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Abstract
This paper comments on the Effects of Racism on Oral Health in the United States (US). It provides the background and sets the stage to raise questions about race: how was race defined originally, what exactly is race, and how have racial categories been enumerated? Following this path, the paper broadens the scope of view regarding data attributable to racial categories pointing to social and cultural factors that influence overall health outcomes, particularly those related to oral health. Oral health researchers, advocates, providers, administrators, program planners, and funders, among others rely on data, often compiled by racial categories. We should be aware of potential vagaries that can accompany race-based data, and its interpretation and application, regarding oral health. The paper suggests we should be mindful of other influences that affect documented differences among populations regarding their oral health status.
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Affiliation(s)
- C A Evans
- College of Dentistry, University of Illinois at Chicago, IL 60612, United States
| | - P D Smith
- College of Dentistry, University of Illinois at Chicago, IL 60612, United States
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2
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Abstract
Eleven patients with lipodermatosclerosis (LDS) and 14 patients without venous or arterial disease underwent measurement of xenon-133 (133Xe) half-clearance times from the gaiter region of the leg. Xenon has similar diffusion characteristics to oxygen, and the investigation reflects the ability of the isotope to diffuse from the skin surface into capillary blood. Median skin half-clearance time for skin in the LDS group was 2.2 min and in the control group 2.1 min. From the subcutaneous tissues, the respective times were 14.1 and 17.4 minutes. These differences are not statistically significant. The study fails to yield evidence suggesting that an oxygen diffusion barrier exists in lipodermatosclerosis.
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Affiliation(s)
- T R Cheatle
- Department of Surgery, University College and Middlesex School of Medicine, Middlesex Hospital, London
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3
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Abstract
Treatment of venous insufficiency and venous ulceration has for many years relied on established principles of compression and limb elevation. Drug treatment has been of little benefit. In recent years, a better understanding of the pathological mechanisms underlying skin damage in venous disease has allowed more rational pharmacotherapeutic approaches to be made. This review examines these, with special reference to current theories of the cause of venous ulceration.
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Affiliation(s)
- T R Cheatle
- University College and Middlesex School of Medicine, Middlesex Hospital, London
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4
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Matusik MR, Smith PD. Ongoing design concerns of portable oxygen cylinders. Anaesth Intensive Care 2018; 46:136-137. [PMID: 29361263] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 06/07/2023]
Affiliation(s)
| | - P D Smith
- Fellow of the Royal Australasian College of Surgeons
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5
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Gulden TD, Nickel H, Weber GW, Beatty RL, Tennery VJ, Lackey WJ, Stinton DP, Sease JD, Huschka H, Vygen P, Allen PL, Ford LH, Shennan JV, Linke J, Koizlik K, Nickel H, Lefevre RLR, Price MST, Wallisch K, Koss P, Delle W, Koizlik K, Price MST, Wolfrum EA, Nickel H, Pollmann E, Pelissier J, Yust CS, Kaae JL, Krautwasser P, Nickel H, Price RJ, Morgan CS, Powell GL, Harmon DP, Scott CB, Bradley RA, Thiele BA, Kaae JL, Kaae JL, Bullock RE, Scott CB, Harmon DP, Bongartz K, Strigl A, Proksch E, Wagner-Löffler M, Smith CL, Grübmeier H, Naoumidis A, Thiele BA, Homan FJ, Lindemer TB, Long EL, Tiegs TN, Beatty RL, Scott CB, Harmon DP, Morgan MT, Malinauskas AP, Stöver D, Hecker R, Smith PD, Steinke RG, Jensen DD, Hama T, Nabielek H, Brown PE, Offermann P, Pointud ML, Chenebault P, Myers BF, Baldwin NL, Bel WE, Groos E, Mielken G, Duwe R, Müller A, Will M, Röllig K, Hollabaugh CM, Wahman LA, Reiswig RD, White RW, Wagner P, Kaae JL, Sterling SA, Yang L, Förthmann R, Grübmeier H, Stöver D, katscher W, Nickel H, Gulden TD. Authors. NUCL TECHNOL 2017. [DOI: 10.13182/nt77-a31878] [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: 11/12/2022]
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6
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Affiliation(s)
- P. D. Smith
- General Atomic Company, P. O. Box 81608 San Diego, California 92138
| | - R. G. Steinke
- General Atomic Company, P. O. Box 81608 San Diego, California 92138
| | - D. D. Jensen
- General Atomic Company, P. O. Box 81608 San Diego, California 92138
| | - T. Hama
- Electric Power Company, Limited Tokyo, Japan
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Daggett JD, Watt AW, Smith PD. Chyle leak following right axillary lymph node dissection: A case report and review of current literature. Int J Surg Case Rep 2016; 20:68-73. [PMID: 26826928 PMCID: PMC4818284 DOI: 10.1016/j.ijscr.2015.12.044] [Citation(s) in RCA: 16] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/07/2015] [Revised: 12/23/2015] [Accepted: 12/25/2015] [Indexed: 01/15/2023] Open
Abstract
Chyle leak is an uncommon complication of axillary node dissection. The majority of reported cases occur on the left side, however several instances of right sided chyle leaks are reported. The majority of chyle leaks respond to conservative management with: diet modification, pressure and drainage. Diagnosis is based on clinical appearance for drainage, laboratory evaluation and lymphscintigraphy.
This report discusses the case of a chyle leak following a right axillary lymph node dissection for breast cancer. This presented as a sudden change in drainage character from a right axillary surgical drain from serous to milky white shortly after restarting a diet. The diagnosis of chyle leak was confirmed by laboratory testing of the fluid and managed with closed suction drainage. Chyle leak is a rare, but increasingly recognized complication following axillary clearance for breast cancer and melanoma.
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Affiliation(s)
- J D Daggett
- Division of Plastic Surgery, Department of Surgery, University of South Florida, Tampa, FL, USA.
| | - A W Watt
- Division of Plastic Surgery, Department of Surgery, University of South Florida, Tampa, FL, USA
| | - P D Smith
- Division of Plastic Surgery, Moffitt Cancer Center, Tampa, FL, USA
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Beloueche-Babari M, Jamin Y, Arunan V, Walker-Samuel S, Revill M, Smith PD, Halliday J, Waterton JC, Barjat H, Workman P, Leach MO, Robinson SP. Acute tumour response to the MEK1/2 inhibitor selumetinib (AZD6244, ARRY-142886) evaluated by non-invasive diffusion-weighted MRI. Br J Cancer 2013; 109:1562-9. [PMID: 23942066 PMCID: PMC3776979 DOI: 10.1038/bjc.2013.456] [Citation(s) in RCA: 22] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/25/2013] [Revised: 07/17/2013] [Accepted: 07/22/2013] [Indexed: 12/20/2022] Open
Abstract
BACKGROUND Non-invasive imaging biomarkers underpin the development of molecularly targeted anti-cancer drugs. This study evaluates tumour apparent diffusion coefficient (ADC), measured by diffusion-weighted magnetic resonance imaging (DW-MRI), as a biomarker of response to the MEK1/2 inhibitor selumetinib (AZD6244, ARRY-142886) in human tumour xenografts. METHODS Nude mice bearing human BRAF(V600D) WM266.4 melanoma or BRAF(V600E) Colo205 colon carcinoma xenografts were treated for 4 days with vehicle or selumetinib. DW-MRI was performed before and 2 h after the last dose and excised tumours analysed for levels of phospho-ERK1/2, cleaved caspase 3 (CC3) and necrosis. RESULTS Selumetinib treatment induced tumour stasis and reduced ERK1/2 phosphorylation in both WM266.4 and Colo205 tumour xenografts. Relative to day 0, mean tumour ADC was unchanged in the control groups but was significantly increased by up to 1.6-fold in selumetinib-treated WM266.4 and Colo205 tumours. Histological analysis revealed a significant increase in necrosis in selumetinib-treated WM266.4 and Colo205 xenografts and CC3 staining in selumetinib-treated Colo205 tumours relative to controls. CONCLUSION Changes in ADC following treatment with the MEK1/2 inhibitor selumetinib in responsive human tumour xenografts were concomitant with induction of tumour cell death. ADC may provide a useful non-invasive pharmacodynamic biomarker for early clinical assessment of response to selumetinib and other MEK-ERK1/2 signalling-targeted therapies.
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Affiliation(s)
- M Beloueche-Babari
- Cancer Research UK and EPSRC Cancer Imaging Centre, Division of Radiotherapy and Imaging, The Institute of Cancer Research and The Royal Marsden NHS Foundation Trust, Sutton, Surrey SM2 5PT, UK
| | - Y Jamin
- Cancer Research UK and EPSRC Cancer Imaging Centre, Division of Radiotherapy and Imaging, The Institute of Cancer Research and The Royal Marsden NHS Foundation Trust, Sutton, Surrey SM2 5PT, UK
| | - V Arunan
- Cancer Research UK and EPSRC Cancer Imaging Centre, Division of Radiotherapy and Imaging, The Institute of Cancer Research and The Royal Marsden NHS Foundation Trust, Sutton, Surrey SM2 5PT, UK
| | - S Walker-Samuel
- Cancer Research UK and EPSRC Cancer Imaging Centre, Division of Radiotherapy and Imaging, The Institute of Cancer Research and The Royal Marsden NHS Foundation Trust, Sutton, Surrey SM2 5PT, UK
| | - M Revill
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
| | - P D Smith
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
| | - J Halliday
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
| | - J C Waterton
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
| | - H Barjat
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
| | - P Workman
- Cancer Research UK Cancer Therapeutics Unit, Division of Cancer Therapeutics, The Institute of Cancer Research, Sutton, Surrey SM2 5NG, UK
| | - M O Leach
- Cancer Research UK and EPSRC Cancer Imaging Centre, Division of Radiotherapy and Imaging, The Institute of Cancer Research and The Royal Marsden NHS Foundation Trust, Sutton, Surrey SM2 5PT, UK
| | - S P Robinson
- Cancer Research UK and EPSRC Cancer Imaging Centre, Division of Radiotherapy and Imaging, The Institute of Cancer Research and The Royal Marsden NHS Foundation Trust, Sutton, Surrey SM2 5PT, UK
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10
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Little AS, Smith PD, Cook SJ. Mechanisms of acquired resistance to ERK1/2 pathway inhibitors. Oncogene 2013; 32:1207-15. [PMID: 22562245 DOI: 10.1038/onc.2012.160] [Citation(s) in RCA: 83] [Impact Index Per Article: 7.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/22/2012] [Revised: 04/03/2012] [Accepted: 04/03/2012] [Indexed: 12/24/2022]
Abstract
The ERK1/2 (extracellular signal-regulated kinase 1 and 2) pathway, comprising the protein kinases RAF (v-raf-1 murine leukemia viral oncogene homolog 1), MEK1/2 (mitogen-activated protein kinase or ERK kinase 1 and 2) and ERK1/2 is frequently de-regulated in human cancers, due to mutations in RAS or BRAF (v-raf-1 murine leukemia viral oncogene homolog B1). New, highly selective inhibitors of BRAF and MEK1/2 have shown promise in clinical trials, including in previously intractable diseases such as melanoma. However, drug-resistant tumour cells invariably emerge leading to disease progression. It is important to understand the mechanisms underlying such acquired resistance since this may lead to the development of rational strategies either to delay its onset or to overcome it once established. It also offers unique insights into the plasticity of signalling pathways, which may in turn inform our understanding of the basic biology of these pathways and lead to the validation of new drug targets. Several recent reports have identified diverse mechanisms of acquired resistance to MEK1/2 or BRAF inhibitors. In this article, we review these studies, discuss the different mechanisms, identify common themes and consider their therapeutic implications.
