low socioeconomic status. Nonetheless, it's difficult to find single TJ cancer patients in both public and private hospital OPD. They may be unable to access a traditional clinic due to social discrimination, financial constraints, or they may be unwilling to disclose their true sex. Even TJ's do not show up at free public clinics. The disclosure of true sex may be beneficial in obtaining better treatment, but the more prevalent reason is social unacceptability, which can be overcome through proper education and community economic growth.
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Affiliation(s)
- B Sarkar
- Apollo Multispecialty Hospitals, Kolkata, India; GLA University, Mathura, India
| | - T Shahid
- Apollo Multispecialty Hospitals, Kolkata, India
| | | | | | - L N Biswas
- Apollo Multispecialty Hospitals, Kolkata, India
| | - S Goswami
- Apollo Multispecialty Hospitals, Kolkata, India
| | - T Ghosh
- Apollo Multispecialty Hospitals, Kolkata, India
| | - S K Ghosh
- Apollo Multispecialty Hospitals, Kolkata, India
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Saha A, Mishra A, Manna S, Ghosh T, Bhattacharya J, Goswami S, Biswas L, Mitra S, Sarkar B, Banik A, Chowdhury S, Biswal S, Mandal S, George K, Soren P, Gazi M. 109P Setting up 4D-CT based image guided radiotherapy (IGRT) for locally advanced lung cancer: Is it safe to reduce PTV margin for dosimetric benefit? J Thorac Oncol 2023. [DOI: 10.1016/s1556-0864(23)00364-7] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 04/03/2023]
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Arunkumar D, Krishnani KK, Kumar N, Sarkar B, Upadhyay AK, Sawant PB, Chadha NK, Abisha R. Mitigating abiotic stresses using natural and modified stilbites synergizing with changes in oxidative stress markers in aquaculture. Environ Geochem Health 2023:10.1007/s10653-023-01507-w. [PMID: 36882549 DOI: 10.1007/s10653-023-01507-w] [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] [Subscribe] [Scholar Register] [Received: 07/06/2022] [Accepted: 02/10/2023] [Indexed: 06/18/2023]
Abstract
In-depth mineralogical understanding and characterization are necessary to explore potential applications of clinoptilolites. In this study, the clinoptilolite collected from quarries and identified as stilbite microscopically and spectroscopically was subjected to physical and chemical treatments for the synthesis of modified stilbites, which were further evaluated for determining their removal efficiencies on ammonical contaminant in a predetermined concentration range from various source of aquaculture water namely fish pond, aquaponics and ornamental under laboratory condition. High-resolution transmission electron microscope results revealed that stilbite was rod-shaped in all forms but physically modified stilbite contains some nano-zeolite particles, synthesized probably due to heat treatment. The natural zeolite (stilbite) and microwave sodium acetate treated stilbite were found to be most effective in ammonia removal, hence both these products were further evaluated for the removal of cadmium and lead under laboratory conditions and for the ammonia removal in fish pond water under wet lab conditions. The results showed that these zeolites at 10-100 mg/L and 100-200 mg/L had a better removal efficiency of ammonical and metallic contaminants, respectively. Fish samples were taken at particular intervals to determine oxidative stress parameters, i.e., superoxide dismutase and catalase enzyme activities were found to be increased in control fish samples without treatment due to abiotic stress caused by higher ammonia concentration. The levels of oxidative stress markers are decreased in the treatments with zeolite-stilbite which brings to light its potential efficiency in alleviating stress in fish. This study revealed the potential of natural and abundantly available native zeolite-stilbite and its chemically modified form in relieving ammonical stress from the aquaculture system. This work has potential applications for the environmental management of aquaculture, ornamental fisheries, and aquaponics.
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Affiliation(s)
- D Arunkumar
- ICAR-Central Institute of Fisheries Education, Panch Marg, Off Yari Road, Versova, Mumbai, Andheri (W), 400061, India
| | - K K Krishnani
- ICAR-Central Institute of Fisheries Education, Panch Marg, Off Yari Road, Versova, Mumbai, Andheri (W), 400061, India.
| | - Neeraj Kumar
- ICAR-National Institute of Abiotic Stress Management, Baramati, Pune, 413115, India
| | - B Sarkar
- ICAR-Indian Institute of Agricultural Biotechnology, Ranchi, India
| | - A K Upadhyay
- ICAR-National Research Centre for Grapes, Pune, India
| | - P B Sawant
- ICAR-Central Institute of Fisheries Education, Panch Marg, Off Yari Road, Versova, Mumbai, Andheri (W), 400061, India
| | - N K Chadha
- ICAR-Central Institute of Fisheries Education, Panch Marg, Off Yari Road, Versova, Mumbai, Andheri (W), 400061, India
| | - R Abisha
- ICAR-Central Institute of Fisheries Education, Panch Marg, Off Yari Road, Versova, Mumbai, Andheri (W), 400061, India
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Sarkar B, Shahid T, Biswal S, Appunu K, Bhattacharya J, Ghosh T, De A, George K, Mandal S, Roy Chowdhury S, Ganesh T, Munshi A, Mukherjee M, Das A, Soren P, Arjunan M, Chatterjee P, Biswas L, Pradhan A. A Comparative Dose-Escalation Analysis for the Head and Neck Reirradiation Patients with and without Appropriate DICOM Based Dose-Volume Information of Primary Radiotherapy. Int J Radiat Oncol Biol Phys 2022. [DOI: 10.1016/j.ijrobp.2022.07.1668] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/29/2022]
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Dubey S, Iyer RD, Azam MQ, Sarkar B, Nongdamba H. Thigh Pain and Peri-Implant Fractures with the Use of Short Cephalo-medullary Nails: A Retrospective Study of 122 Patients. Malays Orthop J 2022; 16:17-23. [PMID: 36589363 PMCID: PMC9791908 DOI: 10.5704/moj.2211.004] [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] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/31/2021] [Accepted: 02/21/2022] [Indexed: 12/12/2022] Open
Abstract
Introduction To assess the incidence and causes of persistent thigh pain and peri-implant fractures after union in patients of intertrochanteric fractures treated with short cephalo-medullary nails. Materials and methods A retrospective observational study conducted at a Level 1 Trauma centre. A total of 122 patients of intertrochanteric fractures who were operated using short cephalo-medullary nails (170mm and 200mm lengths) between January 2018 to June 2019 were included in the study. Main outcomes measured were the incidence of thigh pain and peri-implant fractures. Results Out of the 122 patients with a mean follow-up of 14.1 month, 12 patients had persistent thigh pain. Six patients had the helical blade protruding from the lateral cortex, two of them had distal tip of nail abutting on the anterior cortex and four cases had prominent proximal segment of nail which may explain the cause of their pain. Five of these patients had a combination of these findings. Two patients had pain for which no other obvious cause was found. There were no cases of peri-implant fractures in our study. Conclusion Thigh pain associated with the use of short cephalon-medullary nails is often unrelated to nail length and can be prevented by using proper surgical technique. There seems to be no association between the use of short nails and peri-implant fractures.
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Affiliation(s)
- S Dubey
- Department of Orthopaedics, Shri Ram Murti Smarak Institute of Medical Sciences, Bareilly, India
| | - RD Iyer
- Department of Orthopaedics, All India Institute of Medical Sciences, Raipur, India,Corresponding Author: Iyer R Dinesh, Department of Orthopaedics, All India Institute of Medical Sciences, Gate No, 1, Great Eastern Rd, opposite Gurudwara, AIIMS Campus, Tatibandh, Raipur, Chhattisgarh 492099, India
| | - MQ Azam
- Department of Trauma Surgery, All India Institute of Medical Sciences, Rishikesh, India
| | - B Sarkar
- Department of Orthopaedics, All India Institute of Medical Sciences, Rishikesh, India
| | - H Nongdamba
- Department of Orthopaedics, All India Institute of Medical Sciences, Rishikesh, India
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Shanker AK, Amirineni S, Bhanu D, Yadav SK, Jyothilakshmi N, Vanaja M, Singh J, Sarkar B, Maheswari M, Singh VK. High-resolution dissection of photosystem II electron transport reveals differential response to water deficit and heat stress in isolation and combination in pearl millet [ Pennisetum glaucum (L.) R. Br.]. Front Plant Sci 2022; 13:892676. [PMID: 36035679 PMCID: PMC9412916 DOI: 10.3389/fpls.2022.892676] [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: 03/09/2022] [Accepted: 07/19/2022] [Indexed: 06/15/2023]
Abstract
Heat and Water Deficit Stress (WDS) tend to impede and restrict the efficiency of photosynthesis, chlorophyll fluorescence, and maximum photochemical quantum yield in plants based on their characteristic ability to interfere with the electron transport system in photosystem II. Dissection of the electron transport pathway in Photosystem II (PSII) under water deficit and Heat Stress (HS) can be insightful in gaining knowledge on the various attributes of the photosynthetic performance of a plant. We attempt a high-resolution dissection of electron transport in PSII with studies on chlorophyll a fast fluorescence kinetics and non-photochemical quenching (NPQ) as a response to and recovery from these stresses in pearl millet [Pennisetum glaucum (L.) R. Br.] in isolation and combination. In this study, we bring out the mechanisms by which both heat and water stress, in isolation and in combination, affect the photosynthetic electron transport in Photosystem II. Our results indicate that oxygen evolution complex (OEC) damage is the primary effect of heat stress and is not seen with the same intensity in the water-stressed plants. Low exciton absorption flux in heat stress and combined stress was seen due to OEC damage, and this caused an electron transport traffic jam in the donor side of PS II. Both the specific energy flux model and the phenomenological flux model developed from the derived values in our study show that water deficit stress in combination with heat stress has a much stronger effect than the stresses in isolation on the overall electron transport pathway of the PS II in pearl millet plants.
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Sarkar B, Munshi A, Ganesh T, Rastogi K, Bansal K, Manikandan A, Mohanti BK, Pradhan A. Personal, Social, Economic and Professional Challenges Faced by Female Radiation Oncologists in South Asia. Clin Oncol (R Coll Radiol) 2021; 34:e81-e82. [PMID: 34810070 DOI: 10.1016/j.clon.2021.11.001] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/01/2021] [Revised: 10/20/2021] [Accepted: 11/02/2021] [Indexed: 11/03/2022]
Affiliation(s)
- B Sarkar
- Department of Radiotherapy, Apollo Multispeciality Hospitals, Kolkata, India; Department of Physics, GLA University, Mathura, India.
| | - A Munshi
- Department of Radiotherapy, Manipal Hospitals, Dwarka, New Delhi, India
| | - T Ganesh
- Department of Radiotherapy, Manipal Hospitals, Dwarka, New Delhi, India
| | - K Rastogi
- Department of Radiotherapy, Manipal Hospitals, Dwarka, New Delhi, India
| | - K Bansal
- Department of Radiotherapy, Manipal Hospitals, Dwarka, New Delhi, India
| | - A Manikandan
- Department of Medical Physics, Apollo Proton Cancer Center, Chennai, India
| | - B K Mohanti
- Department of Radiotherapy, Manipal Hospitals, Dwarka, New Delhi, India
| | - A Pradhan
- Department of Mathematics, GLA University, Mathura, India
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Sarkar B, Munshi A, Shahid T, Sengupta S, Bhaskar R, Ganesh T, Paul A, Bhattacharjee B, Pun R, Imbulgoda N, Biswal S, Rastogi K, Bansal K, Baba A, Yasmin T, Bhattacharya J, Ghosh T, De A, Chatterjee P, Pradhan A. Growth Characteristics of Woman Radiation Oncologists in South Asia: Assessment of Gender Neutrality and Leadership Position. Int J Radiat Oncol Biol Phys 2021. [DOI: 10.1016/j.ijrobp.2021.07.1027] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
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Sarkar B, Shahid T, Indira G, Biswal S, Sengupta S, Biswas L, Goswami S, Pusarla C, de A, Ghosh T, Mukherjee M, Samanta A, Raj R, Bhattacharya J. PO-1123 Post mastectomy RT planning on institutional, RTOG & ESTRO contouring guidelines comparison. Radiother Oncol 2021. [DOI: 10.1016/s0167-8140(21)07574-5] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
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Gupta R, Sarkar B, Sharma M, Choudhary S, Mahawar P. Increasing Azithromycin resistance Salmonella bacteremia in pediatric population in a secondary care center in India. Int J Infect Dis 2020. [DOI: 10.1016/j.ijid.2020.09.222] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/25/2022] Open
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Rastogi K, Sarkar B, Munshi A, Ganesh T, Bansal K, Pandey V, Mohanti B. Analysis of Medical Tourism of Cancer patients in Asia-Africa-Oceania region and Financial Toxicity due to Migration. Int J Radiat Oncol Biol Phys 2020. [DOI: 10.1016/j.ijrobp.2020.07.2494] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/23/2022]
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Sarkar B, Munshi A, Shahid T, Ganesh T, Mohanti B, Bansal K, Rastogi K, Chaudhari B, Manikandan A, Biswal S, Bhattacharya J, Ghosh T, De A, Roy Chowdhury S, Mandal S, George K, Mukherjee M, Gazi M, Chauhan R, Chatterjee P. Challenges Faced by Woman Radiation Oncologists (WRO) in South Asia. Int J Radiat Oncol Biol Phys 2020. [DOI: 10.1016/j.ijrobp.2020.07.2538] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022]
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Shahid T, Sarkar B, Mukherjee M, Bhattacharya J, Ghosh T, De A, Munshi A, Ganesh T. Assessment of Unplanned Treatment Interruptions During Modern Day Radiotherapy in a Large Patient Database. Int J Radiat Oncol Biol Phys 2020. [DOI: 10.1016/j.ijrobp.2020.07.1454] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/23/2022]
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Sarkar B, Rastogi K, Munshi A, Ganesh T, Bansal K, Tiwari S, Tyagi B, Mohanti B. Audit of Financial, Social and Logistic Concerns of Overseas Cancer Patients Treated at Tertiary Care Centers in New Delhi. Int J Radiat Oncol Biol Phys 2019. [DOI: 10.1016/j.ijrobp.2019.06.1495] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/26/2022]
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Shukla V, Lakhera VJ, Sarkar B. Extent of tritium contamination of cryogenic helium circuit in a fusion reactor: Mechanism and probable scenarios. Fusion Engineering and Design 2019. [DOI: 10.1016/j.fusengdes.2019.05.014] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 10/26/2022]
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Munshi A, Sarkar B, Roy S, Ganesh T, Mohanti B. Dose fall-off patterns with volumetric modulated arc therapy and three-dimensional conformal radiotherapy including the “organ at risk” effect. Experience of linear accelerator-based frameless radiosurgery from a single institution. Cancer Radiother 2019; 23:138-146. [DOI: 10.1016/j.canrad.2018.10.003] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/27/2018] [Revised: 09/22/2018] [Accepted: 10/02/2018] [Indexed: 12/31/2022]
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Sarkar B, Ganesh T, Manikandan A, Munshi A, Mohanti B. EP-1922: Standardisation of VMAT frameless SRS/SRT planning using ensemble mapped knowledge based planning. Radiother Oncol 2018. [DOI: 10.1016/s0167-8140(18)32231-x] [Citation(s) in RCA: 1] [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: 11/27/2022]
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V K, Osman S, Jassal K, Sarkar B, Singh S, Giri U, T G. EP-1774: Utilization Of Osld As The Quality Control Indicator For In-Vivo Measurements In Tbi Treatment. Radiother Oncol 2018. [DOI: 10.1016/s0167-8140(18)32083-8] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/30/2022]
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Dalal B, Sarkar B, De SK. Effect of Gd and Cr substitution on the structural, electronic and magnetic phases of SrRuO 3: a case study of doping and chemical phase separation. J Phys Condens Matter 2017; 29:495803. [PMID: 29087361 DOI: 10.1088/1361-648x/aa9728] [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: 06/07/2023]
Abstract
We explore the crystal structure, electrical resistivity and magnetic behavior of the compositional series (SrRuO3)[Formula: see text] (GdCrO3) x (where [Formula: see text]), which resides between orthorhombic ferromagnetic (FM) metal SrRuO3 ([Formula: see text] K) and orthorhombic antiferromagnetic (AFM) insulator GdCrO3 ([Formula: see text] K). Crystal structure analysis reveals that complete solid solution exists only up to [Formula: see text], above which chemical phase separation of two/three phases occurs, and persists up to [Formula: see text]. X-ray photoelectron spectroscopy measurement also corroborates the existence of [Formula: see text] for the intermediate composition [Formula: see text], which reinforces the astonishing scheelite-type GdCrO4 formation (at ambient pressure) for [Formula: see text] compositions. Electrical resistivity measurements affirm the temperature driven metal to insulator (M-I) transition for [Formula: see text] and [Formula: see text] samples. Low temperature insulating state in these samples is interpreted by electron-electron interaction of weak disordered systems. Precise analysis of temperature dependent resistivity for [Formula: see text] samples (which have insulating ground state) dictate that the transport phenomenon is mainly associated with Arrhenius-type charge conduction, Mott's variable range hopping, short-range and long-range Coulomb interaction mediated hopping processes, due to the high degree of randomness. Interruption of magnetic Ru-O-Ru interaction by Ru-O-Cr and Cr-O-Cr interactions lowers the FM transition temperature (T C), and thereby introduces Griffiths phase in phase separated samples. Furthermore, we believe that a sharp rise in magnetization at low temperature for [Formula: see text] samples is due to the formation of AFM GdCrO4 phase. Prominent thermal hysteresis in temperature dependent magnetization curves for [Formula: see text], and appearance of spin-reorientation transition for [Formula: see text] are the distinct indications for transformation into canted AFM GdCrO3 oxide at higher x. The effective magnetic moment ([Formula: see text]) continuously increases with the incorporation of higher moment elements (Gd and Cr); while coercive field (H C) exhibits an abrupt variation as a function of x at the onset of phase separation.