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Affiliation(s)
- A S Little
- Signalling Laboratory, The Babraham Institute, Babraham Research Campus, Cambridge, UK
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11
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Doren EL, Smith PD, Sun W, Lacevic M, Fulp W, Reid R, Laronga C. Abstract P4-14-09: Feasibility of liposuction for treatment of arm lymphedema from breast cancer. Cancer Res 2012. [DOI: 10.1158/0008-5472.sabcs12-p4-14-09] [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: 11/16/2022]
Abstract
Abstract
Background: Lymphedema is a dreaded complication of breast cancer treatment affecting 20% of women having axillary node dissection. Liposuction minimizes unwanted fat in targeted areas. Our objective was to explore the feasibility of liposuction to reduce fat volume and thus arm lymphedema.
Methods: An IRB-approved prospective trial was conducted of women having unilateral arm lymphedema resulting from breast cancer treatment. At enrollment there was no evidence of cancer recurrence or arm cellulitis. Arm measurements (circumferential), volumes (water displacement and geometric calculation), and muscle strength differences between the affected and unaffected arms and quality of life/functionality were measured pre-operatively and post-operatively at 6 weeks, 6 months and one year(s). Descriptive statistical analysis was performed.
Results: Six breast cancer survivors underwent the liposuction procedure from 12/2008–4/2011. Median age was 54 yrs (range: 43–60) and median volume of fat aspirated was 700mls (range: 350–700). Average volume difference between the affected and unaffected arms at baseline was 522.5 mls (176–867) (geometric) and 589.2mls (280–770) (water displacement). No immediate complications; 1 cellulitis at 4 months post-operative. Average percent volume reductions for 5 of the 6 women at 6 weeks, 6 months and 1 year were 70%, 47%, 71% mls geometrically and 63%, 18%, 54% by water displacement respectively. Quality of life and functionality improved in all patients. Muscle strength remained unchanged. Pain lessened. Average follow-up is 15.49 months (range: 1.8–24.84 months).
Conclusion: Liposuction can safely reduce volume of arm lymphedema and improve functionality/quality of life. Larger studies (longer follow-up) are required to validate the durability of these early results.
Citation Information: Cancer Res 2012;72(24 Suppl):Abstract nr P4-14-09.
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Affiliation(s)
- EL Doren
- University of South Florida, Tampa, FL; Moffitt Cancer Center, Tampa, FL
| | - PD Smith
- University of South Florida, Tampa, FL; Moffitt Cancer Center, Tampa, FL
| | - W Sun
- University of South Florida, Tampa, FL; Moffitt Cancer Center, Tampa, FL
| | - M Lacevic
- University of South Florida, Tampa, FL; Moffitt Cancer Center, Tampa, FL
| | - W Fulp
- University of South Florida, Tampa, FL; Moffitt Cancer Center, Tampa, FL
| | - R Reid
- University of South Florida, Tampa, FL; Moffitt Cancer Center, Tampa, FL
| | - C Laronga
- University of South Florida, Tampa, FL; Moffitt Cancer Center, Tampa, FL
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12
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Lopez JJ, Laronga C, Doren EL, Sun W, Fulp WJ, Smith PD. Abstract P4-17-01: The effect of body mass index on breast reconstruction outcomes. Cancer Res 2012. [DOI: 10.1158/0008-5472.sabcs12-p4-17-01] [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: 11/16/2022]
Abstract
Abstract
Introduction: With increasing numbers of women choosing mastectomy for breast cancer treatment, breast reconstruction is consequentially on the rise. Obesity, a known predictor for wound healing complications, is also on the rise. Our objective is to review our institutional experience with the association between Body Mass Index (BMI) and breast reconstruction complications.
Methods: An IRB approved retrospective review of prospectively gathered patients having mastectomy with reconstruction was conducted. Data including patient demographics, stage at diagnosis, adjuvant treatment, type of mastectomy, type of reconstruction, and complications were collected. Patients were stratified by BMI into two categories: Normal weight (BMI 18.5–24.9), and overweight/obese (BMI 25 or greater). The statistical analysis was preformed using Wilcoxon Rank-Sum Test and Chi Squared Test, both using exact method with Monte Carlo estimation.
Results: From 06/1996 to 08/2011, 443 patients were identified having mastectomy and reconstruction. Of these, 218 patients had a normal weight at the time of mastectomy; 225 patients were overweight/obese. The overall median age was 49 years (range: 18–82). 780 mastectomies with reconstruction (106 unilateral, 337 bilateral) were performed. The most common reconstruction types included 477 tissue expander with implant reconstructions (62.8% of breasts), 106 latissimus flap with prosthesis (14.0%), and 103 pedicled TRAM flaps (13.6%). 245 patients (55.3%) experienced at least one complication; the most common complications were fat necrosis (80 patients, 18.1% of patients), infection (57, 12.9%), epidermolysis (41, 9.3%), and skin necrosis (39, 8.8%).
The overweight/obese group had a significantly higher prevalence of diabetes (6.3% vs. 0.9%, p = 0.0036) and hypertension (26.7% vs. 11.1%, p < 0.0001) and was more likely to receive neoadjuvant chemotherapy (16.2% vs. 4.8% p = 0.0005), possibly due to presentation at a later stage, but no significant differences were identified. Other comorbid conditions, including smoking, history of breast cancer, adjuvant chemotherapy, and history of or postsurgical radiation, were similar between the two groups. One significant difference was that the overweight/obese group was significantly older than the normal weight group (p = 0.0005).
There were no significant differences identified in the incidence of any individual complication between the two BMI groups. Additionally, the incidence of a patient having any complication was similar between the two groups (128 overweight/obese patients for 56.9% and 117 normal weight patients for 53.7%, p = 0.4918). When using breasts instead of patients as the unit of measure, when an overweight/obese patient had a complication they were significantly more likely to require an unanticipated return to the OR (93/160 breasts with a complication for 58.1% vs. 67/154 for 43.5%, p = 0.0124).
Conclusion: Obesity does not increase the risk of breast reconstruction complications, but increases the severity of complications if one should arise. This supports the continued use of breast reconstruction in patients regardless of their weight, and emphasizes that when the correct procedure is selected for an overweight/obese patient, outcomes can be similar to patients that are of a normal weight.
Citation Information: Cancer Res 2012;72(24 Suppl):Abstract nr P4-17-01.
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Affiliation(s)
- JJ Lopez
- University of South Florida, Tampa, FL; H. Lee Moffitt Cancer Center, Tampa, FL
| | - C Laronga
- University of South Florida, Tampa, FL; H. Lee Moffitt Cancer Center, Tampa, FL
| | - EL Doren
- University of South Florida, Tampa, FL; H. Lee Moffitt Cancer Center, Tampa, FL
| | - W Sun
- University of South Florida, Tampa, FL; H. Lee Moffitt Cancer Center, Tampa, FL
| | - WJ Fulp
- University of South Florida, Tampa, FL; H. Lee Moffitt Cancer Center, Tampa, FL
| | - PD Smith
- University of South Florida, Tampa, FL; H. Lee Moffitt Cancer Center, Tampa, FL
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Freire PCC, Abdo AA, Ajello M, Allafort A, Ballet J, Barbiellini G, Bastieri D, Bechtol K, Bellazzini R, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Brigida M, Bruel P, Buehler R, Buson S, Caliandro GA, Cameron RA, Camilo F, Caraveo PA, Cecchi C, Çelik Ö, Charles E, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cognard I, Cohen-Tanugi J, Cominsky LR, de Palma F, Dermer CD, do Couto e Silva E, Dormody M, Drell PS, Dubois R, Dumora D, Espinoza CM, Favuzzi C, Fegan SJ, Ferrara EC, Focke WB, Fortin P, Fukazawa Y, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giglietto N, Giordano F, Giroletti M, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Hadasch D, Harding AK, Jóhannesson G, Johnson AS, Johnson TJ, Johnston S, Katagiri H, Kataoka J, Keith M, Kerr M, Knödlseder J, Kramer M, Kuss M, Lande J, Latronico L, Lee SH, Lemoine-Goumard M, Longo F, Loparco F, Lovellette MN, Lubrano P, Lyne AG, Manchester RN, Marelli M, Mazziotta MN, McEnery JE, Michelson PF, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Nolan PL, Norris JP, Nuss E, Ohsugi T, Okumura A, Omodei N, Orlando E, Ozaki M, Paneque D, Parent D, Pesce-Rollins M, Pierbattista M, Piron F, Porter TA, Rainò S, Ransom SM, Ray PS, Reimer A, Reimer O, Reposeur T, Ritz S, Romani RW, Roth M, Sadrozinski HFW, Parkinson PMS, Sgrò C, Shannon R, Siskind EJ, Smith DA, Smith PD, Spinelli P, Stappers BW, Suson DJ, Takahashi H, Tanaka T, Tauris TM, Thayer JB, Theureau G, Thompson DJ, Thorsett SE, Tibaldo L, Torres DF, Tosti G, Troja E, Vandenbroucke J, Van Etten A, Vasileiou V, Venter C, Vianello G, Vilchez N, Vitale V, Waite AP, Wang P, Wood KS, Yang Z, Ziegler M, Zimmer S. Fermi Detection of a Luminous γ-Ray Pulsar in a Globular Cluster. Science 2011; 334:1107-10. [PMID: 22052973 DOI: 10.1126/science.1207141] [Citation(s) in RCA: 56] [Impact Index Per Article: 4.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Affiliation(s)
| | - P. C. C. Freire
- Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
| | - A. A. Abdo
- Center for Earth Observing and Space Research, College of Science, George Mason University, Fairfax, VA 22030, USA
| | - M. Ajello
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Allafort
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. Ballet
- Laboratoire AIM (Astrophysique, Instrumentation et Modélisation), CEA-IRFU/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - G. Barbiellini
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - D. Bastieri
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I-35131 Padova, Italy
| | - K. Bechtol
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. Bellazzini
- Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy
| | - R. D. Blandford
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. D. Bloom
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. Bonamente
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - A. W. Borgland
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Brigida
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - P. Bruel
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/IN2P3, Palaiseau, France
| | - R. Buehler
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Buson
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I-35131 Padova, Italy
| | - G. A. Caliandro
- Institut de Ciències de l’Espai (IEEE-CSIC), Campus UAB, 08193 Barcelona, Spain
| | - R. A. Cameron
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - F. Camilo
- Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA
| | - P. A. Caraveo
- INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica, I-20133 Milano, Italy
| | - C. Cecchi
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - Ö. Çelik
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Department of Physics and Center for Space Sciences and Technology, University of Maryland Baltimore County, Baltimore, MD 21250, USA
| | - E. Charles
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Chekhtman
- Artep Inc., 2922 Excelsior Springs Court, Ellicott City, MD 21042, USA
| | - C. C. Cheung
- National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001, USA
| | - J. Chiang
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Ciprini
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
- Agenzia Spaziale Italiana (ASI) Science Data Center, I-00044 Frascati (Roma), Italy
| | - R. Claus
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - I. Cognard
- Laboratoire de Physique et Chimie de l’Environnement, LPCE UMR 6115 CNRS, F-45071 Orléans Cedex 02, and Station de radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, F-18330 Nançay, France
| | - J. Cohen-Tanugi
- Laboratoire Univers et Particules de Montpellier, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - L. R. Cominsky
- Department of Physics and Astronomy, Sonoma State University, Rohnert Park, CA 94928–3609, USA
| | - F. de Palma
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - C. D. Dermer
- Space Science Division, Naval Research Laboratory, Washington, DC 20375–5352, USA