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Affiliation(s)
- B Dalal
- Department of Materials Science, Indian Association for the Cultivation of Science, Jadavpur, Kolkata-700032, India
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Mohapatra S, Sarkar B, Samantaray DP, Daware A, Maity S, Pattnaik S, Bhattacharjee S. Bioconversion of fish solid waste into PHB using Bacillus subtilis based submerged fermentation process. Environ Technol 2017; 38:3201-3208. [PMID: 28162048 DOI: 10.1080/09593330.2017.1291759] [Citation(s) in RCA: 42] [Impact Index Per Article: 6.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/06/2023]
Abstract
Currently, one of the major problem affecting the world is solid waste management, predominantly petroleum-based plastic and fish solid waste (FSW). However, it is very difficult to reduce the consumption of plastic as well as fish products, but it is promising to convert FSW to biopolymer to reduce eco-pollution. On account of that, the bioconversion of FSW extract to polyhydroxybutyrate (PHB) was undertaken by using Bacillus subtilis (KP172548). Under optimized conditions, 1.62 g/L of PHB has been produced by the bacterium. The purified compound was further characterized by advanced analytical technologies to elucidate its chemical structure. Results indicated that the biopolymer was found to be PHB, the most common homopolymer of polyhydroxyalkanoates (PHAs). This is the first report demonstrating the efficacy of B. subtilis to utilize FSW extract to produce biopolymer. The biocompatibility of the PHB against murine macrophage cell line RAW264.7 demonstrated that, it was comparatively less toxic, favourable for surface attachment and proliferation in comparison with poly-lactic acid (PLA) and commercially available PHB. Thus, further exploration is highly indispensable to use FSW extract as a substrate for production of PHB at pilot scale.
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Affiliation(s)
- S Mohapatra
- a Department of Biotechnology , Indian Institute of Technology , Roorke , India
| | - B Sarkar
- b ICAR-Indian Institute of Agricultural Biotechnology, IINRG Campus , Ranchi , Jharkhand , India
| | - D P Samantaray
- c Department of Microbiology , Orissa University of Agriculture and Technology , Bhubaneswar , Odisha, India
| | - A Daware
- d Department of Molecular Biology and Bioinformatics , Tripura University , Agartala , Tripura , India
| | - S Maity
- c Department of Microbiology , Orissa University of Agriculture and Technology , Bhubaneswar , Odisha, India
| | - S Pattnaik
- c Department of Microbiology , Orissa University of Agriculture and Technology , Bhubaneswar , Odisha, India
| | - S Bhattacharjee
- d Department of Molecular Biology and Bioinformatics , Tripura University , Agartala , Tripura , India
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Sarkar B, Munshi A, Manikandan A, Roy S, Ganesh T, Mohanti BK, Pradhan A. A low gradient junction technique of craniospinal irradiation using volumetric-modulated arc therapy and its advantages over the conventional therapy. Cancer Radiother 2017; 22:62-72. [PMID: 29195796 DOI: 10.1016/j.canrad.2017.07.047] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/18/2017] [Revised: 06/27/2017] [Accepted: 07/05/2017] [Indexed: 12/16/2022]
Abstract
A technique using volumetric-modulated arc therapy (VMAT) fields for craniospinal irradiation with low dose gradients at the field junction was tested for its sensitivity to positional inaccuracy. It was compared against the conventional three-dimensional (3D) conformal radiotherapy in terms of dose uniformity at the junction. Treatment plans generated for ten patients who received craniospinal irradiation (35Gy in 21 fractions) by VMAT technique at our centre were included in this study. For these patients, 3D conformal radiotherapy plans were also generated in addition to the VMAT treatment plans. Intentional shifting of the cranial field in the superior and then in the inferior directions was done, creating a gap or overlap between the fields. Consequent changes in dose distributions in these two plans to positional inaccuracies were studied. The 3D conformal radiotherapy plans showed large dose variations at the junction due to positional shifts as compared to the VMAT plans. With a 5mm superior shift of the cranial field isocentre creating a gap between the cranial and spinal fields, the magnitudes of under-dosing were 13.9±3.6Gy and 4.8±2.0Gy for 3D conformal radiotherapy and VMAT respectively. When the cranial field was moved by 5mm inferiorly creating an overlap between the fields, overdose to the effects of 10.3±4.0Gy and 4.9±1.3Gy were observed for the 3D conformal radiotherapy plans and VMAT plans respectively. The VMAT technique is insensitive to longitudinal setup errors (1-3mm) in patients because of the existence of low dose gradients at the junction between fields. This is unlike the 3D conformal radiotherapy plans which have steep dose gradients at the field edges and thus are highly sensitive to setup errors. Such an advantage for VMAT circumvents the need for dose feathering often practiced with the 3D conformal radiotherapy technique and makes the technique simpler to follow.
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Affiliation(s)
- B Sarkar
- Radiation oncology, Fortis Memorial Research Institute, 122002 Gurgaon, Haryana, India; Department of Physics, GLA University, Mathura, Uttar Pradesh, India.
| | - A Munshi
- Radiation oncology, Fortis Memorial Research Institute, 122002 Gurgaon, Haryana, India
| | - A Manikandan
- Radiation oncology, NRI Medical College and General Hospital, Guntur, Andhra Pradesh, India
| | - S Roy
- Radiation oncology, Fortis Memorial Research Institute, 122002 Gurgaon, Haryana, India
| | - T Ganesh
- Radiation oncology, Fortis Memorial Research Institute, 122002 Gurgaon, Haryana, India
| | - B K Mohanti
- Radiation oncology, Fortis Memorial Research Institute, 122002 Gurgaon, Haryana, India
| | - A Pradhan
- Department of mathematics, GLA University, Mathura, Uttar Pradesh, India
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Shukla P, Majumder B, Chatterjee P, Mitra K, Adhikary L, Sudeep K, Ghosh S, Chowdhury S, Chowdhury M, Sarkar B, Chakroborty S. Radial route coronary angiography without intra-arterial diltiazem: Single centre experience in eastern India. Indian Heart J 2017. [DOI: 10.1016/j.ihj.2017.09.140] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/26/2022] Open
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Shukla P, Majumder B, Sudeep K, Chatterjee P, Chakraborty S, Mitra K, Chowdhury S, Sarkar B, Adhikary L, Chowdhury M. Seasonal variation in pacemaker implantation: Our experience in a tertiary care hospital of Eastern India. Indian Heart J 2017. [DOI: 10.1016/j.ihj.2017.09.187] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/25/2022] Open
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Sudeep K, Majumder B, Mitra K, Chatterjee P, Shukla P, Chowdhury M, Chowdhury S, Ghosh S, Adhikary L, Sarkar B, Chakroborty S. A study of coronary anomaly pattern in eastern India: A single centre experience. Indian Heart J 2017. [DOI: 10.1016/j.ihj.2017.09.141] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/26/2022] Open
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Munshi A, Sarkar B, Roy S, Ganesh T, Mohanti B. PV-0135: Short tangential arcs in VMAT based breast and chest wall radiotherapy planning. Radiother Oncol 2017. [DOI: 10.1016/s0167-8140(17)30578-9] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/25/2022]
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Sarkar B, Manikandan A, Nandy M, Munshi A, Sayan P, Sujatha N. Influence of monte carlo variance with fluence smoothing in VMAT treatment planning with Monaco TPS. Indian J Cancer 2017; 53:158-61. [PMID: 27146769 DOI: 10.4103/0019-509x.180820] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/04/2022]
Abstract
INTRODUCTION The study aimed to investigate the interplay between Monte Carlo Variance (MCV) and fluence smoothing factor (FSF) in volumetric modulated arc therapy treatment planning by using a sample set of complex treatment planning cases and a X-ray Voxel Monte Carlo-based treatment planning system equipped with tools to tune fluence smoothness as well as MCV. MATERIALS AND METHODS The dosimetric (dose to tumor volume, and organ at risk) and physical characteristic (treatment time, number of segments, and so on) of a set 45 treatment plans for all combinations of 1%, 3%, 5% MCV and 1, 3, 5 FSF were evaluated for five carcinoma esophagus cases under the study. RESULT Increase in FSF reduce the treatment time. Variation of MCV and FSF gives a highest planning target volume (PTV), heart and lung dose variation of 3.6%, 12.8% and 4.3%, respectively. The heart dose variation was highest among all organs at risk. Highest variation of spinal cord dose was 0.6 Gy. CONCLUSION Variation of MCV and FSF influences the organ at risk (OAR) doses significantly but not PTV coverage and dose homogeneity. Variation in FSF causes difference in dosimetric and physical parameters for the treatment plans but variation of MCV does not. MCV 3% or less do not improve the plan quality significantly (physical and clinical) compared with MCV greater than 3%. The use of MCV between 3% and 5% gives similar results as 1% with lesser calculation time. Minimally detected differences in plan quality suggest that the optimum FSF can be set between 3 and 5.
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Affiliation(s)
- B Sarkar
- Department of Radiation Oncology, AMRI Hospitals, Kolkata, India
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Devi VG, Sircar A, Sarkar B. Application of Computational Fluid Dynamics for the Simulation of Cryogenic Molecular Sieve Bed Adsorber of Hydrogen Isotopes Recovery System for Indian LLCB-TBM. Fusion Science and Technology 2017. [DOI: 10.13182/fst14-t81] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/12/2022]
Affiliation(s)
- V. Gayathri Devi
- Institute for Plasma Research, Bhat, Gandhinagar, Gujarat 382 428, India
| | - Amit Sircar
- Institute for Plasma Research, Bhat, Gandhinagar, Gujarat 382 428, India
| | - B. Sarkar
- Institute for Plasma Research, Bhat, Gandhinagar, Gujarat 382 428, India
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Torane V, Kuyare S, Nataraj G, Mehta P, Dutta S, Sarkar B. Phenotypic and antibiogram pattern of V. cholerae isolates from a tertiary care hospital in Mumbai during 2004-2013: a retrospective cross-sectional study. BMJ Open 2016; 6:e012638. [PMID: 27888174 PMCID: PMC5168530 DOI: 10.1136/bmjopen-2016-012638] [Citation(s) in RCA: 9] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/03/2022] Open
Abstract
OBJECTIVES Cholera is a major gastroenteric disease with reports on fluctuation and resistance. Hence, the objective is to determine the trend in seasonality, resistance pattern, prevalent biotypes, serotypes and phage types between 2004 and 2013 among Vibrio cholerae isolates. DESIGN A retrospective cross-sectional study. SETTINGS A single-centre study was carried out at a tertiary care hospital in a metropolitan city (Mumbai) of a developing country (India). METHODS Records of stool specimen cultures of patients with suspected cholera from January 2004 to December 2013 were analysed. The organisms were identified as per standard protocol. Antimicrobial susceptibility testing was performed as per Clinical Laboratory Standard Institute. Biotyping, serotyping and phage typing were carried out. From the confirmed cases of cholera, demographic and laboratory details were noted. Descriptive analysis was used and the data were presented in the form of percentages. RESULTS Vibrio cholerae was predominant in males and was isolated from 9.41% (439/4664) of stool specimens. Variability was found in terms of the gross appearance of stool specimens, seasonal trend and antibiotic resistance pattern. The antimicrobial susceptibility showed a waxing and waning pattern for most of the antibiotics (ampicillin, cefuroxime, chloramphenicol, tetracycline) tested, while for a few others the strains were either uniformly sensitive (gentamicin, norfloxacin) or resistant (trimethoprim-sulfamethoxazole, nalidixic acid). All isolates belonged to subgroup O1 and biotype El Tor. The most common serotype was Ogawa. The predominant phage type was T2 (old scheme) and T27 (new scheme). CONCLUSIONS The predominant biotype, serotype and phage type were El Tor, Ogawa and T27 phage, respectively. The changing trends in antimicrobial resistance pattern over the years necessitate continued epidemiological and microbiological surveillance of the disease.
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Affiliation(s)
- V Torane
- Department of Microbiology, Seth G.S. Medical College & KEM Hospital, Mumbai, Maharashtra, India
| | - S Kuyare
- Department of Microbiology, Seth G.S. Medical College & KEM Hospital, Mumbai, Maharashtra, India
| | - G Nataraj
- Department of Microbiology, Seth G.S. Medical College & KEM Hospital, Mumbai, Maharashtra, India
| | - P Mehta
- Department of Microbiology, Seth G.S. Medical College & KEM Hospital, Mumbai, Maharashtra, India
| | - S Dutta
- Bacteriology Division, National Institute of Cholera and Enteric Diseases (NICED), Kolkata, West Bengal, India
| | - B Sarkar
- Bacteriology Division, National Institute of Cholera and Enteric Diseases (NICED), Kolkata, West Bengal, India
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Aab A, Abreu P, Aglietta M, Ahn EJ, Al Samarai I, Albuquerque IFM, Allekotte I, Allen JD, Allison P, Almela A, Alvarez Castillo J, Alvarez-Muñiz J, Ambrosio M, Anastasi GA, Anchordoqui L, Andrada B, Andringa S, Aramo C, Arqueros F, Arsene N, Asorey H, Assis P, Aublin J, Avila G, Badescu AM, Baus C, Beatty JJ, Becker KH, Bellido JA, Berat C, Bertaina ME, Bertou X, Biermann PL, Billoir P, Biteau J, Blaess SG, Blanco A, Blazek J, Bleve C, Blümer H, Boháčová M, Boncioli D, Bonifazi C, Borodai N, Botti AM, Brack J, Brancus I, Bretz T, Bridgeman A, Briechle FL, Buchholz P, Bueno A, Buitink S, Buscemi M, Caballero-Mora KS, Caccianiga B, Caccianiga L, Cancio A, Canfora F, Caramete L, Caruso R, Castellina A, Cataldi G, Cazon L, Cester R, Chavez AG, Chiavassa A, Chinellato JA, Chirinos Diaz JC, Chudoba J, Clay RW, Colalillo R, Coleman A, Collica L, Coluccia MR, Conceição R, Contreras F, Cooper MJ, Coutu S, Covault CE, Cronin J, Dallier R, D'Amico S, Daniel B, Dasso S, Daumiller K, Dawson BR, de Almeida RM, de Jong SJ, De Mauro G, de Mello Neto JRT, De Mitri I, de Oliveira J, de Souza V, Debatin J, Del Peral L, Deligny O, Dhital N, Di Giulio C, Di Matteo A, Díaz Castro ML, Diogo F, Dobrigkeit C, D'Olivo JC, Dorofeev A, Dos Anjos RC, Dova MT, Dundovic A, Ebr J, Engel R, Erdmann M, Erfani M, Escobar CO, Espadanal J, Etchegoyen A, Falcke H, Fang K, Farrar GR, Fauth AC, Fazzini N, Ferguson AP, Fick B, Figueira JM, Filevich A, Filipčič A, Fratu O, Freire MM, Fujii T, Fuster A, Gallo F, García B, Garcia-Pinto D, Gate F, Gemmeke H, Gherghel-Lascu A, Ghia PL, Giaccari U, Giammarchi M, Giller M, Głas D, Glaser C, Glass H, Golup G, Gómez Berisso M, Gómez Vitale PF, González N, Gookin B, Gordon J, Gorgi A, Gorham P, Gouffon P, Griffith N, Grillo AF, Grubb TD, Guarino F, Guedes GP, Hampel MR, Hansen P, Harari D, Harrison TA, Harton JL, Hasankiadeh Q, Haungs A, Hebbeker T, Heck D, Heimann P, Herve AE, Hill GC, Hojvat C, Hollon N, Holt E, Homola P, Hörandel JR, Horvath P, Hrabovský M, Huege T, Hulsman J, Insolia A, Isar PG, Jandt I, Jansen S, Jarne C, Johnsen JA, Josebachuili M, Kääpä A, Kambeitz O, Kampert KH, Kasper P, Katkov I, Keilhauer B, Kemp E, Kieckhafer RM, Klages HO, Kleifges M, Kleinfeller J, Krause R, Krohm N, Kuempel D, Kukec Mezek G, Kunka N, Kuotb Awad A, LaHurd D, Latronico L, Lauscher M, Lautridou P, Lebrun P, Legumina R, Leigui de Oliveira MA, Letessier-Selvon A, Lhenry-Yvon I, Link K, Lopes L, López R, López Casado A, Lucero A, Malacari M, Mallamaci M, Mandat D, Mantsch P, Mariazzi AG, Marin V, Mariş IC, Marsella G, Martello D, Martinez H, Martínez Bravo O, Masías Meza JJ, Mathes HJ, Mathys S, Matthews J, Matthews JAJ, Matthiae G, Maurizio D, Mayotte E, Mazur PO, Medina C, Medina-Tanco G, Mello VBB, Melo D, Menshikov A, Messina S, Micheletti MI, Middendorf L, Minaya IA, Miramonti L, Mitrica B, Molina-Bueno L, Mollerach S, Montanet F, Morello C, Mostafá M, Moura CA, Müller G, Muller MA, Müller S, Naranjo I, Navas S, Necesal P, Nellen L, Nelles A, Neuser J, Nguyen PH, Niculescu-Oglinzanu M, Niechciol M, Niemietz L, Niggemann T, Nitz D, Nosek D, Novotny V, Nožka H, Núñez LA, Ochilo L, Oikonomou F, Olinto A, Pakk Selmi-Dei D, Palatka M, Pallotta J, Papenbreer P, Parente G, Parra A, Paul T, Pech M, Pedreira F, Pękala J, Pelayo R, Peña-Rodriguez J, Pepe IM, Pereira LAS, Perrone L, Petermann E, Peters C, Petrera S, Phuntsok J, Piegaia R, Pierog T, Pieroni P, Pimenta M, Pirronello V, Platino M, Plum M, Porowski C, Prado RR, Privitera P, Prouza M, Quel EJ, Querchfeld S, Quinn S, Rautenberg J, Ravel O, Ravignani D, Revenu B, Ridky J, Risse M, Ristori P, Rizi V, Rodrigues de Carvalho W, Rodriguez Rojo J, Rodríguez-Frías MD, Rogozin D, Rosado J, Roth M, Roulet E, Rovero AC, Saffi SJ, Saftoiu A, Salazar H, Saleh A, Salesa Greus F, Salina G, Sanabria Gomez JD, Sánchez F, Sanchez-Lucas P, Santos EM, Santos E, Sarazin F, Sarkar B, Sarmento R, Sarmiento-Cano C, Sato R, Scarso C, Schauer M, Scherini V, Schieler H, Schmidt D, Scholten O, Schoorlemmer H, Schovánek P, Schröder FG, Schulz A, Schulz J, Schumacher J, Sciutto SJ, Segreto A, Settimo M, Shadkam A, Shellard RC, Sigl G, Sima O, Śmiałkowski A, Šmída R, Snow GR, Sommers P, Sonntag S, Sorokin J, Squartini R, Stanca D, Stanič S, Stapleton J, Stasielak J, Strafella F, Stutz A, Suarez F, Suarez Durán M, Sudholz T, Suomijärvi T, Supanitsky AD, Sutherland MS, Swain J, Szadkowski Z, Taborda OA, Tapia A, Tepe A, Theodoro VM, Timmermans C, Todero Peixoto CJ, Tomankova L, Tomé B, Tonachini A, Torralba Elipe G, Torres Machado D, Travnicek P, Trini M, Ulrich R, Unger M, Urban M, Valbuena-Delgado A, Valdés Galicia JF, Valiño I, Valore L, van Aar G, van Bodegom P, van den Berg AM, van Vliet A, Varela E, Vargas Cárdenas B, Varner G, Vázquez JR, Vázquez RA, Veberič D, Verzi V, Vicha J, Videla M, Villaseñor L, Vorobiov S, Wahlberg H, Wainberg O, Walz D, Watson AA, Weber M, Weindl A, Wiencke L, Wilczyński H, Winchen T, Wittkowski D, Wundheiler B, Wykes S, Yang L, Yapici T, Yelos D, Zas E, Zavrtanik D, Zavrtanik M, Zepeda A, Zimmermann B, Ziolkowski M, Zong Z, Zuccarello F. Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory. Phys Rev Lett 2016; 117:192001. [PMID: 27858429 DOI: 10.1103/physrevlett.117.192001] [Citation(s) in RCA: 35] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/23/2016] [Indexed: 06/06/2023]
Abstract
Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (E_{CM}=110-170 TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.