| | - E. do Couto e Silva
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Dormody
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - P. S. Drell
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. Dubois
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - D. Dumora
- Université Bordeaux 1, CNRS/IN2p3, Centre d’Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France
| | - C. M. Espinoza
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, M13 9PL, UK
| | - C. Favuzzi
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - S. J. Fegan
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/IN2P3, Palaiseau, France
| | - E. C. Ferrara
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - W. B. Focke
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Fortin
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/IN2P3, Palaiseau, France
| | - Y. Fukazawa
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - P. Fusco
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - F. Gargano
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - D. Gasparrini
- ASI Science Data Center, I-00044 Frascati (Roma), Italy
| | - N. Gehrels
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - S. Germani
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - N. Giglietto
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - F. Giordano
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - M. Giroletti
- INAF Istituto di Radioastronomia, 40129 Bologna, Italy
| | - T. Glanzman
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - G. Godfrey
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - I. A. Grenier
- Laboratoire AIM (Astrophysique, Instrumentation et Modélisation), CEA-IRFU/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - M.-H. Grondin
- Max-Planck-Institut für Kernphysik, D-69029 Heidelberg, Germany
- Landessternwarte, Universität Heidelberg, Königstuhl, D 69117 Heidelberg, Germany
| | - J. E. Grove
- Space Science Division, Naval Research Laboratory, Washington, DC 20375–5352, USA
| | - L. Guillemot
- Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
| | - S. Guiriec
- Center for Space Plasma and Aeronomic Research (CSPAR), University of Alabama in Huntsville, Huntsville, AL 35899, USA
| | - D. Hadasch
- Institut de Ciències de l’Espai (IEEE-CSIC), Campus UAB, 08193 Barcelona, Spain
| | - A. K. Harding
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - G. Jóhannesson
- Science Institute, University of Iceland, IS-107 Reykjavik, Iceland
| | - A. S. Johnson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. J. Johnson
- Center for Earth Observing and Space Research, College of Science, George Mason University, Fairfax, VA 22030, USA
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001, USA
- Department of Physics and Department of Astronomy, University of Maryland, College Park, MD 20742, USA
| | - S. Johnston
- Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping NSW 1710, Australia
| | - H. Katagiri
- College of Science, Ibaraki University, 2-1-1, Bunkyo, Mito 310-8512, Japan
| | - J. Kataoka
- Research Institute for Science and Engineering, Waseda University, 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan
| | - M. Keith
- Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping NSW 1710, Australia
| | - M. Kerr
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. Knödlseder
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- CNRS, Research Institute in Astrophysics and Planetology (IRAP), F-31028 Toulouse cedex 4, France
| | - M. Kramer
- Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, M13 9PL, UK
| | - M. Kuss
- Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy
| | - J. Lande
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - L. Latronico
- Istituto Nazionale di Fisica Nucleare, Sezioine di Torino, I-10125 Torino, Italy
| | - S.-H. Lee
- Yukawa Institute for Theoretical Physics, Kyoto University, Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto 606-8502, Japan
| | - M. Lemoine-Goumard
- Université Bordeaux 1, CNRS/IN2p3, Centre d’Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France
| | - F. Longo
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - F. Loparco
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - M. N. Lovellette
- Space Science Division, Naval Research Laboratory, Washington, DC 20375–5352, USA
| | - P. Lubrano
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - A. G. Lyne
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, M13 9PL, UK
| | - R. N. Manchester
- Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping NSW 1710, Australia
| | - M. Marelli
- INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica, I-20133 Milano, Italy
| | - M. N. Mazziotta
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - J. E. McEnery
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Department of Physics and Department of Astronomy, University of Maryland, College Park, MD 20742, USA
| | - P. F. Michelson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. Mizuno
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - A. A. Moiseev
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Department of Physics and Department of Astronomy, University of Maryland, College Park, MD 20742, USA
| | - C. Monte
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - M. E. Monzani
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Morselli
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma “Tor Vergata,” I-00133 Roma, Italy
| | - I. V. Moskalenko
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Murgia
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. Nakamori
- Research Institute for Science and Engineering, Waseda University, 3-4-1, Okubo, Shinjuku, Tokyo 169-8555, Japan
| | - P. L. Nolan
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. P. Norris
- Department of Physics, Boise State University, Boise, ID 83725, USA
| | - E. Nuss
- Laboratoire Univers et Particules de Montpellier, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - T. Ohsugi
- Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - A. Okumura
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan
| | - N. Omodei
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. Orlando
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Max-Planck-Institut für Extraterrestrische Physik, 85748 Garching, Germany
| | - M. Ozaki
- Institute of Space and Astronautical Science, JAXA, 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan
| | - D. Paneque
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Max-Planck-Institut für Physik, D-80805 München, Germany
| | - D. Parent
- Center for Earth Observing and Space Research, College of Science, George Mason University, Fairfax, VA 22030, USA
| | - M. Pesce-Rollins
- Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy
| | - M. Pierbattista
- Laboratoire AIM (Astrophysique, Instrumentation et Modélisation), CEA-IRFU/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - F. Piron
- Laboratoire Univers et Particules de Montpellier, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - T. A. Porter
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Rainò
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - S. M. Ransom
- National Radio Astronomy Observatory (NRAO), Charlottesville, VA 22903, USA
| | - P. S. Ray
- Space Science Division, Naval Research Laboratory, Washington, DC 20375–5352, USA
| | - A. Reimer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A-6020 Innsbruck, Austria
| | - O. Reimer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A-6020 Innsbruck, Austria
| | - T. Reposeur
- Université Bordeaux 1, CNRS/IN2p3, Centre d’Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France
| | - S. Ritz
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - R. W. Romani
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Roth
- Department of Physics, University of Washington, Seattle, WA 98195–1560, USA
| | - H. F.-W. Sadrozinski
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - P. M. Saz Parkinson
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - C. Sgrò
- Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, I-56127 Pisa, Italy
| | - R. Shannon
- Commonwealth Scientific and Industrial Research Organisation, Astronomy and Space Science, Australia Telescope National Facility, Epping NSW 1710, Australia
| | - E. J. Siskind
- NYCB Real-Time Computing Inc., Lattingtown, NY 11560–1025, USA
| | - D. A. Smith
- Université Bordeaux 1, CNRS/IN2p3, Centre d’Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France
| | - P. D. Smith
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - P. Spinelli
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - B. W. Stappers
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, M13 9PL, UK
| | - D. J. Suson
- Department of Chemistry and Physics, Purdue University Calumet, Hammond, IN 46323-2094, USA
| | - H. Takahashi
- Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - T. Tanaka
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. M. Tauris
- Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
- Argelander-Institut für Astronomie, Universität Bonn, 53121 Bonn, Germany
| | - J. B. Thayer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - G. Theureau
- Laboratoire de Physique et Chimie de l’Environnement, LPCE UMR 6115 CNRS, F-45071 Orléans Cedex 02, and Station de radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, F-18330 Nançay, France
| | - D. J. Thompson
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - S. E. Thorsett
- Department of Physics, Willamette University, Salem, OR 97031, USA
| | - L. Tibaldo
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I-35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I-35131 Padova, Italy
| | - D. F. Torres
- Institut de Ciències de l’Espai (IEEE-CSIC), Campus UAB, 08193 Barcelona, Spain
- Institució Catalana de Recerca i Estudis Avançats (ICREA), Barcelona, Spain
| | - G. Tosti
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - E. Troja
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - J. Vandenbroucke
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Van Etten
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - V. Vasileiou
- Laboratoire Univers et Particules de Montpellier, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - C. Venter
- Centre for Space Research, North-West University, Potchefstroom Campus, Private Bag X6001, 2520 Potchefstroom, South Africa
| | - G. Vianello
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Consorzio Interuniversitario per la Fisica Spaziale (CIFS), I-10133 Torino, Italy
| | - N. Vilchez
- CNRS, Research Institute in Astrophysics and Planetology (IRAP), F-31028 Toulouse cedex 4, France
- Galaxies, Astrophysique des Hautes Energies et Cosmologie, Université de Toulouse, UPS-OMP, IRAP, Toulouse, France
| | - V. Vitale
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma “Tor Vergata,” I-00133 Roma, Italy
- Dipartimento di Fisica, Università di Roma “Tor Vergata,” I-00133 Roma, Italy
| | - A. P. Waite
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Wang
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - K. S. Wood
- Space Science Division, Naval Research Laboratory, Washington, DC 20375–5352, USA
| | - Z. Yang
- Department of Physics, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE-106 91 Stockholm, Sweden
| | - M. Ziegler
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - S. Zimmer
- Department of Physics, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE-106 91 Stockholm, Sweden
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Ackermann M, Ajello M, Allafort A, Baldini L, Ballet J, Barbiellini G, Bastieri D, Belfiore A, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bottacini E, Brigida M, Bruel P, Buehler R, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cecchi C, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, de Angelis A, de Palma F, Dermer CD, do Couto e Silva E, Drell PS, Dumora D, Favuzzi C, Fegan SJ, Focke WB, Fortin P, Fukazawa Y, Fusco P, Gargano F, Germani S, Giglietto N, Giordano F, Giroletti M, Glanzman T, Godfrey G, Grenier IA, Guillemot L, Guiriec S, Hadasch D, Hanabata Y, Harding AK, Hayashida M, Hayashi K, Hays E, Johannesson G, Johnson AS, Kamae T, Katagiri H, Kataoka J, Kerr M, Knodlseder J, Kuss M, Lande J, Latronico L, Lee SH, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Martin P, Mazziotta MN, McEnery JE, Mehault J, Michelson PF, Mitthumsiri W, Mizuno T, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Naumann-Godo M, Nolan PL, Norris JP, Nuss E, Ohsugi T, Okumura A, Orlando E, Ormes JF, Ozaki M, Paneque D, Parent D, Pesce-Rollins M, Pierbattista M, Piron F, Pohl M, Prokhorov D, Raino S, Rando R, Razzano M, Reposeur T, Ritz S, Parkinson PMS, Sgro C, Siskind EJ, Smith PD, Spinelli P, Strong AW, Takahashi H, Tanaka T, Thayer JG, Thayer JB, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Tramacere A, Troja E, Uchiyama Y, Vandenbroucke J, Vasileiou V, Vianello G, Vitale V, Waite AP, Wang P, Winer BL, Wood KS, Yang Z, Zimmer S, Bontemps S. A Cocoon of Freshly Accelerated Cosmic Rays Detected by Fermi in the Cygnus Superbubble. Science 2011; 334:1103-7. [DOI: 10.1126/science.1210311] [Citation(s) in RCA: 180] [Impact Index Per Article: 13.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