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Affiliation(s)
- A Aab
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - P Abreu
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - M Aglietta
- Osservatorio Astrofisico di Torino (INAF), Torino, Italy
- INFN, Sezione di Torino, Italy
| | - E J Ahn
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
| | - I Al Samarai
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, France
| | | | - I Allekotte
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | - J D Allen
- New York University, New York, New York, USA
| | - P Allison
- Ohio State University, Columbus, Ohio, USA
| | - A Almela
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Argentina
| | | | | | | | | | - L Anchordoqui
- Department of Physics and Astronomy, Lehman College, City University of New York, Bronx, New York, USA
| | - B Andrada
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - S Andringa
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - C Aramo
- INFN, Sezione di Napoli, Italy
| | - F Arqueros
- Universidad Complutense de Madrid, Spain
| | - N Arsene
- University of Bucharest, Physics Department, Romania
| | - H Asorey
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
- Universidad Industrial de Santander, Colombia
| | - P Assis
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - J Aublin
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, France
| | - G Avila
- Observatorio Pierre Auger, Argentina
- Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Argentina
| | - A M Badescu
- University Politehnica of Bucharest, Romania
| | - C Baus
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Germany
| | - J J Beatty
- Ohio State University, Columbus, Ohio, USA
| | - K H Becker
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | | | - C Berat
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, France
| | - M E Bertaina
- INFN, Sezione di Torino, Italy
- Università Torino, Dipartimento di Fisica, Italy
| | - X Bertou
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | - P L Biermann
- Max-Planck-Institut für Radioastronomie, Bonn, Germany
| | - P Billoir
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, France
| | - J Biteau
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, France
| | | | - A Blanco
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - J Blazek
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - C Bleve
- Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Italy
- INFN, Sezione di Lecce, Italy
| | - H Blümer
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Germany
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - M Boháčová
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - D Boncioli
- INFN Laboratori del Gran Sasso, Italy
- Universidade Federal do Rio de Janeiro (UFRJ), Instituto de Física, Brazil
| | - C Bonifazi
- Universidade Federal do Rio de Janeiro (UFRJ), Instituto de Física, Brazil
| | - N Borodai
- Institute of Nuclear Physics PAN, Poland
| | - A M Botti
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - J Brack
- Colorado State University, Fort Collins, Colorado, USA
| | - I Brancus
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Romania
| | - T Bretz
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - A Bridgeman
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - F L Briechle
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - P Buchholz
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - A Bueno
- Universidad de Granada and C.A.F.P.E., Spain
| | - S Buitink
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
| | - M Buscemi
- Università di Catania, Dipartimento di Fisica e Astronomia, Italy
- INFN, Sezione di Catania, Italy
| | | | | | - L Caccianiga
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, France
| | - A Cancio
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Argentina
| | - F Canfora
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
| | | | - R Caruso
- Università di Catania, Dipartimento di Fisica e Astronomia, Italy
- INFN, Sezione di Catania, Italy
| | - A Castellina
- Osservatorio Astrofisico di Torino (INAF), Torino, Italy
- INFN, Sezione di Torino, Italy
| | | | - L Cazon
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - R Cester
- INFN, Sezione di Torino, Italy
- Università Torino, Dipartimento di Fisica, Italy
| | - A G Chavez
- Universidad Michoacana de San Nicolás de Hidalgo, Mexico
| | - A Chiavassa
- INFN, Sezione di Torino, Italy
- Università Torino, Dipartimento di Fisica, Italy
| | | | | | - J Chudoba
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - R W Clay
- University of Adelaide, Australia
| | - R Colalillo
- INFN, Sezione di Napoli, Italy
- Università di Napoli "Federico II", Dipartimento di Fisica, Italy
| | - A Coleman
- Pennsylvania State University, University Park, Pennsylvania, USA
| | | | - M R Coluccia
- Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Italy
- INFN, Sezione di Lecce, Italy
| | - R Conceição
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - F Contreras
- Observatorio Pierre Auger, Argentina
- Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Argentina
| | | | - S Coutu
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - C E Covault
- Case Western Reserve University, Cleveland, Ohio, USA
| | - J Cronin
- University of Chicago, Chicago, Illinois, USA
| | - R Dallier
- SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, France
- Station de Radioastronomie de Nançay, France
| | - S D'Amico
- INFN, Sezione di Lecce, Italy
- Università del Salento, Dipartimento di Ingegneria, Italy
| | - B Daniel
- Universidade Estadual de Campinas (UNICAMP), Brazil
| | - S Dasso
- Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), Argentina
- Departamento de Física and Departamento de Ciencias de la Atmósfera y los Océanos, FCEyN, Universidad de Buenos Aires, Argentina
| | - K Daumiller
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | | | | | - S J de Jong
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
- Nationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Netherlands
| | - G De Mauro
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
| | | | - I De Mitri
- Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Italy
- INFN, Sezione di Lecce, Italy
| | | | - V de Souza
- Universidade de São Paulo, Inst. de Física de São Carlos, São Carlos, Brazil
| | - J Debatin
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | | | - O Deligny
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, France
| | - N Dhital
- Michigan Technological University, Houghton, Michigan, USA
| | - C Di Giulio
- Università di Roma "Tor Vergata", Dipartimento di Fisica, Italy
- INFN, Sezione di Roma "Tor Vergata", Italy
| | - A Di Matteo
- INFN, Sezione di L'Aquila, Italy
- Università dell'Aquila, Dipartimento di Chimica e Fisica, Italy
| | | | - F Diogo
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - C Dobrigkeit
- Universidade Estadual de Campinas (UNICAMP), Brazil
| | - J C D'Olivo
- Universidad Nacional Autónoma de México, Mexico
| | - A Dorofeev
- Colorado State University, Fort Collins, Colorado, USA
| | - R C Dos Anjos
- Universidade Federal do Paraná, Setor Palotina, Brazil
| | - M T Dova
- IFLP, Universidad Nacional de La Plata and CONICET, Argentina
| | - A Dundovic
- Universität Hamburg, II. Institut für Theoretische Physik, Germany
| | - J Ebr
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - R Engel
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - M Erdmann
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - M Erfani
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - C O Escobar
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
- Universidade Estadual de Campinas (UNICAMP), Brazil
| | - J Espadanal
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - A Etchegoyen
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Argentina
| | - H Falcke
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
- Nationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Netherlands
- Stichting Astronomisch Onderzoek in Nederland (ASTRON), Dwingeloo, Netherlands
| | - K Fang
- University of Chicago, Chicago, Illinois, USA
| | - G R Farrar
- New York University, New York, New York, USA
| | - A C Fauth
- Universidade Estadual de Campinas (UNICAMP), Brazil
| | - N Fazzini
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
| | - A P Ferguson
- Case Western Reserve University, Cleveland, Ohio, USA
| | - B Fick
- Michigan Technological University, Houghton, Michigan, USA
| | - J M Figueira
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - A Filevich
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - A Filipčič
- Experimental Particle Physics Department, J. Stefan Institute, Slovenia
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | - O Fratu
- University Politehnica of Bucharest, Romania
| | - M M Freire
- Instituto de Física de Rosario (IFIR)-CONICET/U.N.R. and Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Argentina
| | - T Fujii
- University of Chicago, Chicago, Illinois, USA
| | - A Fuster
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Argentina
| | - F Gallo
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - B García
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM) and Universidad Tecnológica Nacional-Facultad Regional Mendoza (CONICET/CNEA), Argentina
| | | | - F Gate
- SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, France
| | - H Gemmeke
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik (IPE), Germany
| | - A Gherghel-Lascu
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Romania
| | - P L Ghia
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, France
| | - U Giaccari
- Universidade Federal do Rio de Janeiro (UFRJ), Instituto de Física, Brazil
| | | | | | - D Głas
- University of Łódź, Poland
| | - C Glaser
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - H Glass
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
| | - G Golup
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | - M Gómez Berisso
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | - P F Gómez Vitale
- Observatorio Pierre Auger, Argentina
- Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Argentina
| | - N González
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - B Gookin
- Colorado State University, Fort Collins, Colorado, USA
| | - J Gordon
- Ohio State University, Columbus, Ohio, USA
| | - A Gorgi
- Osservatorio Astrofisico di Torino (INAF), Torino, Italy
- INFN, Sezione di Torino, Italy
| | - P Gorham
- University of Hawaii, Honolulu, Hawaii, USA
| | - P Gouffon
- Universidade de São Paulo, Inst. de Física, São Paulo, Brazil
| | - N Griffith
- Ohio State University, Columbus, Ohio, USA
| | | | | | - F Guarino
- INFN, Sezione di Napoli, Italy
- Università di Napoli "Federico II", Dipartimento di Fisica, Italy
| | - G P Guedes
- Universidade Estadual de Feira de Santana (UEFS), Brazil
| | - M R Hampel
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - P Hansen
- IFLP, Universidad Nacional de La Plata and CONICET, Argentina
| | - D Harari
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | | | - J L Harton
- Colorado State University, Fort Collins, Colorado, USA
| | - Q Hasankiadeh
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - A Haungs
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - T Hebbeker
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - D Heck
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - P Heimann
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - A E Herve
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Germany
| | - G C Hill
- University of Adelaide, Australia
| | - C Hojvat
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
| | - N Hollon
- University of Chicago, Chicago, Illinois, USA
| | - E Holt
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - P Homola
- Institute of Nuclear Physics PAN, Poland
| | - J R Hörandel
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
- Nationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Netherlands
| | - P Horvath
- Palacky University, RCPTM, Czech Republic
| | | | - T Huege
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - J Hulsman
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - A Insolia
- Università di Catania, Dipartimento di Fisica e Astronomia, Italy
- INFN, Sezione di Catania, Italy
| | - P G Isar
- Institute of Space Science, Romania
| | - I Jandt
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - S Jansen
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
- Nationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Netherlands
| | - C Jarne
- IFLP, Universidad Nacional de La Plata and CONICET, Argentina
| | - J A Johnsen
- Colorado School of Mines, Golden, Colorado, USA
| | - M Josebachuili
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - A Kääpä
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - O Kambeitz
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Germany
| | - K H Kampert
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - P Kasper
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
| | - I Katkov
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Germany
| | - B Keilhauer
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - E Kemp
- Universidade Estadual de Campinas (UNICAMP), Brazil
| | - R M Kieckhafer
- Michigan Technological University, Houghton, Michigan, USA
| | - H O Klages
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - M Kleifges
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik (IPE), Germany
| | | | - R Krause
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - N Krohm
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - D Kuempel
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - G Kukec Mezek
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | - N Kunka
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik (IPE), Germany
| | - A Kuotb Awad
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - D LaHurd
- Case Western Reserve University, Cleveland, Ohio, USA
| | | | - M Lauscher
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - P Lautridou
- SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, France
| | - P Lebrun
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
| | | | | | - A Letessier-Selvon
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, France
| | - I Lhenry-Yvon
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, France
| | - K Link
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Germany
| | - L Lopes
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - R López
- Benemérita Universidad Autónoma de Puebla (BUAP), Mexico
| | | | - A Lucero
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Argentina
| | | | - M Mallamaci
- INFN, Sezione di Milano, Italy
- Università di Milano, Dipartimento di Fisica, Italy
| | - D Mandat
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - P Mantsch
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
| | - A G Mariazzi
- IFLP, Universidad Nacional de La Plata and CONICET, Argentina
| | - V Marin
- SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, France
| | - I C Mariş
- Universidad de Granada and C.A.F.P.E., Spain
| | - G Marsella
- Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Italy
- INFN, Sezione di Lecce, Italy
| | - D Martello
- Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Italy
- INFN, Sezione di Lecce, Italy
| | - H Martinez
- Centro de Investigación y de Estudios Avanzados del IPN (CINVESTAV), Mexico
| | | | - J J Masías Meza
- Departamento de Física and Departamento de Ciencias de la Atmósfera y los Océanos, FCEyN, Universidad de Buenos Aires, Argentina
| | - H J Mathes
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - S Mathys
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - J Matthews
- Louisiana State University, Baton Rouge, Louisiana, USA
| | | | - G Matthiae
- Università di Roma "Tor Vergata", Dipartimento di Fisica, Italy
- INFN, Sezione di Roma "Tor Vergata", Italy
| | - D Maurizio
- Centro Brasileiro de Pesquisas Fisicas (CBPF), Brazil
| | - E Mayotte
- Colorado School of Mines, Golden, Colorado, USA
| | - P O Mazur
- Fermi National Accelerator Laboratory, Batavia, Illinois, USA
| | - C Medina
- Colorado School of Mines, Golden, Colorado, USA
| | | | - V B B Mello
- Universidade Federal do Rio de Janeiro (UFRJ), Instituto de Física, Brazil
| | - D Melo
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - A Menshikov
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik (IPE), Germany
| | - S Messina
- KVI-Center for Advanced Radiation Technology, University of Groningen, Netherlands
| | - M I Micheletti
- Instituto de Física de Rosario (IFIR)-CONICET/U.N.R. and Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Argentina
| | - L Middendorf
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - I A Minaya
- Universidad Complutense de Madrid, Spain
| | - L Miramonti
- INFN, Sezione di Milano, Italy
- Università di Milano, Dipartimento di Fisica, Italy
| | - B Mitrica
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Romania
| | | | - S Mollerach
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | - F Montanet
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, France
| | - C Morello
- Osservatorio Astrofisico di Torino (INAF), Torino, Italy
- INFN, Sezione di Torino, Italy
| | - M Mostafá
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - C A Moura
- Universidade Federal do ABC (UFABC), Brazil
| | - G Müller
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - M A Muller
- Universidade Estadual de Campinas (UNICAMP), Brazil
- Universidade Federal de Pelotas, Brazil
| | - S Müller
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - I Naranjo
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | - S Navas
- Universidad de Granada and C.A.F.P.E., Spain
| | - P Necesal
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - L Nellen
- Universidad Nacional Autónoma de México, Mexico
| | - A Nelles
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
- Nationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Netherlands
| | - J Neuser
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | | | | | - M Niechciol
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - L Niemietz
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - T Niggemann
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - D Nitz
- Michigan Technological University, Houghton, Michigan, USA
| | - D Nosek
- University Prague, Institute of Particle and Nuclear Physics, Czech Republic
| | - V Novotny
- University Prague, Institute of Particle and Nuclear Physics, Czech Republic
| | - H Nožka
- Palacky University, RCPTM, Czech Republic
| | - L A Núñez
- Universidad Industrial de Santander, Colombia
| | - L Ochilo
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - F Oikonomou