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Baran SD, Lapin JA, Beasley JW, Smith PD, Karsh BT. Identifying Hazards in Primary Care: The Elderly Patient's Perspective. ACTA ACUST UNITED AC 2011. [DOI: 10.1177/1071181311551236] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/15/2022]
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Ajello M, Atwood WB, Baldini L, Barbiellini G, Bastieri D, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bottacini E, Bouvier A, Bregeon J, Brigida M, Bruel P, Buehler R, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Cecchi C, Charles E, Chekhtman A, Ciprini S, Claus R, Cohen-Tanugi J, Cutini S, de Angelis A, de Palma F, Dermer CD, Digel SW, do Couto e Silva E, Drell PS, Favuzzi C, Fegan SJ, Focke WB, Fukazawa Y, Fusco P, Gargano F, Gehrels N, Germani S, Giglietto N, Giordano F, Giroletti M, Glanzman T, Godfrey G, Grenier IA, Guiriec S, Gustafsson M, Hadasch D, Iafrate G, Jóhannesson G, Johnson AS, Kamae T, Katagiri H, Kataoka J, Kuss M, Latronico L, Lionetto AM, Longo F, Loparco F, Lovellette MN, Lubrano P, Mazziotta MN, McEnery JE, Michelson PF, Mizuno T, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Naumann-Godo M, Norris JP, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Ozaki M, Paneque D, Panetta JH, Pesce-Rollins M, Pierbattista M, Piron F, Rainò S, Rando R, Razzano M, Reimer A, Reimer O, Ritz S, Schalk TL, Sgrò C, Siegal-Gaskins J, Siskind EJ, Smith PD, Spandre G, Spinelli P, Suson DJ, Takahashi H, Tanaka T, Thayer JG, Thayer JB, Tibaldo L, Tosti G, Troja E, Usher TL, Vandenbroucke J, Vasileiou V, Vianello G, Vilchez N, Waite AP, Wang P, Winer BL, Wood KS, Yang Z, Zimmer S. Constraints on dark matter models from a Fermi LAT search for high-energy cosmic-ray electrons from the Sun. Int J Clin Exp Med 2011. [DOI: 10.1103/physrevd.84.032007] [Citation(s) in RCA: 27] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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Tolcher AW, Baird RD, Patnaik A, Moreno Garcia V, Papadopoulos KP, Garrett CR, Olmos D, Shannon KA, Zazulina V, Rubin EH, Smith IC, Ryan J, Smith PD, Taylor A, Learoyd M, Lupinacci L, Yan L, De Bono JS. A phase I dose-escalation study of oral MK-2206 (allosteric AKT inhibitor) with oral selumetinib (AZD6244; MEK inhibitor) in patients with advanced or metastatic solid tumors. J Clin Oncol 2011. [DOI: 10.1200/jco.2011.29.15_suppl.3004] [Citation(s) in RCA: 26] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022] Open
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Abdo AA, Ackermann M, Ajello M, Allafort A, Baldini L, Ballet J, Barbiellini G, Bastieri D, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bouvier A, Brandt TJ, Bregeon J, Brez A, Brigida M, Bruel P, Buehler R, Buson S, Caliandro GA, Cameron RA, Cannon A, Caraveo PA, Casandjian JM, Çelik Ö, Charles E, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Costamante L, Cutini S, D’Ammando F, Dermer CD, de Angelis A, de Luca A, de Palma F, Digel SW, do Couto e Silva E, Drell PS, Drlica-Wagner A, Dubois R, Dumora D, Favuzzi C, Fegan SJ, Ferrara EC, Focke WB, Fortin P, Frailis M, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giglietto N, Giordano F, Giroletti M, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guiriec S, Hadasch D, Hanabata Y, Harding AK, Hayashi K, Hayashida M, Hays E, Horan D, Itoh R, Jóhannesson G, Johnson AS, Johnson TJ, Khangulyan D, Kamae T, Katagiri H, Kataoka J, Kerr M, Knödlseder J, Kuss M, Lande J, Latronico L, Lee SH, Lemoine-Goumard M, Longo F, Loparco F, Lubrano P, Madejski GM, Makeev A, Marelli M, Mazziotta MN, McEnery JE, Michelson PF, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Naumann-Godo M, Nolan PL, Norris JP, Nuss E, Ohsugi T, Okumura A, Omodei N, Ormes JF, Ozaki M, Paneque D, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Pierbattista M, Piron F, Porter TA, Rainò S, Rando R, Ray PS, Razzano M, Reimer A, Reimer O, Reposeur T, Ritz S, Romani RW, Sadrozinski HFW, Sanchez D, Parkinson PMS, Scargle JD, Schalk TL, Sgrò C, Siskind EJ, Smith PD, Spandre G, Spinelli P, Strickman MS, Suson DJ, Takahashi H, Takahashi T, Tanaka T, Thayer JB, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Tramacere A, Troja E, Uchiyama Y, Vandenbroucke J, Vasileiou V, Vianello G, Vitale V, Wang P, Wood KS, Yang Z, Ziegler M. Gamma-Ray Flares from the Crab Nebula. Science 2011; 331:739-42. [DOI: 10.1126/science.1199705] [Citation(s) in RCA: 265] [Impact Index Per Article: 20.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Affiliation(s)
- A. A. Abdo
- National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001, USA; Naval Research Laboratory, Washington, DC 20375, USA
| | - M. Ackermann
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Ajello
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Allafort
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - L. Baldini
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - J. Ballet
- Laboratoire AIM, Commissariat à l’Énergie Atomique (CEA)– Institute of Research into the Fundamental Laws of the Universe (IRFU)/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - G. Barbiellini
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - D. Bastieri
- INFN, Sezione di Padova, I-35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I-35131 Padova, Italy
| | - K. Bechtol
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. Bellazzini
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - B. Berenji
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. D. Blandford
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. D. Bloom
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. Bonamente
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - A. W. Borgland
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Bouvier
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. J. Brandt
- Centre d’Étude Spatiale des Rayonnements, CNRS/UPS, BP 44346, F-30128 Toulouse Cedex 4, France
- Department of Physics, Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, USA
| | - J. Bregeon
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - A. Brez
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - M. Brigida
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - P. Bruel
- Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3, Palaiseau, France
| | - R. Buehler
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Buson
- INFN, Sezione di Padova, I-35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I-35131 Padova, Italy
| | - G. A. Caliandro
- Institut de Ciencies de l’Espai, Institut d’Estudis Espacials de Catalunya–Consejo Superior de Investigaciones Científicas (IEEC-CSIC), Campus UAB, 08193 Barcelona, Spain
| | - R. A. Cameron
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Cannon
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- School of Physics, University College Dublin, Belfield, Dublin 4, Ireland
| | - P. A. Caraveo
- Istituto Nazionale di Astrofisica–Istituto di Astrofisica Spaziale e Fisica Cosmica (INAF-IASF), I-20133 Milano, Italy
| | - J. M. Casandjian
- Laboratoire AIM, Commissariat à l’Énergie Atomique (CEA)– Institute of Research into the Fundamental Laws of the Universe (IRFU)/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - Ö. Çelik
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Department of Physics and Center for Space Sciences and Technology, University of Maryland Baltimore County, Baltimore, MD 21250, USA
| | - E. Charles
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Chekhtman
- College of Science, George Mason University, Fairfax, VA 22030, USA; Naval Research Laboratory, Washington, DC 20375, USA
| | - C. C. Cheung
- National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001, USA; Naval Research Laboratory, Washington, DC 20375, USA
| | - J. Chiang
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Ciprini
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - R. Claus
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. Cohen-Tanugi
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - L. Costamante
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Cutini
- Agenzia Spaziale Italiana (ASI) Science Data Center, I-00044 Frascati (Roma), Italy
| | - F. D’Ammando
- IASF Palermo, 90146 Palermo, Italy
- INAF-IASF, I-00133 Roma, Italy
| | - C. D. Dermer
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - A. de Angelis
- Dipartimento di Fisica, Università di Udine and Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Gruppo Collegato di Udine, I-33100 Udine, Italy
| | - A. de Luca
- Istituto Universitario di Studi Superiori (IUSS), I-27100 Pavia, Italy
| | - F. de Palma
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - S. W. Digel
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. do Couto e Silva
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. S. Drell
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Drlica-Wagner
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. Dubois
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - D. Dumora
- Université Bordeaux 1, CNRS/IN2p3, Centre d’Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France
| | - C. Favuzzi
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - S. J. Fegan
- Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3, Palaiseau, France
| | - E. C. Ferrara
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - W. B. Focke
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Fortin
- Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3, Palaiseau, France
| | - M. Frailis
- Dipartimento di Fisica, Università di Udine and Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Gruppo Collegato di Udine, I-33100 Udine, Italy
- Osservatorio Astronomico di Trieste, Istituto Nazionale di Astrofisica, I-34143 Trieste, Italy
| | - Y. Fukazawa
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - S. Funk
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Fusco
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - F. Gargano
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - D. Gasparrini
- Agenzia Spaziale Italiana (ASI) Science Data Center, I-00044 Frascati (Roma), Italy
| | - N. Gehrels
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - S. Germani
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - N. Giglietto
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - F. Giordano
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - M. Giroletti
- INAF–Istituto di Radioastronomia, 40129 Bologna, Italy
| | - T. Glanzman
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - G. Godfrey
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - I. A. Grenier
- Laboratoire AIM, Commissariat à l’Énergie Atomique (CEA)– Institute of Research into the Fundamental Laws of the Universe (IRFU)/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - M.-H. Grondin
- Université Bordeaux 1, CNRS/IN2p3, Centre d’Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France
| | - J. E. Grove
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - S. Guiriec
- Center for Space Plasma and Aeronomic Research (CSPAR), University of Alabama in Huntsville, Huntsville, AL 35899, USA
| | - D. Hadasch
- Institut de Ciencies de l’Espai, Institut d’Estudis Espacials de Catalunya–Consejo Superior de Investigaciones Científicas (IEEC-CSIC), Campus UAB, 08193 Barcelona, Spain
| | - Y. Hanabata
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - A. K. Harding
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - K. Hayashi
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - M. Hayashida
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. Hays
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - D. Horan
- Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3, Palaiseau, France
| | - R. Itoh
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - G. Jóhannesson
- Science Institute, University of Iceland, IS-107 Reykjavik, Iceland
| | - A. S. Johnson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. J. Johnson