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - A Olinto
- University of Chicago, Chicago, Illinois, USA
| | | | - M Palatka
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - J Pallotta
- Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Argentina
| | - P Papenbreer
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - G Parente
- Universidad de Santiago de Compostela, Spain
| | - A Parra
- Benemérita Universidad Autónoma de Puebla (BUAP), Mexico
| | - T Paul
- Department of Physics and Astronomy, Lehman College, City University of New York, Bronx, New York, USA
- Northeastern University, Boston, Massachusetts, USA
| | - M Pech
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - F Pedreira
- Universidad de Santiago de Compostela, Spain
| | - J Pękala
- Institute of Nuclear Physics PAN, Poland
| | - R Pelayo
- Unidad Profesional Interdisciplinaria en Ingeniería y Tecnologías Avanzadas del Instituto Politécnico Nacional (UPIITA-IPN), Mexico
| | | | - I M Pepe
- Universidade Federal da Bahia, Brazil
| | | | - L Perrone
- Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Italy
- INFN, Sezione di Lecce, Italy
| | - E Petermann
- University of Nebraska, Lincoln, Nebraska, USA
| | - C Peters
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - S Petrera
- INFN, Sezione di L'Aquila, Italy
- Università dell'Aquila, Dipartimento di Chimica e Fisica, Italy
| | - J Phuntsok
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - R Piegaia
- Departamento de Física and Departamento de Ciencias de la Atmósfera y los Océanos, FCEyN, Universidad de Buenos Aires, Argentina
| | - T Pierog
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - P Pieroni
- Departamento de Física and Departamento de Ciencias de la Atmósfera y los Océanos, FCEyN, Universidad de Buenos Aires, Argentina
| | - M Pimenta
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - V Pirronello
- Università di Catania, Dipartimento di Fisica e Astronomia, Italy
- INFN, Sezione di Catania, Italy
| | - M Platino
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - M Plum
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - C Porowski
- Institute of Nuclear Physics PAN, Poland
| | - R R Prado
- Universidade de São Paulo, Inst. de Física de São Carlos, São Carlos, Brazil
| | - P Privitera
- University of Chicago, Chicago, Illinois, USA
| | - M Prouza
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - E J Quel
- Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Argentina
| | - S Querchfeld
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - S Quinn
- Case Western Reserve University, Cleveland, Ohio, USA
| | - J Rautenberg
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - O Ravel
- SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, France
| | - D Ravignani
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - B Revenu
- SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, France
| | - J Ridky
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - M Risse
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - P Ristori
- Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Argentina
| | - V Rizi
- INFN, Sezione di L'Aquila, Italy
- Università dell'Aquila, Dipartimento di Chimica e Fisica, Italy
| | | | | | | | - D Rogozin
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - J Rosado
- Universidad Complutense de Madrid, Spain
| | - M Roth
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - E Roulet
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | - A C Rovero
- Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), Argentina
| | | | - A Saftoiu
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Romania
| | - H Salazar
- Benemérita Universidad Autónoma de Puebla (BUAP), Mexico
| | - A Saleh
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | - F Salesa Greus
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - G Salina
- INFN, Sezione di Roma "Tor Vergata", Italy
| | | | - F Sánchez
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | | | - E M Santos
- Universidade de São Paulo, Inst. de Física, São Paulo, Brazil
| | - E Santos
- Universidade Estadual de Campinas (UNICAMP), Brazil
| | - F Sarazin
- Colorado School of Mines, Golden, Colorado, USA
| | - B Sarkar
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - R Sarmento
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | | | - R Sato
- Observatorio Pierre Auger, Argentina
| | - C Scarso
- Observatorio Pierre Auger, Argentina
| | - M Schauer
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - V Scherini
- Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Italy
- INFN, Sezione di Lecce, Italy
| | - H Schieler
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - D Schmidt
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - O Scholten
- KVI-Center for Advanced Radiation Technology, University of Groningen, Netherlands
| | | | - P Schovánek
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - F G Schröder
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - A Schulz
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - J Schulz
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
| | - J Schumacher
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - S J Sciutto
- IFLP, Universidad Nacional de La Plata and CONICET, Argentina
| | - A Segreto
- INFN, Sezione di Catania, Italy
- INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, Italy
| | - M Settimo
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, France
| | - A Shadkam
- Louisiana State University, Baton Rouge, Louisiana, USA
| | - R C Shellard
- Centro Brasileiro de Pesquisas Fisicas (CBPF), Brazil
| | - G Sigl
- Universität Hamburg, II. Institut für Theoretische Physik, Germany
| | - O Sima
- University of Bucharest, Physics Department, Romania
| | | | - R Šmída
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - G R Snow
- University of Nebraska, Lincoln, Nebraska, USA
| | - P Sommers
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - S Sonntag
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | | | | | - D Stanca
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Romania
| | - S Stanič
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | | | | | - F Strafella
- Università del Salento, Dipartimento di Matematica e Fisica "E. De Giorgi", Italy
- INFN, Sezione di Lecce, Italy
| | - A Stutz
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, France
| | - F Suarez
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Argentina
| | | | | | - T Suomijärvi
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, France
| | - A D Supanitsky
- Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), Argentina
| | | | - J Swain
- Northeastern University, Boston, Massachusetts, USA
| | | | - O A Taborda
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), Argentina
| | - A Tapia
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - A Tepe
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - V M Theodoro
- Universidade Estadual de Campinas (UNICAMP), Brazil
| | - C Timmermans
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
- Nationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Netherlands
| | | | - L Tomankova
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - B Tomé
- Laboratório de Instrumentação e Física Experimental de Partículas-LIP and Instituto Superior Técnico-IST, Universidade de Lisboa-UL, Portugal
| | - A Tonachini
- INFN, Sezione di Torino, Italy
- Università Torino, Dipartimento di Fisica, Italy
| | | | - D Torres Machado
- Universidade Federal do Rio de Janeiro (UFRJ), Instituto de Física, Brazil
| | - P Travnicek
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - M Trini
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | - R Ulrich
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - M Unger
- New York University, New York, New York, USA
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - M Urban
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | | | | | - I Valiño
- Universidad de Santiago de Compostela, Spain
| | - L Valore
- INFN, Sezione di Napoli, Italy
- Università di Napoli "Federico II", Dipartimento di Fisica, Italy
| | - G van Aar
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
| | | | - A M van den Berg
- KVI-Center for Advanced Radiation Technology, University of Groningen, Netherlands
| | - A van Vliet
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
| | - E Varela
- Benemérita Universidad Autónoma de Puebla (BUAP), Mexico
| | | | - G Varner
- University of Hawaii, Honolulu, Hawaii, USA
| | | | - R A Vázquez
- Universidad de Santiago de Compostela, Spain
| | - D Veberič
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - V Verzi
- INFN, Sezione di Roma "Tor Vergata", Italy
| | - J Vicha
- Institute of Physics (FZU) of the Academy of Sciences of the Czech Republic, Czech Republic
| | - M Videla
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - L Villaseñor
- Universidad Michoacana de San Nicolás de Hidalgo, Mexico
| | - S Vorobiov
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | - H Wahlberg
- IFLP, Universidad Nacional de La Plata and CONICET, Argentina
| | - O Wainberg
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Argentina
| | - D Walz
- RWTH Aachen University, III. Physikalisches Institut A, Germany
| | - A A Watson
- School of Physics and Astronomy, University of Leeds, Leeds, United Kingdom
| | - M Weber
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik (IPE), Germany
| | - A Weindl
- Karlsruhe Institute of Technology, Institut für Kernphysik (IKP), Germany
| | - L Wiencke
- Colorado School of Mines, Golden, Colorado, USA
| | | | - T Winchen
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - D Wittkowski
- Bergische Universität Wuppertal, Department of Physics, Germany, Germany
| | - B Wundheiler
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
| | - S Wykes
- Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen, Netherlands
| | - L Yang
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | - T Yapici
- Michigan Technological University, Houghton, Michigan, USA
| | - D Yelos
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica, Argentina
- Universidad Tecnológica Nacional-Facultad Regional Buenos Aires, Argentina
| | - E Zas
- Universidad de Santiago de Compostela, Spain
| | - D Zavrtanik
- Experimental Particle Physics Department, J. Stefan Institute, Slovenia
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | - M Zavrtanik
- Experimental Particle Physics Department, J. Stefan Institute, Slovenia
- Laboratory for Astroparticle Physics, University of Nova Gorica, Slovenia
| | - A Zepeda
- Centro de Investigación y de Estudios Avanzados del IPN (CINVESTAV), Mexico
| | - B Zimmermann
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik (IPE), Germany
| | - M Ziolkowski
- Universität Siegen, Fachbereich 7 Physik-Experimentelle Teilchenphysik, Germany
| | - Z Zong
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, France
| | - F Zuccarello
- Università di Catania, Dipartimento di Fisica e Astronomia, Italy
- INFN, Sezione di Catania, Italy
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Sinha R, Maji B, Sarkar B, Meur S. A prospective audit of complications in 100 consecutive pediatric percutaneous renal biopsies done under real-time ultrasound guidance. Indian J Nephrol 2016; 26:329-334. [PMID: 27795625 PMCID: PMC5015509 DOI: 10.4103/0971-4065.171232] [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] [Key Words] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/05/2022] Open
Abstract
Despite being a common procedure, percutaneous renal biopsy (PRB) carries the potential for complications. The British Association of Paediatric Nephrologist (BAPN) has published standards for pediatric PRB. As Indian data are scarce, we conducted a prospective audit of 100 consecutive pediatric renal biopsies (60% males) under real-time ultrasound guidance. Nephrotic syndrome was the most common indication for PRB (68%) with minimal change disease (30%) and focal segmental glomerulosclerosis (25%) being the most common histopathological lesions. Gross hematuria was observed in six cases. Major complications was noted in one case, who needed longer hospital stay. The result of the audit demonstrated achievability of BAPN standards. In addition, we also show the usefulness of 16 gauge biopsy needle over 18 gauge biopsy needles (median number of glomeruli 25, range 3–90 vs 13, range 6–46, P = 0.001) without any increase in complications. Being a single center study, we do hope that our results will encourage a wider survey on the current state of pediatric PRB.
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Affiliation(s)
- R Sinha
- Division of Paediatric Nephrology, Institute of Child Health, Vision Care Hospital (AMRI Hospitals), Kolkata, West Bengal, India; Division of Paediatric Nephrology, Vision Care Hospital (AMRI Hospitals), Kolkata, West Bengal, India
| | - B Maji
- Division of Paediatric Nephrology, Institute of Child Health, Vision Care Hospital (AMRI Hospitals), Kolkata, West Bengal, India
| | - B Sarkar
- Paediatric Intensive Care, Vision Care Hospital (AMRI Hospitals), Kolkata, West Bengal, India
| | - S Meur
- Paediatric Intensive Care, Vision Care Hospital (AMRI Hospitals), Kolkata, West Bengal, India
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Aab A, Abreu P, Aglietta M, Ahn EJ, Al Samarai I, Albuquerque IFM, Allekotte I, Allison P, Almela A, Alvarez Castillo J, Alvarez-Muñiz J, Alves Batista R, Ambrosio M, Aminaei A, Anastasi GA, Anchordoqui L, Andringa S, Aramo C, Arqueros F, Arsene N, Asorey H, Assis P, Aublin J, Avila G, Awal N, Badescu AM, Baus C, Beatty JJ, Becker KH, Bellido JA, Berat C, Bertaina ME, Bertou X, Biermann PL, Billoir P, Blaess SG, Blanco A, Blanco M, Blazek J, Bleve C, Blümer H, Boháčová M, Boncioli D, Bonifazi C, Borodai N, Brack J, Brancus I, Bretz T, Bridgeman A, Brogueira P, Buchholz P, Bueno A, Buitink S, Buscemi M, Caballero-Mora KS, Caccianiga B, Caccianiga L, Candusso M, Caramete L, Caruso R, Castellina A, Cataldi G, Cazon L, Cester R, Chavez AG, Chiavassa A, Chinellato JA, Chudoba J, Cilmo M, Clay RW, Cocciolo G, Colalillo R, Coleman A, Collica L, Coluccia MR, Conceição R, Contreras F, Cooper MJ, Cordier A, Coutu S, Covault CE, Cronin J, Dallier R, Daniel B, Dasso S, Daumiller K, Dawson BR, de Almeida RM, de Jong SJ, De Mauro G, de Mello Neto JRT, De Mitri I, de Oliveira J, de Souza V, Del Peral L, Deligny O, Dhital N, Di Giulio C, Di Matteo A, Diaz JC, Díaz Castro ML, Diogo F, Dobrigkeit C, Docters W, D'Olivo JC, Dorofeev A, Dorosti Hasankiadeh Q, Dos Anjos RC, Dova MT, Ebr J, Engel R, Erdmann M, Erfani M, Escobar CO, Espadanal J, Etchegoyen A, Falcke H, Fang K, Farrar G, Fauth AC, Fazzini N, Ferguson AP, Fick B, Figueira JM, Filevich A, Filipčič A, Fratu O, Freire MM, Fujii T, García B, Garcia-Gamez D, Garcia-Pinto D, Gate F, Gemmeke H, Gherghel-Lascu A, Ghia PL, Giaccari U, Giammarchi M, Giller M, Głas D, Glaser C, Glass H, Golup G, Gómez Berisso M, Gómez Vitale PF, González N, Gookin B, Gordon J, Gorgi A, Gorham P, Gouffon P, Griffith N, Grillo AF, Grubb TD, Guarino F, Guedes GP, Hampel MR, Hansen P, Harari D, Harrison TA, Hartmann S, Harton JL, Haungs A, Hebbeker T, Heck D, Heimann P, Herve AE, Hill GC, Hojvat C, Hollon N, Holt E, Homola P, Hörandel JR, Horvath P, Hrabovský M, Huber D, Huege T, Insolia A, Isar PG, Jandt I, Jansen S, Jarne C, Johnsen JA, Josebachuili M, Kääpä A, Kambeitz O, Kampert KH, Kasper P, Katkov I, Keilhauer B, Kemp E, Kieckhafer RM, Klages HO, Kleifges M, Kleinfeller J, Krause R, Krohm N, Kuempel D, Kukec Mezek G, Kunka N, Kuotb Awad AW, LaHurd D, Latronico L, Lauer R, Lauscher M, Lautridou P, Le Coz S, Lebrun D, Lebrun P, Leigui de Oliveira MA, Letessier-Selvon A, Lhenry-Yvon I, Link K, Lopes L, López R, López Casado A, Louedec K, Lucero A, Malacari M, Mallamaci M, Maller J, Mandat D, Mantsch P, Mariazzi AG, Marin V, Mariş IC, Marsella G, Martello D, Martinez H, Martínez Bravo O, Martraire D, Masías Meza JJ, Mathes HJ, Mathys S, Matthews J, Matthews JAJ, Matthiae G, Maurizio D, Mayotte E, Mazur PO, Medina C, Medina-Tanco G, Meissner R, Mello VBB, Melo D, Menshikov A, Messina S, Micheletti MI, Middendorf L, Minaya IA, Miramonti L, Mitrica B, Molina-Bueno L, Mollerach S, Montanet F, Morello C, Mostafá M, Moura CA, Muller MA, Müller G, Müller S, Navas S, Necesal P, Nellen L, Nelles A, Neuser J, Nguyen PH, Niculescu-Oglinzanu M, Niechciol M, Niemietz L, Niggemann T, Nitz D, Nosek D, Novotny V, Nožka L, Núñez LA, Ochilo L, Oikonomou F, Olinto A, Pacheco N, Pakk Selmi-Dei D, Palatka M, Pallotta J, Papenbreer P, Parente G, Parra A, Paul T, Pech M, Pȩkala J, Pelayo R, Pepe IM, Perrone L, Petermann E, Peters C, Petrera S, Petrov Y, Phuntsok J, Piegaia R, Pierog T, Pieroni P, Pimenta M, Pirronello V, Platino M, Plum M, Porcelli A, Porowski C, Prado RR, Privitera P, Prouza M, Quel EJ, Querchfeld S, Quinn S, Rautenberg J, Ravel O, Ravignani D, Reinert D, Revenu B, Ridky J, Risse M, Ristori P, Rizi V, Rodrigues de Carvalho W, Rodriguez Rojo J, Rodríguez-Frías MD, Rogozin D, Rosado J, Roth M, Roulet E, Rovero AC, Saffi SJ, Saftoiu A, Salazar H, Saleh A, Salesa Greus F, Salina G, Sanabria Gomez JD, Sánchez F, Sanchez-Lucas P, Santos E, Santos EM, Sarazin F, Sarkar B, Sarmento R, Sarmiento-Cano C, Sato R, Scarso C, Schauer M, Scherini V, Schieler H, Schmidt D, Scholten O, Schoorlemmer H, Schovánek P, Schröder FG, Schulz A, Schulz J, Schumacher J, Sciutto SJ, Segreto A, Settimo M, Shadkam A, Shellard RC, Sigl G, Sima O, Śmiałkowski A, Šmída R, Snow GR, Sommers P, Sonntag S, Sorokin J, Squartini R, Srivastava YN, Stanca D, Stanič S, Stapleton J, Stasielak J, Stephan M, Stutz A, Suarez F, Suarez Durán M, Suomijärvi T, Supanitsky AD, Sutherland MS, Swain J, Szadkowski Z, Taborda OA, Tapia A, Tepe A, Theodoro VM, Timmermans C, Todero Peixoto CJ, Toma G, Tomankova L, Tomé B, Tonachini A, Torralba Elipe G, Torres Machado D, Travnicek P, Trini M, Ulrich R, Unger M, Urban M, Valdés Galicia JF, Valiño I, Valore L, van Aar G, van Bodegom P, van den Berg AM, van Velzen S, van Vliet A, Varela E, Vargas Cárdenas B, Varner G, Vasquez R, Vázquez JR, Vázquez RA, Veberič D, Verzi V, Vicha J, Videla M, Villaseñor L, Vlcek B, Vorobiov S, Wahlberg H, Wainberg O, Walz D, Watson AA, Weber M, Weidenhaupt K, Weindl A, Welling C, Werner F, Widom A, Wiencke L, Wilczyński H, Winchen T, Wittkowski D, Wundheiler B, Wykes S, Yang L, Yapici T, Yushkov A, Zas E, Zavrtanik D, Zavrtanik M, Zepeda A, Zimmermann B, Ziolkowski M, Zuccarello F. Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy. Phys Rev Lett 2016; 116:241101. [PMID: 27367377 DOI: 10.1103/physrevlett.116.241101] [Citation(s) in RCA: 27] [Impact Index Per Article: 3.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/27/2015] [Indexed: 06/06/2023]
Abstract
We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.