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Department of Physics and Department of Astronomy, University of Maryland, College Park, MD 20742, USA
| | - D. Khangulyan
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan
| | - T. Kamae
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - H. Katagiri
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - J. Kataoka
- Research Institute for Science and Engineering, Waseda University, 3-4-1, Okubo, Shinjuku, Tokyo, 169-8555 Japan
| | - M. Kerr
- Department of Physics, University of Washington, Seattle, WA 98195–1560, USA
| | - J. Knödlseder
- Centre d’Étude Spatiale des Rayonnements, CNRS/UPS, BP 44346, F-30128 Toulouse Cedex 4, France
| | - M. Kuss
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - J. Lande
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - L. Latronico
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - S.-H. Lee
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Lemoine-Goumard
- Université Bordeaux 1, CNRS/IN2p3, Centre d’Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France
| | - F. Longo
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - F. Loparco
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - P. Lubrano
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - G. M. Madejski
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Makeev
- College of Science, George Mason University, Fairfax, VA 22030, USA; Naval Research Laboratory, Washington, DC 20375, USA
| | - M. Marelli
- Istituto Nazionale di Astrofisica–Istituto di Astrofisica Spaziale e Fisica Cosmica (INAF-IASF), I-20133 Milano, Italy
| | | | - J. E. McEnery
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Department of Physics and Department of Astronomy, University of Maryland, College Park, MD 20742, USA
| | - P. F. Michelson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - W. Mitthumsiri
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. Mizuno
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - A. A. Moiseev
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Department of Physics and Department of Astronomy, University of Maryland, College Park, MD 20742, USA
| | - C. Monte
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - M. E. Monzani
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Morselli
- INFN, Sezione di Roma “Tor Vergata,” I-00133 Roma, Italy
| | - I. V. Moskalenko
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Murgia
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. Nakamori
- Research Institute for Science and Engineering, Waseda University, 3-4-1, Okubo, Shinjuku, Tokyo, 169-8555 Japan
| | - M. Naumann-Godo
- Laboratoire AIM, Commissariat à l’Énergie Atomique (CEA)– Institute of Research into the Fundamental Laws of the Universe (IRFU)/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - P. L. Nolan
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. P. Norris
- Department of Physics and Astronomy, University of Denver, Denver, CO 80208, USA
| | - E. Nuss
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - T. Ohsugi
- Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - A. Okumura
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan
| | - N. Omodei
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. F. Ormes
- Department of Physics and Astronomy, University of Denver, Denver, CO 80208, USA
| | - M. Ozaki
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan
| | - D. Paneque
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - D. Parent
- College of Science, George Mason University, Fairfax, VA 22030, USA; Naval Research Laboratory, Washington, DC 20375, USA
| | - V. Pelassa
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - M. Pepe
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - M. Pesce-Rollins
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - M. Pierbattista
- Laboratoire AIM, Commissariat à l’Énergie Atomique (CEA)– Institute of Research into the Fundamental Laws of the Universe (IRFU)/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - F. Piron
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - T. A. Porter
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Rainò
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - R. Rando
- INFN, Sezione di Padova, I-35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I-35131 Padova, Italy
| | - P. S. Ray
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - M. Razzano
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - A. Reimer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A-6020 Innsbruck, Austria
| | - O. Reimer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A-6020 Innsbruck, Austria
| | - T. Reposeur
- Université Bordeaux 1, CNRS/IN2p3, Centre d’Études Nucléaires de Bordeaux Gradignan, 33175 Gradignan, France
| | - S. Ritz
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - R. W. Romani
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - H. F.-W. Sadrozinski
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - D. Sanchez
- Laboratoire Leprince-Ringuet, École polytechnique, CNRS/IN2P3, Palaiseau, France
| | - P. M. Saz Parkinson
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - J. D. Scargle
- Space Sciences Division, NASA Ames Research Center, Moffett Field, CA 94035–1000, USA
| | - T. L. Schalk
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - C. Sgrò
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - E. J. Siskind
- NYCB Real-Time Computing, Lattingtown, NY 11560–1025, USA
| | - P. D. Smith
- Department of Physics, Center for Cosmology and Astro-Particle Physics, Ohio State University, Columbus, OH 43210, USA
| | - G. Spandre
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I-56127 Pisa, Italy
| | - P. Spinelli
- Dipartimento di Fisica “M. Merlin” dell’Università e del Politecnico di Bari, I-70126 Bari, Italy
- INFN, Sezione di Bari, 70126 Bari, Italy
| | - M. S. Strickman
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - D. J. Suson
- Department of Chemistry and Physics, Purdue University Calumet, Hammond, IN 46323–2094, USA
| | - H. Takahashi
- Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526, Japan
| | - T. Takahashi
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan
| | - T. Tanaka
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. B. Thayer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - D. J. Thompson
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - L. Tibaldo
- Laboratoire AIM, Commissariat à l’Énergie Atomique (CEA)– Institute of Research into the Fundamental Laws of the Universe (IRFU)/CNRS/Université Paris Diderot, Service d’Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
- INFN, Sezione di Padova, I-35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I-35131 Padova, Italy
| | - D. F. Torres
- Institut de Ciencies de l’Espai, Institut d’Estudis Espacials de Catalunya–Consejo Superior de Investigaciones Científicas (IEEC-CSIC), Campus UAB, 08193 Barcelona, Spain
- Institució Catalana de Recerca i Estudis Avançats (ICREA), Barcelona, Spain
| | - G. Tosti
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I-06123 Perugia, Italy
| | - A. Tramacere
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Consorzio Interuniversitario per la Fisica Spaziale (CIFS), I-10133 Torino, Italy
- INTEGRAL Science Data Centre, CH-1290 Versoix, Switzerland
| | - E. Troja
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - Y. Uchiyama
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. Vandenbroucke
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - V. Vasileiou
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Department of Physics and Center for Space Sciences and Technology, University of Maryland Baltimore County, Baltimore, MD 21250, USA
| | - G. Vianello
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Consorzio Interuniversitario per la Fisica Spaziale (CIFS), I-10133 Torino, Italy
| | - V. Vitale
- INFN, Sezione di Roma “Tor Vergata,” I-00133 Roma, Italy
- Dipartimento di Fisica, Università di Roma “Tor Vergata,” I-00133 Roma, Italy
| | - P. Wang
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - K. S. Wood
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - Z. Yang
- Department of Physics, Stockholm University, AlbaNova, SE-106 91 Stockholm, Sweden
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE-106 91 Stockholm, Sweden
| | - M. Ziegler
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
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Abstract
Macrophages in the gastrointestinal mucosa represent the largest pool of tissue macrophages in the body. In order to maintain mucosal homeostasis, resident intestinal macrophages uniquely do not express the lipopolysaccharide (LPS) co-receptor CD14 or the IgA (CD89) and IgG (CD16, 32, and 64) receptors, yet prominently display Toll-like receptors (TLRs) 3-9. Remarkably, intestinal macrophages also do not produce proinflammatory cytokines in response to TLR ligands, likely because of extracellular matrix (stromal) transforming growth factor-β (TGF-β) dysregulation of nuclear factor (NF)-κB signal proteins and, via Smad signaling, expression of IκBα, thereby inhibiting NF-κB-mediated activities. Thus, in noninflamed mucosa, resident macrophages are inflammation anergic but retain avid scavenger and host defense function, an ideal profile for macrophages in close proximity to gut microbiota. In the event of impaired epithelial integrity during intestinal infection or inflammation, however, blood monocytes also accumulate in the lamina propria and actively pursue invading microorganisms through uptake and degradation of the organism and release of inflammatory mediators. Consequently, resident intestinal macrophages are inflammation adverse, but when the need arises, they receive assistance from newly recruited circulating monocytes.
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Affiliation(s)
- PD Smith
- Department of Medicine (Gastroenterology) University of Alabama at Birmingham Birmingham, Alabama 35294-2182, USA
| | - LE Smythies
- Department of Medicine (Gastroenterology) University of Alabama at Birmingham Birmingham, Alabama 35294-2182, USA
| | - R Shen
- Department of Medicine (Gastroenterology) University of Alabama at Birmingham Birmingham, Alabama 35294-2182, USA
| | - T Greenwell-Wild
- Oral Infection and Immunity Branch National Institute of Dental and Craniofacial Research National Institutes of Health Bethesda, MD 20892-4352, USA
| | - M Gliozzi
- Oral Infection and Immunity Branch National Institute of Dental and Craniofacial Research National Institutes of Health Bethesda, MD 20892-4352, USA
| | - SM Wahl
- Oral Infection and Immunity Branch National Institute of Dental and Craniofacial Research National Institutes of Health Bethesda, MD 20892-4352, USA
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Metselaar M, Thompson KD, Gratacap RML, Kik MJL, LaPatra SE, Lloyd SJ, Call DR, Smith PD, Adams A. Association of red-mark syndrome with a Rickettsia-like organism and its connection with strawberry disease in the USA. J Fish Dis 2010; 33:849-858. [PMID: 20854353 DOI: 10.1111/j.1365-2761.2010.01187.x] [Citation(s) in RCA: 27] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/29/2023]
Abstract
Red-mark syndrome (RMS), a disease seen mostly in rainbow trout, Oncorhynchus mykiss, is of unknown aetiology. The research presented here indicates the presence of an intracellular bacterium in RMS-affected fish. A positive reaction was observed using immunohistochemistry (IHC) with skin lesions, liver, kidney and spleen of affected fish sampled from several locations within the United Kingdom using two different polyclonal antisera raised against Piscirickettsia salmonis. The same reaction was also seen with a number of different anti-P. salmonis monoclonal antibodies (MAbs). A disease with similar clinical signs to RMS, referred to as strawberry disease (SD), has been reported in the USA. A Rickettsia-like organism (RLO) has recently been associated with SD based on analysis of 16S rDNA sequences. Using the same panel of anti-P. salmonis antibodies used to screen the RMS samples, similar staining was obtained in tissue of SD-affected fish by IHC. A polymerase chain reaction (PCR) using RLO-specific primers was also performed on RMS-affected fish from the United Kingdom, and the samples were positive for the RLO 16S rRNA sequence. These findings suggest that the same aetiological agent may be responsible for RMS in the United Kingdom and SD in the USA.
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Affiliation(s)
- M Metselaar
- Aquatic Vaccine Unit, Institute of Aquaculture, University of Stirling, UK.
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21
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Abdo AA, Ackermann M, Ajello M, Atwood WB, Baldini L, Ballet J, Barbiellini G, Bastieri D, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bouvier A, Brandt TJ, Bregeon J, Brez A, Brigida M, Bruel P, Buehler R, Burnett TH, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Carrigan S, Casandjian JM, Cecchi C, Celik O, Charles E, Chaty S, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Conrad J, Corbel S, Corbet R, DeCesar ME, den Hartog PR, Dermer CD, de Palma F, Digel SW, Donato D, do Couto e Silva E, Drell PS, Dubois R, Dubus G, Dumora D, Favuzzi C, Fegan SJ, Ferrara EC, Fortin P, Frailis M, Fuhrmann L, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giglietto N, Giordano F, Giroletti M, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guiriec S, Hadasch D, Harding AK, Hayashida M, Hays E, Healey SE, Hill AB, Horan D, Hughes RE, Itoh R, Jean P, Jóhannesson G, Johnson AS, Johnson RP, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kataoka J, Kerr M, Knödlseder J, Koerding E, Kuss M, Lande J, Latronico L, Lee SH, Lemoine-Goumard M, Garde ML, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Makeev A, Mazziotta MN, McConville W, McEnery JE, Mehault J, Michelson PF, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Naumann-Godo M, Nestoras I, Nolan PL, Norris JP, Nuss E, Ohno M, Ohsugi T, Okumura A, Omodei N, Orlando E, Ormes JF, Ozaki M, Paneque D, Panetta JH, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piron F, Porter TA, Rainò S, Rando R, Ray PS, Razzano M, Razzaque S, Rea N, Reimer A, Reimer O, Reposeur T, Ripken J, Ritz S, Romani RW, Roth M, Sadrozinski HFW, Sander A, Parkinson PMS, Scargle JD, Schinzel FK, Sgrò C, Shaw MS, Siskind EJ, Smith DA, Smith PD, Sokolovsky KV, Spandre G, Spinelli P, Stawarz Ł, Strickman MS, Suson DJ, Takahashi H, Takahashi T, Tanaka T, Tanaka Y, Thayer JB, Thayer JG, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Vandenbroucke J, Vasileiou V, Vilchez N, Vitale V, Waite AP, Wallace E, Wang P, Winer BL, Wolff MT, Wood KS, Yang Z, Ylinen T, Ziegler M, Maehara H, Nishiyama K, Kabashima F, Bach U, Bower GC, Falcone A, Forster JR, Henden A, Kawabata KS, Koubsky P, Mukai K, Nelson T, Oates SR, Sakimoto K, Sasada M, Shenavrin VI, Shore SN, Skinner GK, Sokoloski J, Stroh M, Tatarnikov AM, Uemura M, Wahlgren GM, Yamanaka M. Gamma-ray emission concurrent with the nova in the symbiotic binary V407 Cygni. Science 2010; 329:817-21. [PMID: 20705855 DOI: 10.1126/science.1192537] [Citation(s) in RCA: 146] [Impact Index Per Article: 10.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Novae are thermonuclear explosions on a white dwarf surface fueled by mass accreted from a companion star. Current physical models posit that shocked expanding gas from the nova shell can produce x-ray emission, but emission at higher energies has not been widely expected. Here, we report the Fermi Large Area Telescope detection of variable gamma-ray emission (0.1 to 10 billion electron volts) from the recently detected optical nova of the symbiotic star V407 Cygni. We propose that the material of the nova shell interacts with the dense ambient medium of the red giant primary and that particles can be accelerated effectively to produce pi(0) decay gamma-rays from proton-proton interactions. Emission involving inverse Compton scattering of the red giant radiation is also considered and is not ruled out.
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Affiliation(s)
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- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
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22
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Abdo AA, Ackermann M, Ajello M, Atwood WB, Baldini L, Ballet J, Barbiellini G, Bastieri D, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cavazzuti E, Cecchi C, Celik O, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Colafrancesco S, Cominsky LR, Conrad J, Costamante L, Cutini S, Davis DS, Dermer CD, de Angelis A, de Palma F, Digel SW, do Couto e Silva E, Drell PS, Dubois R, Dumora D, Farnier C, Favuzzi C, Fegan SJ, Finke J, Focke WB, Fortin P, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Georganopoulos M, Germani S, Giebels B, Giglietto N, Giordano F, Giroletti M, Glanzman T, Godfrey G, Grenier IA, Grove JE, Guillemot L, Guiriec S, Hanabata Y, Harding AK, Hayashida M, Hays E, Hughes RE, Jackson MS, Jóhannesson G, Johnson AS, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kataoka J, Kawai N, Kerr M, Knödlseder J, Kocian ML, Kuss M, Lande J, Latronico L, Lemoine-Goumard M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Madejski GM, Makeev A, Mazziotta MN, McConville W, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nolan PL, Norris JP, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Paneque D, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piron F, Porter TA, Rainò S, Rando R, Razzano M, Razzaque S, Reimer A, Reimer O, Reposeur T, Ritz S, Rochester LS, Rodriguez AY, Romani RW, Roth M, Ryde F, Sadrozinski HFW, Sambruna R, Sanchez D, Sander A, Saz Parkinson PM, Scargle JD, Sgrò C, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Starck JL, Stawarz Ł, Strickman MS, Suson DJ, Tajima H, Takahashi H, Takahashi T, Tanaka T, Thayer JB, Thayer JG, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Vasileiou V, Vilchez N, Vitale V, Waite AP, Wallace E, Wang P, Winer BL, Wood KS, Ylinen T, Ziegler M, Hardcastle MJ, Kazanas D. Fermi Gamma-Ray Imaging of a Radio Galaxy. Science 2010; 328:725-9. [PMID: 20360067 DOI: 10.1126/science.1184656] [Citation(s) in RCA: 175] [Impact Index Per Article: 12.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
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23
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Abdo AA, Ackermann M, Ajello M, Atwood WB, Baldini L, Ballet J, Barbiellini G, Bastieri D, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cavazzuti E, Cecchi C, Celik O, Charles E, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Cominsky LR, Conrad J, Cutini S, Dermer CD, de Angelis A, de Palma F, Digel SW, Di Bernardo G, do Couto e Silva E, Drell PS, Drlica-Wagner A, Dubois R, Dumora D, Farnier C, Favuzzi C, Fegan SJ, Focke WB, Fortin P, Frailis M, Fukazawa Y, Funk S, Fusco P, Gaggero D, Gargano F, Gasparrini D, Gehrels N, Germani S, Giebels B, Giglietto N, Giommi P, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Gustafsson M, Hanabata Y, Harding AK, Hayashida M, Hughes RE, Itoh R, Jackson MS, Jóhannesson G, Johnson AS, Johnson RP, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kataoka J, Kawai N, Kerr M, Knödlseder J, Kocian ML, Kuehn F, Kuss M, Lande J, Latronico L, Lemoine-Goumard M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Madejski GM, Makeev A, Mazziotta MN, McConville W, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nolan PL, Norris JP, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Paneque D, Panetta JH, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piron F, Porter TA, Rainò S, Rando R, Razzano M, Reimer A, Reimer O, Reposeur T, Ritz S, Rochester LS, Rodriguez AY, Roth M, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Saz Parkinson PM, Scargle JD, Sellerholm A, Sgrò C, Shaw MS, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Starck JL, Strickman MS, Strong AW, Suson DJ, Tajima H, Takahashi H, Takahashi T, Tanaka T, Thayer JB, Thayer JG, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Vasileiou V, Vilchez N, Vitale V, Waite AP, Wang P, Winer BL, Wood KS, Ylinen T, Ziegler M. Spectrum of the isotropic diffuse gamma-ray emission derived from first-year Fermi Large Area Telescope data. Phys Rev Lett 2010; 104:101101. [PMID: 20366411 DOI: 10.1103/physrevlett.104.101101] [Citation(s) in RCA: 30] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/04/2009] [Indexed: 05/29/2023]
Abstract
We report on the first Fermi Large Area Telescope (LAT) measurements of the so-called "extragalactic" diffuse gamma-ray emission (EGB). This component of the diffuse gamma-ray emission is generally considered to have an isotropic or nearly isotropic distribution on the sky with diverse contributions discussed in the literature. The derivation of the EGB is based on detailed modeling of the bright foreground diffuse Galactic gamma-ray emission, the detected LAT sources, and the solar gamma-ray emission. We find the spectrum of the EGB is consistent with a power law with a differential spectral index gamma = 2.41 +/- 0.05 and intensity I(>100 MeV) = (1.03 +/- 0.17) x 10(-5) cm(-2) s(-1) sr(-1), where the error is systematics dominated. Our EGB spectrum is featureless, less intense, and softer than that derived from EGRET data.
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Affiliation(s)
- A A Abdo
- Space Science Division, Naval Research Laboratory, Washington, D.C. 20375, USA
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Abdo AA, Ackermann M, Ajello M, Atwood WB, Baldini L, Ballet J, Barbiellini G, Bastieri D, Bechtol K, Bellazzini R, Berenji B, Bloom ED, Bonamente E, Borgland AW, Bouvier A, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Carrigan S, Casandjian JM, Cecchi C, Celik O, Chekhtman A, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Conrad J, Dermer CD, de Angelis A, de Palma F, Digel SW, do Couto E Silva E, Drell PS, Drlica-Wagner A, Dubois R, Dumora D, Edmonds Y, Essig R, Farnier C, Favuzzi C, Fegan SJ, Focke WB, Fortin P, Frailis M, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giglietto N, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grove JE, Guillemot L, Guiriec S, Gustafsson M, Hadasch D, Harding AK, Horan D, Hughes RE, Jackson MS, Jóhannesson G, Johnson AS, Johnson RP, Johnson WN, Kamae T, Katagiri H, Kataoka J, Kawai N, Kerr M, Knödlseder J, Kuss M, Lande J, Latronico L, Llena Garde M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Makeev A, Mazziotta MN, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nolan PL, Norris JP, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Ozaki M, Paneque D, Panetta JH, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piron F, Rainò S, Rando R, Razzano M, Reimer A, Reimer O, Reposeur T, Ripken J, Ritz S, Rodriguez AY, Roth M, Sadrozinski HFW, Sander A, Parkinson PMS, Scargle JD, Schalk TL, Sellerholm A, Sgrò C, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Starck JL, Strickman MS, Suson DJ, Tajima H, Takahashi H, Tanaka T, Thayer JB, Thayer JG, Tibaldo L, Torres DF, Uchiyama Y, Usher TL, Vasileiou V, Vilchez N, Vitale V, Waite AP, Wang P, Winer BL, Wood KS, Ylinen T, Ziegler M. Fermi large area telescope search for photon lines from 30 to 200 GeV and dark matter implications. Phys Rev Lett 2010; 104:091302. [PMID: 20366979 DOI: 10.1103/physrevlett.104.091302] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/19/2009] [Indexed: 05/29/2023]
Abstract
Dark matter (DM) particle annihilation or decay can produce monochromatic gamma rays readily distinguishable from astrophysical sources. gamma-ray line limits from 30 to 200 GeV obtained from 11 months of Fermi Large Area Space Telescope data from 20-300 GeV are presented using a selection based on requirements for a gamma-ray line analysis, and integrated over most of the sky. We obtain gamma-ray line flux upper limits in the range 0.6-4.5x10{-9} cm{-2} s{-1}, and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
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Affiliation(s)
- A A Abdo
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
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Abdo AA, Ackermann M, Ajello M, Baldini L, Ballet J, Barbiellini G, Baring MG, Bastieri D, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cecchi C, Çelik Ö, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cognard I, Cohen-Tanugi J, Cominsky LR, Conrad J, Cutini S, Dermer CD, de Angelis A, de Palma F, Digel SW, do Couto e Silva E, Drell PS, Dubois R, Dumora D, Espinoza C, Farnier C, Favuzzi C, Fegan SJ, Focke WB, Fortin P, Frailis M, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giavitto G, Giebels B, Giglietto N, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Hanabata Y, Harding AK, Hayashida M, Hays E, Hughes RE, Jackson MS, Jóhannesson G, Johnson AS, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kataoka J, Katsuta J, Kawai N, Kerr M, Knödlseder J, Kocian ML, Kramer M, Kuss M, Lande J, Latronico L, Lemoine-Goumard M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Lyne AG, Madejski GM, Makeev A, Mazziotta MN, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Nolan PL, Norris JP, Noutsos A, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Paneque D, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piron F, Porter TA, Rainò S, Rando R, Razzano M, Reimer A, Reimer O, Reposeur T, Rochester LS, Rodriguez AY, Romani RW, Roth M, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Parkinson PMS, Scargle JD, Sgrò C, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Stappers BW, Stecker FW, Strickman MS, Suson DJ, Tajima H, Takahashi H, Takahashi T, Tanaka T, Thayer JB, Thayer JG, Theureau G, Thompson DJ, Tibaldo L, Tibolla O, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Vasileiou V, Venter C, Vilchez N, Vitale V, Waite AP, Wang P, Winer BL, Wood KS, Yamazaki R, Ylinen T, Ziegler M. Gamma-Ray Emission from the Shell of Supernova Remnant W44 Revealed by the Fermi LAT. Science 2010; 327:1103-6. [PMID: 20056857 DOI: 10.1126/science.1182787] [Citation(s) in RCA: 206] [Impact Index Per Article: 14.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Affiliation(s)