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Affiliation(s)
- A Aab
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - P Abreu
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - M Aglietta
- Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - E J Ahn
- Fermilab, Batavia, Illinois, USA
| | - I Al Samarai
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - I F M Albuquerque
- Universidade de São Paulo, Instituto de Física, São Paulo, São Paulo, Brazil
| | - I Allekotte
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - P Allison
- Ohio State University, Columbus, Ohio, USA
| | - A Almela
- Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - J Alvarez Castillo
- Universidad Nacional Autónoma de México, México, Distrito Federal, Mexico
| | - J Alvarez-Muñiz
- Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - R Alves Batista
- Universität Hamburg, II. Institut für Theoretische Physik, Hamburg, Germany
| | - M Ambrosio
- Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy
| | - A Aminaei
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - G A Anastasi
- Università di Catania and Sezione INFN, Catania, Italy
| | - L Anchordoqui
- Department of Physics and Astronomy, Lehman College, City University of New York, Bronx, New York, USA
| | - S Andringa
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - C Aramo
- Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy
| | - F Arqueros
- Universidad Complutense de Madrid, Madrid, Spain
| | - N Arsene
- University of Bucharest, Physics Department, Bucharest, Romania
| | - H Asorey
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
- Universidad Industrial de Santander, Bucaramanga, Colombia
| | - P Assis
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - J Aublin
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - G Avila
- Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina
| | - N Awal
- New York University, New York, New York, USA
| | - A M Badescu
- University Politehnica of Bucharest, Bucharest, Romania
| | - C Baus
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
| | - J J Beatty
- Ohio State University, Columbus, Ohio, USA
| | - K H Becker
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - J A Bellido
- University of Adelaide, Adelaide, South Australia, Australia
| | - C Berat
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - M E Bertaina
- Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - X Bertou
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - P L Biermann
- Max-Planck-Institut für Radioastronomie, Bonn, Germany
| | - P Billoir
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - S G Blaess
- University of Adelaide, Adelaide, South Australia, Australia
| | - A Blanco
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - M Blanco
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - J Blazek
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - C Bleve
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - H Blümer
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - M Boháčová
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - D Boncioli
- INFN, Laboratori Nazionali del Gran Sasso, Assergi (L'Aquila), Italy
| | - C Bonifazi
- Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro, Rio de Janeiro, Brazil
| | - N Borodai
- Institute of Nuclear Physics PAN, Krakow, Poland
| | - J Brack
- Colorado State University, Fort Collins, Colorado, USA
| | - I Brancus
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - T Bretz
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A Bridgeman
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - P Brogueira
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - P Buchholz
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - A Bueno
- Universidad de Granada and C.A.F.P.E., Granada, Spain
| | - S Buitink
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - M Buscemi
- Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy
| | | | - B Caccianiga
- Università di Milano and Sezione INFN, Milan, Italy
| | - L Caccianiga
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - M Candusso
- Università di Roma II "Tor Vergata" and Sezione INFN, Roma, Italy
| | - L Caramete
- Institute of Space Science, Bucharest-Magurele, Romania
| | - R Caruso
- Università di Catania and Sezione INFN, Catania, Italy
| | - A Castellina
- Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - G Cataldi
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - L Cazon
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - R Cester
- Università di Torino and Sezione INFN, Torino, Italy
| | - A G Chavez
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Michoacán, Mexico
| | - A Chiavassa
- Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - J A Chinellato
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - J Chudoba
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - M Cilmo
- Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy
| | - R W Clay
- University of Adelaide, Adelaide, South Australia, Australia
| | - G Cocciolo
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - R Colalillo
- Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy
| | - A Coleman
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - L Collica
- Università di Milano and Sezione INFN, Milan, Italy
| | - M R Coluccia
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - R Conceição
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - F Contreras
- Observatorio Pierre Auger, Malargüe, Argentina
| | - M J Cooper
- University of Adelaide, Adelaide, South Australia, Australia
| | - A Cordier
- Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - S Coutu
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - C E Covault
- Case Western Reserve University, Cleveland, Ohio, USA
| | - J Cronin
- University of Chicago, Enrico Fermi Institute, Chicago, Illinois, USA
| | - R Dallier
- SUBATECH, école des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
- Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, Nançay, France
| | - B Daniel
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - S Dasso
- Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), Buenos Aires, Argentina
- Departamento de Física, FCEyN, Universidad de Buenos Aires and CONICET, Buenos Aires, Argentina
| | - K Daumiller
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - B R Dawson
- University of Adelaide, Adelaide, South Australia, Australia
| | - R M de Almeida
- Universidade Federal Fluminense, EEIMVR, Volta Redonda, Rio de Janeiro, Brazil
| | - S J de Jong
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- Nikhef, Science Park, Amsterdam, Netherlands
| | - G De Mauro
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - J R T de Mello Neto
- Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro, Rio de Janeiro, Brazil
| | - I De Mitri
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - J de Oliveira
- Universidade Federal Fluminense, EEIMVR, Volta Redonda, Rio de Janeiro, Brazil
| | - V de Souza
- Universidade de São Paulo, Instituto de Física de São Carlos, São Carlos, São Paulo, Brazil
| | - L Del Peral
- Universidad de Alcalá, Alcalá de Henares, Madrid, Spain
| | - O Deligny
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - N Dhital
- Michigan Technological University, Houghton, Michigan, USA
| | - C Di Giulio
- Università di Roma II "Tor Vergata" and Sezione INFN, Roma, Italy
| | - A Di Matteo
- Dipartimento di Scienze Fisiche e Chimiche dell'Università dell'Aquila and INFN, L'Aquila, Italy
| | - J C Diaz
- Michigan Technological University, Houghton, Michigan, USA
| | - M L Díaz Castro
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - F Diogo
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - C Dobrigkeit
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - W Docters
- KVI - Center for Advanced Radiation Technology, University of Groningen, Groningen, Netherlands
| | - J C D'Olivo
- Universidad Nacional Autónoma de México, México, Distrito Federal, Mexico
| | - A Dorofeev
- Colorado State University, Fort Collins, Colorado, USA
| | | | - R C Dos Anjos
- Universidade de São Paulo, Instituto de Física de São Carlos, São Carlos, São Paulo, Brazil
| | - M T Dova
- IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - J Ebr
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - R Engel
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - M Erdmann
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - M Erfani
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - C O Escobar
- Fermilab, Batavia, Illinois, USA
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - J Espadanal
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - A Etchegoyen
- Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - H Falcke
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- Nikhef, Science Park, Amsterdam, Netherlands
- ASTRON, Dwingeloo, Netherlands
| | - K Fang
- University of Chicago, Enrico Fermi Institute, Chicago, Illinois, USA
| | - G Farrar
- New York University, New York, New York, USA
| | - A C Fauth
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | | | - A P Ferguson
- Case Western Reserve University, Cleveland, Ohio, USA
| | - B Fick
- Michigan Technological University, Houghton, Michigan, USA
| | - J M Figueira
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A Filevich
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A Filipčič
- Experimental Particle Physics Department, J. Stefan Institute, Ljubljana, Slovenia
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - O Fratu
- University Politehnica of Bucharest, Bucharest, Romania
| | - M M Freire
- Instituto de Física de Rosario (IFIR) - CONICET/U.N.R. and Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Rosario, Argentina
| | - T Fujii
- University of Chicago, Enrico Fermi Institute, Chicago, Illinois, USA
| | - B García
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), and Universidad Tecnológica Nacional - Facultad Regional Mendoza (CONICET/CNEA), Mendoza, Argentina
| | - D Garcia-Gamez
- Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, France
| | | | - F Gate
- SUBATECH, école des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - H Gemmeke
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - A Gherghel-Lascu
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - P L Ghia
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - U Giaccari
- Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro, Rio de Janeiro, Brazil
| | - M Giammarchi
- Università di Milano and Sezione INFN, Milan, Italy
| | - M Giller
- University of Łódź, Łódź, Poland
| | - D Głas
- University of Łódź, Łódź, Poland
| | - C Glaser
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - H Glass
- Fermilab, Batavia, Illinois, USA
| | - G Golup
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - M Gómez Berisso
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - P F Gómez Vitale
- Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina
| | - N González
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - B Gookin
- Colorado State University, Fort Collins, Colorado, USA
| | - J Gordon
- Ohio State University, Columbus, Ohio, USA
| | - A Gorgi
- Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - P Gorham
- University of Hawaii, Honolulu, Hawaii, USA
| | - P Gouffon
- Universidade de São Paulo, Instituto de Física, São Paulo, São Paulo, Brazil
| | - N Griffith
- Ohio State University, Columbus, Ohio, USA
| | - A F Grillo
- INFN, Laboratori Nazionali del Gran Sasso, Assergi (L'Aquila), Italy
| | - T D Grubb
- University of Adelaide, Adelaide, South Australia, Australia
| | - F Guarino
- Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy
| | - G P Guedes
- Universidade Estadual de Feira de Santana, Feira de Santana, Brazil
| | - M R Hampel
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - P Hansen
- IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - D Harari
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - T A Harrison
- University of Adelaide, Adelaide, South Australia, Australia
| | - S Hartmann
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - J L Harton
- Colorado State University, Fort Collins, Colorado, USA
| | - A Haungs
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - T Hebbeker
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - D Heck
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - P Heimann
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - A E Herve
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - G C Hill
- University of Adelaide, Adelaide, South Australia, Australia
| | - C Hojvat
- Fermilab, Batavia, Illinois, USA
| | - N Hollon
- University of Chicago, Enrico Fermi Institute, Chicago, Illinois, USA
| | - E Holt
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - P Homola
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - J R Hörandel
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- Nikhef, Science Park, Amsterdam, Netherlands
| | - P Horvath
- Palacky University, RCPTM, Olomouc, Czech Republic
| | - M Hrabovský
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
- Palacky University, RCPTM, Olomouc, Czech Republic
| | - D Huber
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
| | - T Huege
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - A Insolia
- Università di Catania and Sezione INFN, Catania, Italy
| | - P G Isar
- Institute of Space Science, Bucharest-Magurele, Romania
| | - I Jandt
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - S Jansen
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- Nikhef, Science Park, Amsterdam, Netherlands
| | - C Jarne
- IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - J A Johnsen
- Colorado School of Mines, Golden, Colorado, USA
| | - M Josebachuili
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A Kääpä
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - O Kambeitz
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
| | - K H Kampert
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - P Kasper
- Fermilab, Batavia, Illinois, USA
| | - I Katkov
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
| | - B Keilhauer
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - E Kemp
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - R M Kieckhafer
- Michigan Technological University, Houghton, Michigan, USA
| | - H O Klages
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - M Kleifges
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | | | - R Krause
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - N Krohm
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - D Kuempel
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - G Kukec Mezek
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - N Kunka
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - A W Kuotb Awad
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - D LaHurd
- Case Western Reserve University, Cleveland, Ohio, USA
| | - L Latronico
- Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - R Lauer
- University of New Mexico, Albuquerque, New Mexico, USA
| | - M Lauscher
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - P Lautridou
- SUBATECH, école des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - S Le Coz
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - D Lebrun
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - P Lebrun
- Fermilab, Batavia, Illinois, USA
| | | | - A Letessier-Selvon
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - I Lhenry-Yvon
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - K Link
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
| | - L Lopes
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - R López
- Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - A López Casado
- Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - K Louedec
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - A Lucero
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - M Malacari
- University of Adelaide, Adelaide, South Australia, Australia
| | - M Mallamaci
- Università di Milano and Sezione INFN, Milan, Italy
| | - J Maller
- SUBATECH, école des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - D Mandat
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | | | - A G Mariazzi
- IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - V Marin
- SUBATECH, école des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - I C Mariş
- Universidad de Granada and C.A.F.P.E., Granada, Spain
| | - G Marsella
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - D Martello
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - H Martinez
- Centro de Investigación y de Estudios Avanzados del IPN (CINVESTAV), México, Distrito Federal, Mexico
| | | | - D Martraire
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - J J Masías Meza
- Departamento de Física, FCEyN, Universidad de Buenos Aires and CONICET, Buenos Aires, Argentina
| | - H J Mathes
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - S Mathys
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - J Matthews
- Louisiana State University, Baton Rouge, Louisiana, USA
| | | | - G Matthiae
- Università di Roma II "Tor Vergata" and Sezione INFN, Roma, Italy
| | - D Maurizio
- Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, Rio de Janeiro, Brazil
| | - E Mayotte
- Colorado School of Mines, Golden, Colorado, USA
| | | | - C Medina
- Colorado School of Mines, Golden, Colorado, USA
| | - G Medina-Tanco
- Universidad Nacional Autónoma de México, México, Distrito Federal, Mexico
| | - R Meissner
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - V B B Mello
- Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro, Rio de Janeiro, Brazil
| | - D Melo
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A Menshikov
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - S Messina
- KVI - Center for Advanced Radiation Technology, University of Groningen, Groningen, Netherlands
| | - M I Micheletti
- Instituto de Física de Rosario (IFIR) - CONICET/U.N.R. and Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Rosario, Argentina
| | - L Middendorf
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - I A Minaya
- Universidad Complutense de Madrid, Madrid, Spain
| | - L Miramonti
- Università di Milano and Sezione INFN, Milan, Italy
| | - B Mitrica
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | | | - S Mollerach
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - F Montanet
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - C Morello
- Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - M Mostafá
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - C A Moura
- Universidade Federal do ABC, Santo André, São Paulo, Brazil
| | - M A Muller
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
- Universidade Federal de Pelotas, Pelotas, Rio Grande do Sul, Brazil
| | - G Müller
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - S Müller
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - S Navas
- Universidad de Granada and C.A.F.P.E., Granada, Spain
| | - P Necesal
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - L Nellen
- Universidad Nacional Autónoma de México, México, Distrito Federal, Mexico
| | - A Nelles
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- Nikhef, Science Park, Amsterdam, Netherlands
| | - J Neuser
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - P H Nguyen
- University of Adelaide, Adelaide, South Australia, Australia
| | - M Niculescu-Oglinzanu
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - M Niechciol
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - L Niemietz
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - T Niggemann
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - D Nitz
- Michigan Technological University, Houghton, Michigan, USA
| | - D Nosek
- Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Prague, Czech Republic
| | - V Novotny
- Charles University, Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Prague, Czech Republic
| | - L Nožka
- Palacky University, RCPTM, Olomouc, Czech Republic
| | - L A Núñez
- Universidad Industrial de Santander, Bucaramanga, Colombia
| | - L Ochilo
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - F Oikonomou
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - A Olinto
- University of Chicago, Enrico Fermi Institute, Chicago, Illinois, USA
| | - N Pacheco
- Universidad de Alcalá, Alcalá de Henares, Madrid, Spain
| | - D Pakk Selmi-Dei
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - M Palatka
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - J Pallotta
- Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Villa Martelli, Argentina
| | - P Papenbreer
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - G Parente
- Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - A Parra
- Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - T Paul
- Department of Physics and Astronomy, Lehman College, City University of New York, Bronx, New York, USA
- Northeastern University, Boston, Massachusetts, USA
| | - M Pech
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - J Pȩkala
- Institute of Nuclear Physics PAN, Krakow, Poland
| | - R Pelayo
- Unidad Profesional Interdisciplinaria en Ingeniería y Tecnologías Avanzadas del Instituto Politécnico Nacional (UPIITA- IPN), México, Distrito Federal, Mexico
| | - I M Pepe
- Universidade Federal da Bahia, Salvador, BA, Brazil
| | - L Perrone
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - E Petermann
- University of Nebraska, Lincoln, Nebraska, USA
| | - C Peters
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - S Petrera
- Dipartimento di Scienze Fisiche e Chimiche dell'Università dell'Aquila and INFN, L'Aquila, Italy
- Gran Sasso Science Institute (INFN), L'Aquila, Italy
| | - Y Petrov
- Colorado State University, Fort Collins, Colorado, USA
| | - J Phuntsok
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - R Piegaia
- Departamento de Física, FCEyN, Universidad de Buenos Aires and CONICET, Buenos Aires, Argentina
| | - T Pierog
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - P Pieroni
- Departamento de Física, FCEyN, Universidad de Buenos Aires and CONICET, Buenos Aires, Argentina
| | - M Pimenta
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - V Pirronello
- Università di Catania and Sezione INFN, Catania, Italy
| | - M Platino
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - M Plum