- A. A. Abdo
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - M. Ackermann
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Ajello
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - L. Baldini
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - J. Ballet
- Laboratoire Astrophysique Instrumentation Modélisation, Commissariat à l’Énergie Atomique (CEA)–Institut de Recherche sur les Lois Fondamentales de l’Univers (IRFU)/CNRS/Université Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - G. Barbiellini
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I–34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I–34127 Trieste, Italy
| | - M. G. Baring
- Rice University, Department of Physics and Astronomy, MS–108, Post Office Box 1892, Houston, TX 77251, USA
| | - D. Bastieri
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I–35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I–35131 Padova, Italy
| | - B. M. Baughman
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - K. Bechtol
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. Bellazzini
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - B. Berenji
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. D. Blandford
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. D. Bloom
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. Bonamente
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - A. W. Borgland
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. Bregeon
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - A. Brez
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - M. Brigida
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - P. Bruel
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - T. H. Burnett
- Department of Physics, University of Washington, Seattle, WA 98195–1560, USA
| | - S. Buson
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I–35131 Padova, Italy
| | - G. A. Caliandro
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - R. A. Cameron
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. A. Caraveo
- Istituto di Astrofisica Spaziale e Fisica Cosmica, Istituto Nazionale di Astrofisica (INAF), I–20133 Milano, Italy
| | - J. M. Casandjian
- Laboratoire Astrophysique Instrumentation Modélisation, Commissariat à l’Énergie Atomique (CEA)–Institut de Recherche sur les Lois Fondamentales de l’Univers (IRFU)/CNRS/Université Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - C. Cecchi
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - Ö. Çelik
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Center for Research and Exploration in Space Science and Technology (CRESST), NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- University of Maryland, Baltimore County, Baltimore, MD 21250, USA
| | - A. Chekhtman
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
- George Mason University, Fairfax, VA 22030, USA
| | - C. C. Cheung
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - J. Chiang
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Ciprini
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - R. Claus
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - I. Cognard
- Laboratoire de Physique et Chemie de l'Environnement (LPCE), LPCE UMR 6115 CNRS, F–45071 Orléans Cedex 02, France, and Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/Institut National des Sciences de l’Univers (INSU), F–18330 Nançay, France
| | - J. Cohen-Tanugi
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - L. R. Cominsky
- Department of Physics and Astronomy, Sonoma State University, Rohnert Park, CA 94928–3609, USA
| | - J. Conrad
- Department of Physics, Stockholm University, AlbaNova, SE–106 91 Stockholm, Sweden
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE–106 91 Stockholm, Sweden
| | - S. Cutini
- Agenzia Spaziale Italiana (ASI) Science Data Center, I–00044 Frascati (Roma), Italy
| | - C. D. Dermer
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - A. de Angelis
- Dipartimento di Fisica, Università di Udine and Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Gruppo Collegato di Udine, I–33100 Udine, Italy
| | - F. de Palma
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - S. W. Digel
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. do Couto e Silva
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. S. Drell
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - R. Dubois
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - D. Dumora
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - C. Espinoza
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
| | - C. Farnier
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - C. Favuzzi
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - S. J. Fegan
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - W. B. Focke
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Fortin
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - M. Frailis
- Dipartimento di Fisica, Università di Udine and Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Gruppo Collegato di Udine, I–33100 Udine, Italy
| | - Y. Fukazawa
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - S. Funk
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Fusco
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - F. Gargano
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - D. Gasparrini
- Agenzia Spaziale Italiana (ASI) Science Data Center, I–00044 Frascati (Roma), Italy
| | - N. Gehrels
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- University of Maryland, College Park, MD 20742, USA
| | - S. Germani
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - G. Giavitto
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, and Università di Trieste, I–34127 Trieste, Italy
| | - B. Giebels
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - N. Giglietto
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - F. Giordano
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - T. Glanzman
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - G. Godfrey
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - I. A. Grenier
- Laboratoire Astrophysique Instrumentation Modélisation, Commissariat à l’Énergie Atomique (CEA)–Institut de Recherche sur les Lois Fondamentales de l’Univers (IRFU)/CNRS/Université Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
| | - M.-H. Grondin
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - J. E. Grove
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - L. Guillemot
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - S. Guiriec
- University of Alabama in Huntsville, Huntsville, AL 35899, USA
| | - Y. Hanabata
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - A. K. Harding
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - M. Hayashida
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - E. Hays
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - R. E. Hughes
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - M. S. Jackson
- Department of Physics, Stockholm University, AlbaNova, SE–106 91 Stockholm, Sweden
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE–106 91 Stockholm, Sweden
- Department of Physics, Royal Institute of Technology (KTH), AlbaNova, SE–106 91 Stockholm, Sweden
| | - G. Jóhannesson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. S. Johnson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. J. Johnson
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- University of Maryland, College Park, MD 20742, USA
| | - W. N. Johnson
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - T. Kamae
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - H. Katagiri
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - J. Kataoka
- Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152–8551, Japan
- Waseda University, 1-104 Totsukamachi, Shinjuku-ku, Tokyo 169–8050, Japan
| | - J. Katsuta
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229–8510, Japan
- Department of Physics, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113–0033, Japan
| | - N. Kawai
- Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152–8551, Japan
- Cosmic Radiation Laboratory, Institute of Physical and Chemical Research (RIKEN), Wako, Saitama 351–0198, Japan
| | - M. Kerr
- Department of Physics, University of Washington, Seattle, WA 98195–1560, USA
| | - J. Knödlseder
- Centre d'Étude Spatiale des Rayonnements, CNRS/Université Paul Sabatier (UPS), BP 44346, F–30128 Toulouse Cedex 4, France
| | - M. L. Kocian
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Kramer
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
- Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
| | - M. Kuss
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - J. Lande
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - L. Latronico
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - M. Lemoine-Goumard
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - F. Longo
- Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I–34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I–34127 Trieste, Italy
| | - F. Loparco
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - B. Lott
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - M. N. Lovellette
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - P. Lubrano
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - A. G. Lyne
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
| | - G. M. Madejski
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Makeev
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
- George Mason University, Fairfax, VA 22030, USA
| | - M. N. Mazziotta
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - J. E. McEnery
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - C. Meurer
- Department of Physics and Astronomy, Sonoma State University, Rohnert Park, CA 94928–3609, USA
- Department of Physics, Stockholm University, AlbaNova, SE–106 91 Stockholm, Sweden
| | - P. F. Michelson
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - W. Mitthumsiri
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. Mizuno
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - C. Monte
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - M. E. Monzani
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Morselli
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma “Tor Vergata,” I–00133 Roma, Italy
| | - I. V. Moskalenko
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - S. Murgia
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. Nakamori
- Department of Physics, Tokyo Institute of Technology, Meguro City, Tokyo 152–8551, Japan
| | - P. L. Nolan
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. P. Norris
- Department of Physics and Astronomy, University of Denver, Denver, CO 80208, USA
| | - A. Noutsos
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
| | - E. Nuss
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - T. Ohsugi
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - N. Omodei
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - E. Orlando
- Max-Planck Institut für Extraterrestrische Physik, 85748 Garching, Germany
| | - J. F. Ormes
- Department of Physics and Astronomy, University of Denver, Denver, CO 80208, USA
| | - D. Paneque
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - D. Parent
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - V. Pelassa
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - M. Pepe
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - M. Pesce-Rollins
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - F. Piron
- Laboratoire de Physique Théorique et Astroparticules, Université Montpellier 2, CNRS/IN2P3, Montpellier, France
| | - T. A. Porter
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - S. Rainò
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - R. Rando
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I–35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I–35131 Padova, Italy
| | - M. Razzano
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - A. Reimer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A–6020 Innsbruck, Austria
| | - O. Reimer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Institut für Astro- und Teilchenphysik and Institut für Theoretische Physik, Leopold-Franzens-Universität Innsbruck, A–6020 Innsbruck, Austria
| | - T. Reposeur
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - L. S. Rochester
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - A. Y. Rodriguez
- Institut de Ciencies de l'Espai (IEEC-CSIC), Campus UAB, 08193 Barcelona, Spain
| | - R. W. Romani
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - M. Roth
- Department of Physics, University of Washington, Seattle, WA 98195–1560, USA
| | - F. Ryde
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE–106 91 Stockholm, Sweden
- Department of Physics, Royal Institute of Technology (KTH), AlbaNova, SE–106 91 Stockholm, Sweden
| | - H. F.-W. Sadrozinski
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - D. Sanchez
- Laboratoire Leprince-Ringuet, École Polytechnique, CNRS/Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), Palaiseau, France
| | - A. Sander
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - P. M. Saz Parkinson
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
| | - J. D. Scargle
- Space Sciences Division, NASA Ames Research Center, Moffett Field, CA 94035–1000, USA
| | - C. Sgrò
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - E. J. Siskind