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A Porcelli
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - C Porowski
- Institute of Nuclear Physics PAN, Krakow, Poland
| | - R R Prado
- Universidade de São Paulo, Instituto de Física de São Carlos, São Carlos, São Paulo, Brazil
| | - P Privitera
- University of Chicago, Enrico Fermi Institute, Chicago, Illinois, USA
| | - M Prouza
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - E J Quel
- Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Villa Martelli, Argentina
| | - S Querchfeld
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - S Quinn
- Case Western Reserve University, Cleveland, Ohio, USA
| | - J Rautenberg
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - O Ravel
- SUBATECH, école des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - D Ravignani
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - D Reinert
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - B Revenu
- SUBATECH, école des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - J Ridky
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - M Risse
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - P Ristori
- Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Villa Martelli, Argentina
| | - V Rizi
- Dipartimento di Scienze Fisiche e Chimiche dell'Università dell'Aquila and INFN, L'Aquila, Italy
| | | | | | | | - D Rogozin
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - J Rosado
- Universidad Complutense de Madrid, Madrid, Spain
| | - M Roth
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - E Roulet
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - A C Rovero
- Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), Buenos Aires, Argentina
| | - S J Saffi
- University of Adelaide, Adelaide, South Australia, Australia
| | - A Saftoiu
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - H Salazar
- Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - A Saleh
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - F Salesa Greus
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - G Salina
- Università di Roma II "Tor Vergata" and Sezione INFN, Roma, Italy
| | | | - F Sánchez
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | | | - E Santos
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - E M Santos
- Universidade de São Paulo, Instituto de Física, São Paulo, São Paulo, Brazil
| | - F Sarazin
- Colorado School of Mines, Golden, Colorado, USA
| | - B Sarkar
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - R Sarmento
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | | | - R Sato
- Observatorio Pierre Auger, Malargüe, Argentina
| | - C Scarso
- Observatorio Pierre Auger, Malargüe, Argentina
| | - M Schauer
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - V Scherini
- Dipartimento di Matematica e Fisica "E. De Giorgi" dell'Università del Salento and Sezione INFN, Lecce, Italy
| | - H Schieler
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - D Schmidt
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - O Scholten
- KVI - Center for Advanced Radiation Technology, University of Groningen, Groningen, Netherlands
- Vrije Universiteit Brussel, Brussels, Belgium
| | | | - P Schovánek
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - F G Schröder
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - A Schulz
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - J Schulz
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - J Schumacher
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - S J Sciutto
- IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - A Segreto
- Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy
| | - M Settimo
- Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - A Shadkam
- Louisiana State University, Baton Rouge, Louisiana, USA
| | - R C Shellard
- Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, Rio de Janeiro, Brazil
| | - G Sigl
- Universität Hamburg, II. Institut für Theoretische Physik, Hamburg, Germany
| | - O Sima
- University of Bucharest, Physics Department, Bucharest, Romania
| | | | - R Šmída
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - G R Snow
- University of Nebraska, Lincoln, Nebraska, USA
| | - P Sommers
- Pennsylvania State University, University Park, Pennsylvania, USA
| | - S Sonntag
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - J Sorokin
- University of Adelaide, Adelaide, South Australia, Australia
| | - R Squartini
- Observatorio Pierre Auger, Malargüe, Argentina
| | | | - D Stanca
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - S Stanič
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | | | - J Stasielak
- Institute of Nuclear Physics PAN, Krakow, Poland
| | - M Stephan
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A Stutz
- Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - F Suarez
- Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - M Suarez Durán
- Universidad Industrial de Santander, Bucaramanga, Colombia
| | - T Suomijärvi
- Institut de Physique Nucléaire d'Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - A D Supanitsky
- Instituto de Astronomía y Física del Espacio (IAFE, CONICET-UBA), Buenos Aires, Argentina
| | | | - J Swain
- Northeastern University, Boston, Massachusetts, USA
| | | | - O A Taborda
- Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - A Tapia
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A Tepe
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - V M Theodoro
- Universidade Estadual de Campinas, IFGW, Campinas, São Paulo, Brazil
| | - C Timmermans
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- Nikhef, Science Park, Amsterdam, Netherlands
| | - C J Todero Peixoto
- Universidade de São Paulo, Escola de Engenharia de Lorena, Lorena, São Paulo, Brazil
| | - G Toma
- "Horia Hulubei" National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - L Tomankova
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - B Tomé
- Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisboa, Portugal
| | - A Tonachini
- Università di Torino and Sezione INFN, Torino, Italy
| | - G Torralba Elipe
- Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - D Torres Machado
- Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro, Rio de Janeiro, Brazil
| | - P Travnicek
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - M Trini
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - R Ulrich
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - M Unger
- New York University, New York, New York, USA
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - M Urban
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - J F Valdés Galicia
- Universidad Nacional Autónoma de México, México, Distrito Federal, Mexico
| | - I Valiño
- Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - L Valore
- Università di Napoli "Federico II" and Sezione INFN, Napoli, Italy
| | - G van Aar
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - P van Bodegom
- University of Adelaide, Adelaide, South Australia, Australia
| | - A M van den Berg
- KVI - Center for Advanced Radiation Technology, University of Groningen, Groningen, Netherlands
| | - S van Velzen
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - A van Vliet
- Universität Hamburg, II. Institut für Theoretische Physik, Hamburg, Germany
| | - E Varela
- Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - B Vargas Cárdenas
- Universidad Nacional Autónoma de México, México, Distrito Federal, Mexico
| | - G Varner
- University of Hawaii, Honolulu, Hawaii, USA
| | - R Vasquez
- Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro, Rio de Janeiro, Brazil
| | - J R Vázquez
- Universidad Complutense de Madrid, Madrid, Spain
| | - R A Vázquez
- Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - D Veberič
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - V Verzi
- Università di Roma II "Tor Vergata" and Sezione INFN, Roma, Italy
| | - J Vicha
- Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - M Videla
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - L Villaseñor
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Michoacán, Mexico
| | - B Vlcek
- Universidad de Alcalá, Alcalá de Henares, Madrid, Spain
| | - S Vorobiov
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - H Wahlberg
- IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - O Wainberg
- Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - D Walz
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A A Watson
- School of Physics and Astronomy, University of Leeds, Leeds, United Kingdom
| | - M Weber
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - K Weidenhaupt
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A Weindl
- Karlsruhe Institute of Technology, Institut für Kernphysik, Karlsruhe, Germany
| | - C Welling
- RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - F Werner
- Karlsruhe Institute of Technology, Institut für Experimentelle Kernphysik (IEKP), Karlsruhe, Germany
| | - A Widom
- Northeastern University, Boston, Massachusetts, USA
| | - L Wiencke
- Colorado School of Mines, Golden, Colorado, USA
| | - H Wilczyński
- Institute of Nuclear Physics PAN, Krakow, Poland
| | - T Winchen
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - D Wittkowski
- Bergische Universität Wuppertal, Fachbereich C - Physik, Wuppertal, Germany
| | - B Wundheiler
- Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - S Wykes
- IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - L Yang
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - T Yapici
- Michigan Technological University, Houghton, Michigan, USA
| | - A Yushkov
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - E Zas
- Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - D Zavrtanik
- Experimental Particle Physics Department, J. Stefan Institute, Ljubljana, Slovenia
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - M Zavrtanik
- Experimental Particle Physics Department, J. Stefan Institute, Ljubljana, Slovenia
- Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - A Zepeda
- Centro de Investigación y de Estudios Avanzados del IPN (CINVESTAV), México, Distrito Federal, Mexico
| | - B Zimmermann
- Karlsruhe Institute of Technology, Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - M Ziolkowski
- Universität Siegen, Fachbereich 7 Physik - Experimentelle Teilchenphysik, Siegen, Germany
| | - F Zuccarello
- Università di Catania and Sezione INFN, Catania, Italy
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Sarkar B, Manikandan A, Jassal K, Ganesh T, Munshi A, Mohanti B, Pradhan A. SU-F-J-126: Influence of Six Dimensional Motions in Frameless Stereotactic Dosimetry Incorporating Rotational Shifts as Equivalent Translational Shifts: A Feasibility Study for Elekta-BrainLAB Stereotactic System. Med Phys 2016. [DOI: 10.1118/1.4956034] [Citation(s) in RCA: 4] [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: 11/07/2022] Open
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Giri U, Ganesh T, Saini V, Munshi A, Sarkar B, Mohanti B. SU-F-J-47: Inherent Uncertainty in the Positional Shifts Determined by a Volumetric Cone Beam Imaging System. Med Phys 2016. [DOI: 10.1118/1.4955955] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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Ganesh T, Sarkar B, Munshi A, Mohanti B. SU-F-T-429: Craniospinal Irradiation by VMAT Technique: Impact of FFF Beam and High Resolution MLC On Plan Quality. Med Phys 2016. [DOI: 10.1118/1.4956614] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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Kaur H, Kumar S, Sarkar B, Ganesh T, Giri U, Jassal K, Rathinamuthu S, Gulia G, Gopal V, Mohanti B, Munshi A. SU-F-T-327: Total Body Irradiation In-Vivo Dose Measurements Using Optically Stimulated Luminescence (OSL) NanoDots and Farmer Type Ion Chamber. Med Phys 2016. [DOI: 10.1118/1.4956512] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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Giri U, Sarkar B, Kaur H, Ganesh T, Munshi A, Mohanti B. SU-F-T-414: Mathematical Formulation of Gantry Starting Angle for Right Medial Tangential Arc in Left Intact Partial Breast Irradiation Using Volumetric Modulated Arc Therapy (VMAT). Med Phys 2016. [DOI: 10.1118/1.4956599] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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Giri U, Sarkar B, Munshi A, Kaur H, Jassal K, Rathinamuthu S, Kumar S, Ganesh T, Mohanti B. SU-F-T-422: Detection of Optimal Tangential Partial Arc Span for VMAT Planning in IntactLeft-Breast Treatment. Med Phys 2016. [DOI: 10.1118/1.4956607] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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Jassal K, Sarkar B, Ganesh T, Kaur H, Giri U, Mohanti B, Munshi A. SU-F-T-343: Dosimetric Investigation for Fluence Smoothing On VMAT Plans in Monaco for Head - Neck Cancers. Med Phys 2016. [DOI: 10.1118/1.4956528] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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Kumar S, Sarkar B, Kaur H, Rathinamuthu S, Giri U, Jassal K, Ganesh T, Munshi A, Mohanti B, Krishnankutty S, Sathiya J. SU-F-P-50: Performance Evaluation of Optically Stimulated Luminescence (OSL) NanoDots in Therapy and Imaging In-Vivo Dose Measurement During Patient Treatment. Med Phys 2016. [DOI: 10.1118/1.4955757] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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Munshi A, Sarkar B, Roy S, Ganesh T, Mohanti B. EP-1667: Dose fall off patterns and the OAR effect - experience of Linac based frameless radiosurgery. Radiother Oncol 2016. [DOI: 10.1016/s0167-8140(16)32918-8] [Citation(s) in RCA: 4] [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: 10/21/2022]
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Sarkar B, Pradhan A, Munshi A, Roy S, Ganesh T, Mohanti B. EP-1685: Influence of flat, flattening filter free beam model and different MLC’s on VMAT based SRS/SRT. Radiother Oncol 2016. [DOI: 10.1016/s0167-8140(16)32936-x] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/21/2022]
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Sarkar B, Pradhan A, Munshi A. Do technological advances in linear accelerators improve dosimetric outcomes in stereotaxy? A head-on comparison of seven linear accelerators using volumetric modulated arc therapy-based stereotactic planning. Indian J Cancer 2016; 53:166-73. [DOI: 10.4103/0019-509x.180815] [Citation(s) in RCA: 10] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/04/2022]
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Chekli L, Bayatsarmadi B, Sekine R, Sarkar B, Shen AM, Scheckel KG, Skinner W, Naidu R, Shon HK, Lombi E, Donner E. Analytical characterisation of nanoscale zero-valent iron: A methodological review. Anal Chim Acta 2015; 903:13-35. [PMID: 26709296 DOI: 10.1016/j.aca.2015.10.040] [Citation(s) in RCA: 69] [Impact Index Per Article: 7.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/26/2015] [Revised: 10/27/2015] [Accepted: 10/29/2015] [Indexed: 12/01/2022]
Abstract
Zero-valent iron nanoparticles (nZVI) have been widely tested as they are showing significant promise for environmental remediation. However, many recent studies have demonstrated that their mobility and reactivity in subsurface environments are significantly affected by their tendency to aggregate. Both the mobility and reactivity of nZVI mainly depends on properties such as particle size, surface chemistry and bulk composition. In order to ensure efficient remediation, it is crucial to accurately assess and understand the implications of these properties before deploying these materials into contaminated environments. Many analytical techniques are now available to determine these parameters and this paper provides a critical review of their usefulness and limitations for nZVI characterisation. These analytical techniques include microscopy and light scattering techniques for the determination of particle size, size distribution and aggregation state, and X-ray techniques for the characterisation of surface chemistry and bulk composition. Example characterisation data derived from commercial nZVI materials is used to further illustrate method strengths and limitations. Finally, some important challenges with respect to the characterisation of nZVI in groundwater samples are discussed.
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Affiliation(s)
- L Chekli
- School of Civil and Environmental Engineering, University of Technology, Sydney, Post Box 129, Broadway, NSW 2007, Australia; CRC CARE, PO Box 486, Salisbury, SA 5106, Australia
| | - B Bayatsarmadi
- School of Chemical Engineering, The University of Adelaide, Engineering North Building, Adelaide, SA 5005, Australia
| | - R Sekine
- Centre for Environmental Risk Assessment and Remediation, University of South Australia, Building X, Mawson Lakes Campus, SA 5095, Australia
| | - B Sarkar
- CRC CARE, PO Box 486, Salisbury, SA 5106, Australia; Centre for Environmental Risk Assessment and Remediation, University of South Australia, Building X, Mawson Lakes Campus, SA 5095, Australia
| | - A Maoz Shen
- Centre for Environmental Risk Assessment and Remediation, University of South Australia, Building X, Mawson Lakes Campus, SA 5095, Australia
| | - K G Scheckel
- U.S. Environmental Protection Agency, National Risk Management Research Laboratory, Land Remediation and Pollution Control Division, 5995 Center Hill Avenue, Cincinnati, OH, USA
| | - W Skinner
- Ian Wark Research Institute, University of South Australia, Building IW, Mawson Lakes Campus, SA 5095, Australia
| | - R Naidu
- CRC CARE, PO Box 486, Salisbury, SA 5106, Australia; Centre for Environmental Risk Assessment and Remediation, University of South Australia, Building X, Mawson Lakes Campus, SA 5095, Australia
| | - H K Shon
- School of Civil and Environmental Engineering, University of Technology, Sydney, Post Box 129, Broadway, NSW 2007, Australia; CRC CARE, PO Box 486, Salisbury, SA 5106, Australia
| | - E Lombi
- Centre for Environmental Risk Assessment and Remediation, University of South Australia, Building X, Mawson Lakes Campus, SA 5095, Australia.
| | - E Donner
- CRC CARE, PO Box 486, Salisbury, SA 5106, Australia; Centre for Environmental Risk Assessment and Remediation, University of South Australia, Building X, Mawson Lakes Campus, SA 5095, Australia
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Vanaja M, Maheswari M, Sathish P, Vagheera P, Jyothi Lakshmi N, Vijay Kumar G, Yadav SK, Razzaq A, Singh J, Sarkar B. Genotypic variability in physiological, biomass and yield response to drought stress in pigeonpea. Physiol Mol Biol Plants 2015; 21:541-549. [PMID: 26600680 PMCID: PMC4646872 DOI: 10.1007/s12298-015-0324-0] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/14/2015] [Revised: 09/21/2015] [Accepted: 10/05/2015] [Indexed: 06/03/2023]
Abstract
Three pigeonpea (Cajanus cajan L. Millsp.) genotypes- GT-1, AKP-1 and PRG-158 with varying crop duration, growth habit and flowering pattern were evaluated for variability in their response for drought stress. Drought stress was imposed at initiation of flowering and the observations on biomass and seed yield parameters were recorded at harvest. The magnitude of response of individual component to drought stress was found to be genotype specific. Drought stress significantly decreased photosynthetic rate (PN), transpiration rate (Tr) and relative water content (RWC) in all the genotypes, however the magnitude of reduction differed with genotype. With drought stress, the reduction of PN was highest in GT-1 while reduction in Tr was highest in PRG-158. The genotype AKP-1, accumulated significantly higher concentrations of osmotic solutes especially proline under water deficit stress, this facilitated it to maintain higher relative water content (RWC) and lower malondialdehyde (MDA) content as compared to other genotypes. Drought stress also impacted biomass production and their partitioning to vegetative and reproductive components at harvest. There was significant variability between the genotypes for seed yield under drought stress while it was non-significant under well-watered condition. Drought stress enhanced flower drop and decreased flower to pod conversion resulting in reduced pod number and seed number in PRG-158 and GT-1. The genotype AKP-1 recorded superior performance for seed yield under stress environment due to its ability in maintaining pod and seed number as well as improved test weight (100 seed weight). Under drought stress, significant positive association of seed yield with proline, seed number, pod number and test weight clearly indicating their role in drought tolerance.
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Affiliation(s)
- M. Vanaja
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - M. Maheswari
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - P. Sathish
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - P. Vagheera
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - N. Jyothi Lakshmi
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - G. Vijay Kumar
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - S. K. Yadav
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - Abdul Razzaq
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - Jainender Singh
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
| | - B. Sarkar
- Division of Crop Sciences, Central Research Institute for Dryland Agriculture (ICAR), Santoshnagar, Hyderabad, Telangana 500059 India
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Abstract
Therapeutic plasma exchange (TPE) has been reported to be a useful adjunct in severe systemic lupus erythematosus (SLE) but paediatric literature continues to be scanty. We hereby present three cases of refractory paediatric SLE (pSLE) with thrombotic thrombocytopenic purpura (TTP), diffuse alveolar haemorrhage (DAH) and crescentic glomerulonephritis which were treated with TPE as an adjunctive therapy. TPE was carried out in haemodialysis units using the membrane filtration technique. Demonstrable benefit of TPE was seen in all three cases. In refractory pSLE, TPE may be a useful tool and should be considered. The report additionally highlights the feasibility of undertaking TPE in haemodialysis units, which is important as haemodialysis units are more readily available than dedicated apheresis units in developing countries.
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Affiliation(s)
| | - R Sinha
- Institute of Child Health, Kolkata, India
- AMRI Hospitals, Kolkata, India
| | - P Pal
- Institute of Child Health, Kolkata, India
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Aab A, Abreu P, Aglietta M, Ahn EJ, Samarai IA, Albuquerque IFM, Allekotte I, Allen J, Allison P, Almela A, Castillo JA, Alvarez-Muñiz J, Batista RA, Ambrosio M, Aminaei A, Anchordoqui L, Andringa S, Aramo C, Aranda VM, Arqueros F, Asorey H, Assis P, Aublin J, Ave M, Avenier M, Avila G, Awal N, Badescu AM, Barber KB, Bäuml J, Baus C, Beatty JJ, Becker KH, Bellido JA, Berat C, Bertaina ME, Bertou X, Biermann PL, Billoir P, Blaess S, Blanco M, Bleve C, Blümer H, Boháčová M, Boncioli D, Bonifazi C, Bonino R, Borodai N, Brack J, Brancus I, Bridgeman A, Brogueira P, Brown WC, Buchholz P, Bueno A, Buitink S, Buscemi M, Caballero-Mora KS, Caccianiga B, Caccianiga L, Candusso M, Caramete L, Caruso R, Castellina A, Cataldi G, Cazon L, Cester R, Chavez AG, Chiavassa A, Chinellato JA, Chudoba J, Cilmo M, Clay RW, Cocciolo G, Colalillo R, Coleman A, Collica L, Coluccia MR, Conceição R, Contreras F, Cooper MJ, Cordier A, Coutu S, Covault CE, Cronin J, Curutiu A, Dallier R, Daniel B, Dasso S, Daumiller K, Dawson BR, Almeida RMD, Domenico MD, Jong SJD, Neto JRTDM, Mitri ID, Oliveira JD, Souza VD, Peral LD, Deligny O, Dembinski H, Dhital N, Giulio CD, Matteo AD, Diaz JC, Castro MLD, Diogo F, Dobrigkeit C, Docters W, D’Olivo JC, Dorofeev A, Hasankiadeh QD, Dova MT, Ebr J, Engel R, Erdmann M, Erfani M, Escobar CO, Espadanal J, Etchegoyen A, Luis PFS, Falcke H, Fang K, Farrar G, Fauth AC, Fazzini N, Ferguson AP, Fernandes M, Fick B, Figueira JM, Filevich A, Filipčič A, Fox BD, Fratu O, Fröhlich U, Fuchs B, Fujii T, Gaior R, García B, Roca STG, Garcia-Gamez D, Garcia-Pinto D, Garilli G, Bravo AG, Gate F, Gemmeke H, Ghia PL, Giaccari U, Giammarchi M, Giller M, Glaser C, Glass H, Berisso MG, Vitale PFG, Gonçalves P, Gonzalez JG, González N, Gookin B, Gordon J, Gorgi A, Gorham P, Gouffon P, Grebe S, Griffith N, Grillo AF, Grubb TD, Guarino F, Guedes GP, Hampel MR, Hansen P, Harari D, Harrison TA, Hartmann S, Harton JL, Haungs A, Hebbeker T, Heck D, Heimann P, Herve AE, Hill GC, Hojvat C, Hollon N, Holt E, Homola P, Hörandel JR, Horvath P, Hrabovský M, Huber D, Huege T, Insolia A, Isar PG, Jandt I, Jansen S, Jarne C, Josebachuili M, Kääpä A, Kambeitz O, Kampert KH, Kasper P, Katkov I, Kégl B, Keilhauer B, Keivani A, Kemp E, Kieckhafer RM, Klages HO, Kleifges M, Kleinfeller J, Krause R, Krohm N, Krömer O, Kruppke-Hansen D, Kuempel D, Kunka N, LaHurd D, Latronico L, Lauer R, Lauscher M, Lautridou P, Coz SL, Leão MSAB, Lebrun D, Lebrun P, Oliveira MALD, Letessier-Selvon A, Lhenry-Yvon I, Link K, López R, Agüera AL, Louedec K, Bahilo JL, Lu L, Lucero A, Ludwig M, Malacari M, Maldera S, Mallamaci M, Maller J, Mandat D, Mantsch P, Mariazzi AG, Marin V, Mariş IC, Marsella G, Martello D, Martin L, Martinez H, Bravo OM, Martraire D, Meza JJM, Mathes HJ, Mathys S, Matthews J, Matthews JAJ, Matthiae G, Maurel D, Maurizio D, Mayotte E, Mazur PO, Medina C, Medina-Tanco G, Meissner R, Melissas M, Melo D, Menshikov A, Messina S, Meyhandan R, Mićanović S, Micheletti MI, Middendorf L, Minaya IA, Miramonti L, Mitrica B, Molina-Bueno L, Mollerach S, Monasor M, Ragaigne DM, Montanet F, Morello C, Mostafá M, Moura CA, Muller MA, Müller G, Müller S, Münchmeyer M, Mussa R, Navarra G, Navas S, Necesal P, Nellen L, Nelles A, Neuser J, Nguyen P, Niechciol M, Niemietz L, Niggemann T, Nitz D, Nosek D, Novotny V, Nožka L, Ochilo L, Olinto A, Oliveira M, Pacheco N, Selmi-Dei DP, Palatka M, Pallotta J, Palmieri N, Papenbreer P, Parente G, Parra A, Paul T, Pech M, Pȩkala J, Pelayo R, Pepe IM, Perrone L, Petermann E, Peters C, Petrera S, Petrov Y, Phuntsok J, Piegaia R, Pierog T, Pieroni P, Pimenta M, Pirronello V, Platino M, Plum M, Porcelli A, Porowski C, Prado RR, Privitera P, Prouza M, Purrello V, Quel EJ, Querchfeld S, Quinn S, Rautenberg J, Ravel O, Ravignani D, Revenu B, Ridky J, Riggi S, Risse M, Ristori P, Rizi V, Carvalho WRD, Cabo IR, Fernandez GR, Rojo JR, Rodríguez-Frías MD, Rogozin D, Ros G, Rosado J, Rossler T, Roth M, Roulet E, Rovero AC, Saffi SJ, Saftoiu A, Salamida F, Salazar H, Saleh A, Greus FS, Salina G, Sánchez F, Sanchez-Lucas P, Santo CE, Santos E, Santos EM, Sarazin F, Sarkar B, Sarmento R, Sato R, Scharf N, Scherini V, Schieler H, Schiffer P, Schmidt D, Schröder FG, Scholten O, Schoorlemmer H, Schovánek P, Schulz A, Schulz J, Schumacher J, Sciutto SJ, Segreto A, Settimo M, Shadkam A, Shellard RC, Sidelnik I, Sigl G, Sima O, kowski AŚ, Šmída R, Snow GR, Sommers P, Sorokin J, Squartini R, Srivastava YN, Stanič S, Stapleton J, Stasielak J, Stephan M, Stutz A, Suarez F, Suomijärvi T, Supanitsky AD, Sutherland MS, Swain J, Szadkowski Z, Szuba M, Taborda OA, Tapia A, Tartare M, Tepe A, Theodoro VM, Timmermans C, Peixoto CJT, Toma G, Tomankova L, Tomé B, Tonachini A, Elipe GT, Machado DT, Travnicek P, Trovato E, Tueros M, Ulrich R, Unger M, Urban M, Galicia JFV, Valiño I, Valore L, Aar GV, Bodegom PV, Berg AMVD, Velzen SV, Vliet AV, Varela E, Vargas Cárdenas B, Varner G, Vázquez JR, Vázquez RA, Veberič D, Verzi V, Vicha J, Videla M, Villaseñor L, Vlcek B, Vorobiov S, Wahlberg H, Wainberg O, Walz D, Watson AA, Weber M, Weidenhaupt K, Weindl A, Werner F, Widom A, Wiencke L, Wilczyńska B, Wilczyński H, Will M, Williams C, Winchen T, Wittkowski D, Wundheiler B, Wykes S, Yamamoto T, Yapici T, Yuan G, Yushkov A, Zamorano B, Zas E, Zavrtanik D, Zavrtanik M, Zaw I, Zepeda A, Zhou J, Zhu Y, Silva MZ, Ziolkowski M, Zuccarello F. Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory. Eur Phys J C Part Fields 2015; 75:269. [PMID: 26120280 PMCID: PMC4477714 DOI: 10.1140/epjc/s10052-015-3471-0] [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] [Figures] [Subscribe] [Scholar Register] [Received: 10/03/2014] [Accepted: 05/20/2015] [Indexed: 06/04/2023]
Abstract
Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with [Formula: see text] eV by analyzing cosmic rays with energies above [Formula: see text] eV arriving within an angular separation of approximately 15[Formula: see text]. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with astrophysical scenarios can therefore be used to obtain constraints on related model parameters such as strength of cosmic-ray deflection and density of point sources.
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Affiliation(s)
- A. Aab
- />Universität Siegen, Siegen, Germany
| | - P. Abreu
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - M. Aglietta
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | | | - I. Al Samarai
- />Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | | | - I. Allekotte
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - J. Allen
- />New York University, New York, NY USA
| | - P. Allison
- />Ohio State University, Columbus, OH USA
| | - A. Almela
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
- />Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina
| | | | - J. Alvarez-Muñiz
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | | | - M. Ambrosio
- />Università di Napoli “Federico II” and Sezione INFN, Napoli, Italy
| | - A. Aminaei
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - L. Anchordoqui
- />Department of Physics and Astronomy, City University of New York, New York, USA
| | - S. Andringa
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - C. Aramo
- />Università di Napoli “Federico II” and Sezione INFN, Napoli, Italy
| | - V. M. Aranda
- />Universidad Complutense de Madrid, Madrid, Spain
| | - F. Arqueros
- />Universidad Complutense de Madrid, Madrid, Spain
| | - H. Asorey
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - P. Assis
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - J. Aublin
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - M. Ave
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - M. Avenier
- />Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - G. Avila
- />Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina
| | - N. Awal
- />New York University, New York, NY USA
| | - A. M. Badescu
- />University Politehnica of Bucharest, Bucharest, Romania
| | - K. B. Barber
- />University of Adelaide, Adelaide, SA Australia
| | - J. Bäuml
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - C. Baus
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | | | - K. H. Becker
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | | | - C. Berat
- />Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - M. E. Bertaina
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - X. Bertou
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - P. L. Biermann
- />Max-Planck-Institut für Radioastronomie, Bonn, Germany
| | - P. Billoir
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - S. Blaess
- />University of Adelaide, Adelaide, SA Australia
| | - M. Blanco
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - C. Bleve
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | - H. Blümer
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - M. Boháčová
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - D. Boncioli
- />INFN, Laboratori Nazionali del Gran Sasso, Assergi, L’Aquila Italy
| | - C. Bonifazi
- />Instituto de Física, Universidade Federal do Rio de Janeiro, Rio de Janeiro, RJ Brazil
| | - R. Bonino
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - N. Borodai
- />Institute of Nuclear Physics PAN, Krakow, Poland
| | - J. Brack
- />Colorado State University, Fort Collins, CO USA
| | - I. Brancus
- />’Horia Hulubei’ National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - A. Bridgeman
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - P. Brogueira
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | | | | | - A. Bueno
- />Universidad de Granada and C.A.F.P.E., Granada, Spain
| | - S. Buitink
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - M. Buscemi
- />Università di Napoli “Federico II” and Sezione INFN, Napoli, Italy
| | - K. S. Caballero-Mora
- />Centro de Investigación y de Estudios Avanzados del IPN (CINVESTAV), Mexico, Mexico
| | - B. Caccianiga
- />Università di Milano and Sezione INFN, Milan, Italy
| | - L. Caccianiga
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - M. Candusso
- />Università di Roma II “Tor Vergata” and Sezione INFN, Roma, Italy
| | - L. Caramete
- />Max-Planck-Institut für Radioastronomie, Bonn, Germany
| | - R. Caruso
- />Università di Catania and Sezione INFN, Catania, Italy
| | - A. Castellina
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - G. Cataldi
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | - L. Cazon
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - R. Cester
- />Università di Torino and Sezione INFN, Torino, Italy
| | - A. G. Chavez
- />Universidad Michoacana de San Nicolas de Hidalgo, Morelia, Michoacan Mexico
| | - A. Chiavassa
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | | | - J. Chudoba
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - M. Cilmo
- />Università di Napoli “Federico II” and Sezione INFN, Napoli, Italy
| | - R. W. Clay
- />University of Adelaide, Adelaide, SA Australia
| | - G. Cocciolo
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | - R. Colalillo
- />Università di Napoli “Federico II” and Sezione INFN, Napoli, Italy
| | - A. Coleman
- />Pennsylvania State University, University Park, PA USA
| | - L. Collica
- />Università di Milano and Sezione INFN, Milan, Italy
| | - M. R. Coluccia
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | - R. Conceição
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - F. Contreras
- />Observatorio Pierre Auger, Malargüe, Argentina
| | - M. J. Cooper
- />University of Adelaide, Adelaide, SA Australia
| | - A. Cordier
- />Laboratoire de l’Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - S. Coutu
- />Pennsylvania State University, University Park, PA USA
| | - C. E. Covault
- />Case Western Reserve University, Cleveland, OH USA
| | - J. Cronin
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - A. Curutiu
- />Max-Planck-Institut für Radioastronomie, Bonn, Germany
| | - R. Dallier
- />Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, Nançay, France
- />SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - B. Daniel
- />Universidade Estadual de Campinas, IFGW, Campinas, SP Brazil
| | - S. Dasso
- />Departamento de Física, FCEyN Universidad de Buenos Aires y CONICET, Buenos Aires, Argentina
- />Instituto de Astronomía y Física del Espacio (CONICET-UBA), Buenos Aires, Argentina
| | - K. Daumiller
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - B. R. Dawson
- />University of Adelaide, Adelaide, SA Australia
| | - R. M. de Almeida
- />Universidade Federal Fluminense, EEIMVR, Volta Redonda, RJ Brazil
| | - M. De Domenico
- />Università di Catania and Sezione INFN, Catania, Italy
| | - S. J. de Jong
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- />Nikhef, Science Park, Amsterdam, Netherlands
| | - J. R. T. de Mello Neto
- />Instituto de Física, Universidade Federal do Rio de Janeiro, Rio de Janeiro, RJ Brazil
| | - I. De Mitri
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | - J. de Oliveira
- />Universidade Federal Fluminense, EEIMVR, Volta Redonda, RJ Brazil
| | - V. de Souza
- />Instituto de Física de São Carlos, Universidade de São Paulo, São Carlos, SP Brazil
| | - L. del Peral
- />Universidad de Alcalá, Alcalá de Henares, Madrid Spain
| | - O. Deligny
- />Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - H. Dembinski
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - N. Dhital
- />Michigan Technological University, Houghton, MI USA
| | - C. Di Giulio
- />Università di Roma II “Tor Vergata” and Sezione INFN, Roma, Italy
| | - A. Di Matteo
- />Dipartimento di Scienze Fisiche e Chimiche dell’Università dell’Aquila and INFN, L’Aquila, Italy
| | - J. C. Diaz
- />Michigan Technological University, Houghton, MI USA
| | | | - F. Diogo
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - C. Dobrigkeit
- />Universidade Estadual de Campinas, IFGW, Campinas, SP Brazil
| | - W. Docters
- />KVI - Center for Advanced Radiation Technology, University of Groningen, Groningen, Netherlands
| | - J. C. D’Olivo
- />Universidad Nacional Autonoma de Mexico, Mexico, D.F., Mexico
| | - A. Dorofeev
- />Colorado State University, Fort Collins, CO USA
| | - Q. Dorosti Hasankiadeh
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - M. T. Dova
- />IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - J. Ebr
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - R. Engel
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - M. Erdmann
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - M. Erfani
- />Universität Siegen, Siegen, Germany
| | - C. O. Escobar
- />Universidade Estadual de Campinas, IFGW, Campinas, SP Brazil
- />Fermilab, Batavia, IL USA
| | - J. Espadanal
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - A. Etchegoyen
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
- />Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina
| | | | - H. Falcke
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- />Nikhef, Science Park, Amsterdam, Netherlands
- />ASTRON, Dwingeloo, Netherlands
| | - K. Fang
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - G. Farrar
- />New York University, New York, NY USA
| | - A. C. Fauth
- />Universidade Estadual de Campinas, IFGW, Campinas, SP Brazil
| | | | | | - M. Fernandes
- />Instituto de Física, Universidade Federal do Rio de Janeiro, Rio de Janeiro, RJ Brazil
| | - B. Fick
- />Michigan Technological University, Houghton, MI USA
| | - J. M. Figueira
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A. Filevich
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A. Filipčič
- />Experimental Particle Physics Department, J. Stefan Institute, Ljubljana, Slovenia
- />Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - B. D. Fox
- />University of Hawaii, Honolulu, HI USA
| | - O. Fratu
- />University Politehnica of Bucharest, Bucharest, Romania
| | | | - B. Fuchs
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - T. Fujii
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - R. Gaior
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - B. García
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM) and National Technological University, Faculty Mendoza (CONICET/CNEA), Mendoza, Argentina
| | - S. T. Garcia Roca
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - D. Garcia-Gamez
- />Laboratoire de l’Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, France
| | | | - G. Garilli
- />Università di Catania and Sezione INFN, Catania, Italy
| | | | - F. Gate
- />SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - H. Gemmeke
- />Karlsruhe Institute of Technology - Campus North - Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - P. L. Ghia
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - U. Giaccari
- />Instituto de Física, Universidade Federal do Rio de Janeiro, Rio de Janeiro, RJ Brazil
| | - M. Giammarchi
- />Università di Milano and Sezione INFN, Milan, Italy
| | | | - C. Glaser
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | | | - M. Gómez Berisso
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - P. F. Gómez Vitale
- />Observatorio Pierre Auger and Comisión Nacional de Energía Atómica, Malargüe, Argentina
| | - P. Gonçalves
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - J. G. Gonzalez
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - N. González
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - B. Gookin
- />Colorado State University, Fort Collins, CO USA
| | - J. Gordon
- />Ohio State University, Columbus, OH USA
| | - A. Gorgi
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - P. Gorham
- />University of Hawaii, Honolulu, HI USA
| | - P. Gouffon
- />Instituto de Física, Universidade de São Paulo, São Paulo, SP Brazil
| | - S. Grebe
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- />Nikhef, Science Park, Amsterdam, Netherlands
| | | | - A. F. Grillo
- />INFN, Laboratori Nazionali del Gran Sasso, Assergi, L’Aquila Italy
| | - T. D. Grubb
- />University of Adelaide, Adelaide, SA Australia
| | - F. Guarino
- />Università di Napoli “Federico II” and Sezione INFN, Napoli, Italy
| | - G. P. Guedes
- />Universidade Estadual de Feira de Santana, Feira de Santana, Brazil
| | - M. R. Hampel
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - P. Hansen
- />IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - D. Harari
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | | | - S. Hartmann
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - J. L. Harton
- />Colorado State University, Fort Collins, CO USA
| | - A. Haungs
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - T. Hebbeker
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - D. Heck
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | | | - A. E. Herve
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - G. C. Hill
- />University of Adelaide, Adelaide, SA Australia
| | | | - N. Hollon
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - E. Holt
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - P. Homola
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - J. R. Hörandel
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- />Nikhef, Science Park, Amsterdam, Netherlands
| | - P. Horvath
- />Palacky University, RCPTM, Olomouc, Czech Republic
| | - M. Hrabovský
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
- />Palacky University, RCPTM, Olomouc, Czech Republic
| | - D. Huber
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - T. Huege
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - A. Insolia
- />Università di Catania and Sezione INFN, Catania, Italy
| | - P. G. Isar
- />Institute of Space Sciences, Bucharest-Magurele, Romania
| | - I. Jandt
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - S. Jansen
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- />Nikhef, Science Park, Amsterdam, Netherlands
| | - C. Jarne
- />IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - M. Josebachuili
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A. Kääpä
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - O. Kambeitz
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - K. H. Kampert
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | | | - I. Katkov
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - B. Kégl
- />Laboratoire de l’Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - B. Keilhauer
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - A. Keivani
- />Pennsylvania State University, University Park, PA USA
| | - E. Kemp
- />Universidade Estadual de Campinas, IFGW, Campinas, SP Brazil
| | | | - H. O. Klages
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - M. Kleifges
- />Karlsruhe Institute of Technology - Campus North - Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | | | - R. Krause
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - N. Krohm
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - O. Krömer
- />Karlsruhe Institute of Technology - Campus North - Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | | | - D. Kuempel
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - N. Kunka
- />Karlsruhe Institute of Technology - Campus North - Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - D. LaHurd
- />Case Western Reserve University, Cleveland, OH USA
| | - L. Latronico
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - R. Lauer
- />University of New Mexico, Albuquerque, NM USA
| | - M. Lauscher
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - P. Lautridou
- />SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - S. Le Coz
- />Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - M. S. A. B. Leão
- />Faculdade Independente do Nordeste, Vitória da Conquista, Brazil
| | - D. Lebrun
- />Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | | | | | - A. Letessier-Selvon
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - I. Lhenry-Yvon
- />Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - K. Link
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - R. López
- />Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - A. Lopez Agüera
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - K. Louedec
- />Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | | | - L. Lu
- />Bergische Universität Wuppertal, Wuppertal, Germany
- />School of Physics and Astronomy, University of Leeds, Leeds, UK
| | - A. Lucero
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - M. Ludwig
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - M. Malacari
- />University of Adelaide, Adelaide, SA Australia
| | - S. Maldera
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - M. Mallamaci
- />Università di Milano and Sezione INFN, Milan, Italy
| | - J. Maller
- />SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - D. Mandat
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | | | - A. G. Mariazzi
- />IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - V. Marin
- />SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - I. C. Mariş
- />Universidad de Granada and C.A.F.P.E., Granada, Spain
| | - G. Marsella
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | - D. Martello
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | - L. Martin
- />Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, Nançay, France
- />SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - H. Martinez
- />Centro de Investigación y de Estudios Avanzados del IPN (CINVESTAV), Mexico, Mexico
| | | | - D. Martraire
- />Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - J. J. Masías Meza
- />Departamento de Física, FCEyN Universidad de Buenos Aires y CONICET, Buenos Aires, Argentina
| | - H. J. Mathes
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - S. Mathys
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - J. Matthews
- />Louisiana State University, Baton Rouge, LA USA
| | | | - G. Matthiae
- />Università di Roma II “Tor Vergata” and Sezione INFN, Roma, Italy
| | - D. Maurel
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - D. Maurizio
- />Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJ Brazil
| | - E. Mayotte
- />Colorado School of Mines, Golden, CO USA
| | | | - C. Medina
- />Colorado School of Mines, Golden, CO USA
| | - G. Medina-Tanco
- />Universidad Nacional Autonoma de Mexico, Mexico, D.F., Mexico
| | - R. Meissner
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - M. Melissas
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - D. Melo
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - A. Menshikov
- />Karlsruhe Institute of Technology - Campus North - Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - S. Messina
- />KVI - Center for Advanced Radiation Technology, University of Groningen, Groningen, Netherlands
| | | | - S. Mićanović
- />Rudjer Bošković Institute, 10000 Zagreb, Croatia
| | - M. I. Micheletti
- />Instituto de Física de Rosario (IFIR), CONICET/U.N.R. and Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Rosario, Argentina
| | - L. Middendorf
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - I. A. Minaya
- />Universidad Complutense de Madrid, Madrid, Spain
| | - L. Miramonti
- />Università di Milano and Sezione INFN, Milan, Italy
| | - B. Mitrica
- />’Horia Hulubei’ National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | | | - S. Mollerach
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - M. Monasor
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - D. Monnier Ragaigne
- />Laboratoire de l’Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - F. Montanet
- />Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - C. Morello
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - M. Mostafá
- />Pennsylvania State University, University Park, PA USA
| | - C. A. Moura
- />Universidade Federal do ABC, Santo André, SP Brazil
| | - M. A. Muller
- />Universidade Estadual de Campinas, IFGW, Campinas, SP Brazil
- />Universidade Federal de Pelotas, Pelotas, RS Brazil
| | - G. Müller
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - S. Müller
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - M. Münchmeyer
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - R. Mussa
- />Università di Torino and Sezione INFN, Torino, Italy
| | - G. Navarra
- />Osservatorio Astrofisico di Torino (INAF), Università di Torino and Sezione INFN, Torino, Italy
| | - S. Navas
- />Universidad de Granada and C.A.F.P.E., Granada, Spain
| | - P. Necesal
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - L. Nellen
- />Universidad Nacional Autonoma de Mexico, Mexico, D.F., Mexico
| | - A. Nelles
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- />Nikhef, Science Park, Amsterdam, Netherlands
| | - J. Neuser
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - P. Nguyen
- />University of Adelaide, Adelaide, SA Australia
| | | | - L. Niemietz
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - T. Niggemann
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - D. Nitz
- />Michigan Technological University, Houghton, MI USA
| | - D. Nosek
- />Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Charles University, Prague, Czech Republic
| | - V. Novotny
- />Faculty of Mathematics and Physics, Institute of Particle and Nuclear Physics, Charles University, Prague, Czech Republic
| | - L. Nožka
- />Palacky University, RCPTM, Olomouc, Czech Republic
| | - L. Ochilo
- />Universität Siegen, Siegen, Germany
| | - A. Olinto
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - M. Oliveira
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - N. Pacheco
- />Universidad de Alcalá, Alcalá de Henares, Madrid Spain
| | | | - M. Palatka
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - J. Pallotta
- />Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Villa Martelli, Buenos Aires, Argentina
| | - N. Palmieri
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - P. Papenbreer
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - G. Parente
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - A. Parra
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - T. Paul
- />Department of Physics and Astronomy, City University of New York, New York, USA
- />Northeastern University, Boston, MA USA
| | - M. Pech
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - J. Pȩkala
- />Institute of Nuclear Physics PAN, Krakow, Poland
| | - R. Pelayo
- />Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - I. M. Pepe
- />Universidade Federal da Bahia, Salvador, BA Brazil
| | - L. Perrone
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | | | - C. Peters
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - S. Petrera
- />Dipartimento di Scienze Fisiche e Chimiche dell’Università dell’Aquila and INFN, L’Aquila, Italy
- />Gran Sasso Science Institute (INFN), L’Aquila, Italy
| | - Y. Petrov
- />Colorado State University, Fort Collins, CO USA
| | - J. Phuntsok
- />Pennsylvania State University, University Park, PA USA
| | - R. Piegaia
- />Departamento de Física, FCEyN Universidad de Buenos Aires y CONICET, Buenos Aires, Argentina
| | - T. Pierog
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - P. Pieroni
- />Departamento de Física, FCEyN Universidad de Buenos Aires y CONICET, Buenos Aires, Argentina
| | - M. Pimenta
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - V. Pirronello
- />Università di Catania and Sezione INFN, Catania, Italy
| | - M. Platino
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - M. Plum
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A. Porcelli
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - C. Porowski
- />Institute of Nuclear Physics PAN, Krakow, Poland
| | - R. R. Prado
- />Instituto de Física de São Carlos, Universidade de São Paulo, São Carlos, SP Brazil
| | - P. Privitera
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - M. Prouza
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - V. Purrello
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - E. J. Quel
- />Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Villa Martelli, Buenos Aires, Argentina
| | - S. Querchfeld
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - S. Quinn
- />Case Western Reserve University, Cleveland, OH USA
| | - J. Rautenberg
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - O. Ravel
- />SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - D. Ravignani
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - B. Revenu
- />SUBATECH, École des Mines de Nantes, CNRS-IN2P3, Université de Nantes, Nantes, France
| | - J. Ridky
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - S. Riggi
- />Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - M. Risse
- />Universität Siegen, Siegen, Germany
| | - P. Ristori
- />Centro de Investigaciones en Láseres y Aplicaciones, CITEDEF and CONICET, Villa Martelli, Buenos Aires, Argentina
| | - V. Rizi
- />Dipartimento di Scienze Fisiche e Chimiche dell’Università dell’Aquila and INFN, L’Aquila, Italy
| | | | - I. Rodriguez Cabo
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - G. Rodriguez Fernandez
- />Università di Roma II “Tor Vergata” and Sezione INFN, Roma, Italy
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | | | | | - D. Rogozin
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - G. Ros
- />Universidad de Alcalá, Alcalá de Henares, Madrid Spain
| | - J. Rosado
- />Universidad Complutense de Madrid, Madrid, Spain
| | - T. Rossler
- />Palacky University, RCPTM, Olomouc, Czech Republic
| | - M. Roth
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - E. Roulet
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - A. C. Rovero
- />Instituto de Astronomía y Física del Espacio (CONICET-UBA), Buenos Aires, Argentina
| | - S. J. Saffi
- />University of Adelaide, Adelaide, SA Australia
| | - A. Saftoiu
- />’Horia Hulubei’ National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - F. Salamida
- />Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - H. Salazar
- />Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - A. Saleh
- />Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | | | - G. Salina
- />Università di Roma II “Tor Vergata” and Sezione INFN, Roma, Italy
| | - F. Sánchez
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | | | - C. E. Santo
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - E. Santos
- />Universidade Estadual de Campinas, IFGW, Campinas, SP Brazil
| | - E. M. Santos
- />Instituto de Física, Universidade de São Paulo, São Paulo, SP Brazil
| | - F. Sarazin
- />Colorado School of Mines, Golden, CO USA
| | - B. Sarkar
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - R. Sarmento
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - R. Sato
- />Observatorio Pierre Auger, Malargüe, Argentina
| | - N. Scharf
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - V. Scherini
- />Dipartimento di Matematica e Fisica “E. De Giorgi” dell’Università del Salento and Sezione INFN, Lecce, Italy
| | - H. Schieler
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | | | - D. Schmidt
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - F. G. Schröder
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - O. Scholten
- />KVI - Center for Advanced Radiation Technology, University of Groningen, Groningen, Netherlands
| | - H. Schoorlemmer
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- />Nikhef, Science Park, Amsterdam, Netherlands
- />University of Hawaii, Honolulu, HI USA
| | - P. Schovánek
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - A. Schulz
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - J. Schulz
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - J. Schumacher
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - S. J. Sciutto
- />IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - A. Segreto
- />Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo (INAF), Palermo, Italy
| | - M. Settimo
- />Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, Paris, France
| | - A. Shadkam
- />Louisiana State University, Baton Rouge, LA USA
| | - R. C. Shellard
- />Centro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJ Brazil
| | - I. Sidelnik
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - G. Sigl
- />Universität Hamburg, Hamburg, Germany
| | - O. Sima
- />Physics Department, University of Bucharest, Bucharest, Romania
| | | | - R. Šmída
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - G. R. Snow
- />University of Nebraska, Lincoln, NE USA
| | - P. Sommers
- />Pennsylvania State University, University Park, PA USA
| | - J. Sorokin
- />University of Adelaide, Adelaide, SA Australia
| | - R. Squartini
- />Observatorio Pierre Auger, Malargüe, Argentina
| | | | - S. Stanič
- />Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | | | - J. Stasielak
- />Institute of Nuclear Physics PAN, Krakow, Poland
| | - M. Stephan
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A. Stutz
- />Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - F. Suarez
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - T. Suomijärvi
- />Institut de Physique Nucléaire d’Orsay (IPNO), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - A. D. Supanitsky
- />Instituto de Astronomía y Física del Espacio (CONICET-UBA), Buenos Aires, Argentina
| | | | - J. Swain
- />Northeastern University, Boston, MA USA
| | | | - M. Szuba
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - O. A. Taborda
- />Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, Argentina
| | - A. Tapia
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - M. Tartare
- />Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Grenoble-Alpes, CNRS/IN2P3, Grenoble, France
| | - A. Tepe
- />Universität Siegen, Siegen, Germany
| | - V. M. Theodoro
- />Universidade Estadual de Campinas, IFGW, Campinas, SP Brazil
| | - C. Timmermans
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
- />Nikhef, Science Park, Amsterdam, Netherlands
| | | | - G. Toma
- />’Horia Hulubei’ National Institute for Physics and Nuclear Engineering, Bucharest-Magurele, Romania
| | - L. Tomankova
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - B. Tomé
- />Laboratório de Instrumentação e Física Experimental de Partículas - LIP and Instituto Superior Técnico - IST, Universidade de Lisboa - UL, Lisbon, Portugal
| | - A. Tonachini
- />Università di Torino and Sezione INFN, Torino, Italy
| | - G. Torralba Elipe
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - D. Torres Machado
- />Instituto de Física, Universidade Federal do Rio de Janeiro, Rio de Janeiro, RJ Brazil
| | - P. Travnicek
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - E. Trovato
- />Università di Catania and Sezione INFN, Catania, Italy
| | - M. Tueros
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - R. Ulrich
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - M. Unger
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - M. Urban
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | | | - I. Valiño
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - L. Valore
- />Università di Napoli “Federico II” and Sezione INFN, Napoli, Italy
| | - G. van Aar
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | | | - A. M. van den Berg
- />KVI - Center for Advanced Radiation Technology, University of Groningen, Groningen, Netherlands
| | - S. van Velzen
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | | | - E. Varela
- />Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | | | - G. Varner
- />University of Hawaii, Honolulu, HI USA
| | | | - R. A. Vázquez
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - D. Veberič
- />Laboratoire de l’Accélérateur Linéaire (LAL), Université Paris 11, CNRS-IN2P3, Orsay, France
| | - V. Verzi
- />Università di Roma II “Tor Vergata” and Sezione INFN, Roma, Italy
| | - J. Vicha
- />Institute of Physics of the Academy of Sciences of the Czech Republic, Prague, Czech Republic
| | - M. Videla
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - L. Villaseñor
- />Universidad Michoacana de San Nicolas de Hidalgo, Morelia, Michoacan Mexico
| | - B. Vlcek
- />Universidad de Alcalá, Alcalá de Henares, Madrid Spain
| | - S. Vorobiov
- />Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - H. Wahlberg
- />IFLP, Universidad Nacional de La Plata and CONICET, La Plata, Argentina
| | - O. Wainberg
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
- />Universidad Tecnológica Nacional - Facultad Regional Buenos Aires, Buenos Aires, Argentina
| | - D. Walz
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A. A. Watson
- />School of Physics and Astronomy, University of Leeds, Leeds, UK
| | - M. Weber
- />Karlsruhe Institute of Technology - Campus North - Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | - K. Weidenhaupt
- />RWTH Aachen University, III. Physikalisches Institut A, Aachen, Germany
| | - A. Weindl
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - F. Werner
- />Karlsruhe Institute of Technology - Campus South - Institut für Experimentelle, Kernphysik (IEKP), Karlsruhe, Germany
| | - A. Widom
- />Northeastern University, Boston, MA USA
| | - L. Wiencke
- />Colorado School of Mines, Golden, CO USA
| | | | | | - M. Will
- />Karlsruhe Institute of Technology - Campus North - Institut für Kernphysik, Karlsruhe, Germany
| | - C. Williams
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - T. Winchen
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - D. Wittkowski
- />Bergische Universität Wuppertal, Wuppertal, Germany
| | - B. Wundheiler
- />Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, Argentina
| | - S. Wykes
- />IMAPP, Radboud University Nijmegen, Nijmegen, Netherlands
| | - T. Yamamoto
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - T. Yapici
- />Michigan Technological University, Houghton, MI USA
| | - G. Yuan
- />Louisiana State University, Baton Rouge, LA USA
| | | | - B. Zamorano
- />Universidad de Granada and C.A.F.P.E., Granada, Spain
| | - E. Zas
- />Universidad de Santiago de Compostela, Santiago de Compostela, Spain
| | - D. Zavrtanik
- />Experimental Particle Physics Department, J. Stefan Institute, Ljubljana, Slovenia
- />Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - M. Zavrtanik
- />Experimental Particle Physics Department, J. Stefan Institute, Ljubljana, Slovenia
- />Laboratory for Astroparticle Physics, University of Nova Gorica, Nova Gorica, Slovenia
| | - I. Zaw
- />New York University, New York, NY USA
| | - A. Zepeda
- />Centro de Investigación y de Estudios Avanzados del IPN (CINVESTAV), Mexico, Mexico
| | - J. Zhou
- />Enrico Fermi Institute, University of Chicago, Chicago, IL USA
| | - Y. Zhu
- />Karlsruhe Institute of Technology - Campus North - Institut für Prozessdatenverarbeitung und Elektronik, Karlsruhe, Germany
| | | | | | - F. Zuccarello
- />Università di Catania and Sezione INFN, Catania, Italy
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Jassal K, Sarkar B, Mohanti B, Roy S, Ganesh T, Munshi A, Chougule A, Sachdev K. SU-E-T-77: A Statistical Approach to Manage Quality for Pre-Treatment Verification in IMRT/VMAT. Med Phys 2015. [DOI: 10.1118/1.4924438] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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Sarkar B, Roy S, Munshi A, Pradhan A. SU-E-T-583: Operated Left Breast and Chest Wall Radiotherapy: A Dosimetric Comparison Between 3DCRT,IMRT and VMAT. Med Phys 2015. [DOI: 10.1118/1.4924945] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022] Open
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