- NYCB Real-Time Computing Incorporated, Lattingtown, NY 11560–1025, USA
| | - D. A. Smith
- Centre d'Études Nucléaires Bordeaux Gradignan, Université de Bordeaux, UMR 5797, 33175 Gradignan, France
- Centre d'Études Nucléaires Bordeaux Gradignan, CNRS/IN2P3, UMR 5797, Gradignan 33175, France
| | - P. D. Smith
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - G. Spandre
- Istituto Nazionale di Fisica Nucleare (INFN), Sezione di Pisa, I–56127 Pisa, Italy
| | - P. Spinelli
- Dipartimento di Fisica “M. Merlin” dell'Università e del Politecnico di Bari, I–70126 Bari, Italy
- Istituto Nazionale di Fisica Nucleare, Sezione di Bari, 70126 Bari, Italy
| | - B. W. Stappers
- Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester, Manchester M13 9PL, UK
| | - F. W. Stecker
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - M. S. Strickman
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - D. J. Suson
- Department of Chemistry and Physics, Purdue University Calumet, Hammond, IN 46323–2094, USA
| | - H. Tajima
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - H. Takahashi
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - T. Takahashi
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229–8510, Japan
| | - T. Tanaka
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. B. Thayer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - J. G. Thayer
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - G. Theureau
- Laboratoire de Physique et Chemie de l'Environnement (LPCE), LPCE UMR 6115 CNRS, F–45071 Orléans Cedex 02, France, and Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/Institut National des Sciences de l’Univers (INSU), F–18330 Nançay, France
| | - D. J. Thompson
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - L. Tibaldo
- Laboratoire Astrophysique Instrumentation Modélisation, Commissariat à l’Énergie Atomique (CEA)–Institut de Recherche sur les Lois Fondamentales de l’Univers (IRFU)/CNRS/Université Paris Diderot, Service d'Astrophysique, CEA Saclay, 91191 Gif sur Yvette, France
- Istituto Nazionale di Fisica Nucleare, Sezione di Padova, I–35131 Padova, Italy
- Dipartimento di Fisica “G. Galilei,” Università di Padova, I–35131 Padova, Italy
| | - O. Tibolla
- Max-Planck-Institut für Kernphysik, D–69029 Heidelberg, Germany
| | - D. F. Torres
- Institut de Ciencies de l'Espai (IEEC-CSIC), Campus UAB, 08193 Barcelona, Spain
- Institució Catalana de Recerca i Estudis Avançats (ICREA), 08010 Barcelona, Spain
| | - G. Tosti
- Istituto Nazionale di Fisica Nucleare, Sezione di Perugia, I–06123 Perugia, Italy
- Dipartimento di Fisica, Università degli Studi di Perugia, I–06123 Perugia, Italy
| | - A. Tramacere
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
- Consorzio Interuniversitario per la Fisica Spaziale (CIFS), I–10133 Torino, Italy
| | - Y. Uchiyama
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - T. L. Usher
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - V. Vasileiou
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Center for Research and Exploration in Space Science and Technology (CRESST), NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- University of Maryland, Baltimore County, Baltimore, MD 21250, USA
| | - C. Venter
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- North-West University, Potchefstroom Campus, Potchefstroom 2520, South Africa
| | - N. Vilchez
- Centre d'Étude Spatiale des Rayonnements, CNRS/Université Paul Sabatier (UPS), BP 44346, F–30128 Toulouse Cedex 4, France
| | - V. Vitale
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma “Tor Vergata,” I–00133 Roma, Italy
- Dipartimento di Fisica, Università di Roma “Tor Vergata,” I–00133 Roma, Italy
| | - A. P. Waite
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - P. Wang
- W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94305, USA
| | - B. L. Winer
- Department of Physics, Center for Cosmology and Astro-Particle Physics, The Ohio State University, Columbus, OH 43210, USA
| | - K. S. Wood
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
| | - R. Yamazaki
- Department of Physical Sciences, Hiroshima University, Higashi-Hiroshima, Hiroshima 739–8526, Japan
| | - T. Ylinen
- The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova, SE–106 91 Stockholm, Sweden
- Department of Physics, Royal Institute of Technology (KTH), AlbaNova, SE–106 91 Stockholm, Sweden
- School of Pure and Applied Natural Sciences, University of Kalmar, SE–391 82 Kalmar, Sweden
| | - M. Ziegler
- Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064, USA
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Abdo AA, Ackermann M, Ajello M, Anderson B, Atwood WB, Axelsson M, Baldini L, Ballet J, Barbiellini G, Bastieri D, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cecchi C, Charles E, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Conrad J, Dereli H, Dermer CD, de Angelis A, de Palma F, Digel SW, Di Bernardo G, Dormody M, do Couto e Silva E, Drell PS, Dubois R, Dumora D, Edmonds Y, Farnier C, Favuzzi C, Fegan SJ, Focke WB, Frailis M, Fukazawa Y, Funk S, Fusco P, Gaggero D, Gargano F, Gehrels N, Germani S, Giebels B, Giglietto N, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Hanabata Y, Harding AK, Hayashida M, Hays E, Hughes RE, Jóhannesson G, Johnson AS, Johnson RP, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kataoka J, Kawai N, Kerr M, Knödlseder J, Kocian ML, Kuehn F, Kuss M, Lande J, Latronico L, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Madejski GM, Makeev A, Mazziotta MN, McConville W, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nolan PL, Nuss E, Ohsugi T, Okumura A, Omodei N, Orlando E, Ormes JF, Paneque D, Panetta JH, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piron F, Porter TA, Rainò S, Rando R, Razzano M, Reimer A, Reimer O, Reposeur T, Ritz S, Rodriguez AY, Roth M, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Saz Parkinson PM, Scargle JD, Sellerholm A, Sgrò C, Smith DA, Smith PD, Spandre G, Spinelli P, Starck JL, Stecker FW, Striani E, Strickman MS, Strong AW, Suson DJ, Tajima H, Takahashi H, Tanaka T, Thayer JB, Thayer JG, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Vasileiou V, Vilchez N, Vitale V, Waite AP, Wang P, Winer BL, Wood KS, Ylinen T, Ziegler M. Fermi large area telescope measurements of the diffuse gamma-ray emission at intermediate galactic latitudes. Phys Rev Lett 2009; 103:251101. [PMID: 20366246 DOI: 10.1103/physrevlett.103.251101] [Citation(s) in RCA: 16] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/13/2009] [Indexed: 05/29/2023]
Abstract
The diffuse galactic gamma-ray emission is produced by cosmic rays (CRs) interacting with the interstellar gas and radiation field. Measurements by the Energetic Gamma-Ray Experiment Telescope (EGRET) instrument on the Compton Gamma-Ray Observatory indicated excess gamma-ray emission greater, > or approximately equal to 1 GeV relative to diffuse galactic gamma-ray emission models consistent with directly measured CR spectra (the so-called "EGRET GeV excess"). The Large Area Telescope (LAT) instrument on the Fermi Gamma-Ray Space Telescope has measured the diffuse gamma-ray emission with improved sensitivity and resolution compared to EGRET. We report on LAT measurements for energies 100 MeV to 10 GeV and galactic latitudes 10 degrees < or = |b| < or = 20 degrees. The LAT spectrum for this region of the sky is well reproduced by a diffuse galactic gamma-ray emission model that is consistent with local CR spectra and inconsistent with the EGRET GeV excess.
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Affiliation(s)
- A A Abdo
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
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Abdo AA, Ackermann M, Ajello M, Axelsson M, Baldini L, Ballet J, Barbiellini G, Bastieri D, Baughman B, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Brez A, Brigida M, Bruel P, Burnett TH, Buson S, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cecchi C, Çelik Ö, Chaty S, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen Tanugi J, Cominsky LR, Conrad J, Corbel S, Corbet R, Dermer CD, de Palma F, Digel S, do Couto e Silva E, Drell PS, Dubois R, Dubus G, Dumora D, Farnier C, Favuzzi C, Fegan SJ, Focke WB, Fortin P, Frailis M, Fusco P, Gargano F, Gehrels N, Germani S, Giavitto G, Giebels B, Giglietto N, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Hanabata Y, Harding A, Hayashida M, Hays E, Hill AB, Hjalmarsdotter L, Horan D, Hughes RE, Jackson MS, Jóhannesson G, Johnson AS, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kawai N, Kerr M, Knödlseder J, Kocian ML, Koerding E, Kuss M, Lande J, Latronico L, Lemoine Goumard M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Madejski GM, Makeev A, Marchand L, Marelli M, Moerbeck WM, Mazziotta MN, McColl N, McEnery JE, Meurer C, Michelson PF, Migliari S, Mitthumsiri W, Mizuno T, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nolan PL, Norris JP, Nuss E, Ohsugi T, Omodei N, Ong RA, Ormes JF, Paneque D, Parent D, Pelassa V, Pepe M, Rollins MP, Piron F, Pooley G, Porter TA, Pottschmidt K, Rainò S, Rando R, Ray PS, Razzano M, Rea N, Readhead A, Reimer A, Reimer O, Richards JL, Rochester LS, Rodriguez J, Rodriguez AY, Romani RW, Ryde F, Sadrozinski HFW, Sander A, Parkinson PMS, Sgrò C, Siskind EJ, Smith DA, Smith PD, Spinelli P, Starck JL, Stevenson M, Strickman MS, Suson DJ, Takahashi H, Tanaka T, Thayer JB, Thompson DJ, Tibaldo L, Tomsick JA, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Vasileiou V, Vilchez N, Vitale V, Waite AP, Wang P, Wilms J, Winer BL, Wood KS, Ylinen T, Ziegler M. Modulated High-Energy Gamma-Ray Emission from the Microquasar Cygnus X-3. Science 2009; 326:1512-6. [DOI: 10.1126/science.1182174] [Citation(s) in RCA: 179] [Impact Index Per Article: 11.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
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Abdo AA, Ackermann M, Ajello M, Atwood WB, Axelsson M, Baldini L, Ballet J, Barbiellini G, Bastieri D, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cecchi C, Celik O, Charles E, Chaty S, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Conrad J, Cutini S, Dermer CD, de Palma F, Digel SW, Dormody M, do Couto e Silva E, Drell PS, Dubois R, Dumora D, Farnier C, Favuzzi C, Fegan SJ, Focke WB, Frailis M, Fukazawa Y, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giebels B, Giglietto N, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grove JE, Guillemot L, Guiriec S, Hanabata Y, Harding AK, Hayashida M, Hays E, Horan D, Hughes RE, Jóhannesson G, Johnson AS, Johnson RP, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kawai N, Kerr M, Knödlseder J, Kuehn F, Kuss M, Lande J, Latronico L, Lemoine-Goumard M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Makeev A, Mazziotta MN, McConville W, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nolan PL, Norris JP, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Paneque D, Panetta JH, Parent D, Pelassa V, Pepe M, Pierbattista M, Piron F, Porter TA, Rainò S, Rando R, Razzano M, Rea N, Reimer A, Reimer O, Reposeur T, Ritz S, Rochester LS, Rodriguez AY, Romani RW, Roth M, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Saz Parkinson PM, Sgrò C, Smith DA, Smith PD, Spandre G, Spinelli P, Starck JL, Strickman MS, Suson DJ, Tajima H, Takahashi H, Tanaka T, Thayer JB, Thayer JG, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Vasileiou V, Vilchez N, Vitale V, Wang P, Webb N, Winer BL, Wood KS, Ylinen T, Ziegler M. Detection of high-energy gamma-ray emission from the globular cluster 47 Tucanae with Fermi. Science 2009; 325:845-8. [PMID: 19679807 DOI: 10.1126/science.1177023] [Citation(s) in RCA: 71] [Impact Index Per Article: 4.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
We report the detection of gamma-ray emissions above 200 megaelectron volts at a significance level of 17sigma from the globular cluster 47 Tucanae, using data obtained with the Large Area Telescope onboard the Fermi Gamma-ray Space Telescope. Globular clusters are expected to emit gamma rays because of the large populations of millisecond pulsars that they contain. The spectral shape of 47 Tucanae is consistent with gamma-ray emission from a population of millisecond pulsars. The observed gamma-ray luminosity implies an upper limit of 60 millisecond pulsars present in 47 Tucanae.
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Affiliation(s)
- A A Abdo
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
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Abdo AA, Ackermann M, Ajello M, Anderson B, Atwood WB, Axelsson M, Baldini L, Ballet J, Barbiellini G, Baring MG, Bastieri D, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Bignami GF, Blandford RD, Bloom ED, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Cecchi C, Celik O, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Conrad J, Cutini S, Dermer CD, de Angelis A, de Luca A, de Palma F, Digel SW, Dormody M, do Couto e Silva E, Drell PS, Dubois R, Dumora D, Farnier C, Favuzzi C, Fegan SJ, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giebels B, Giglietto N, Giommi P, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Gwon C, Hanabata Y, Harding AK, Hayashida M, Hays E, Hughes RE, Jóhannesson G, Johnson RP, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kataoka J, Kawai N, Kerr M, Knödlseder J, Kocian ML, Kuss M, Lande J, Latronico L, Lemoine-Goumard M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Madejski GM, Makeev A, Marelli M, Mazziotta MN, McConville W, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nolan PL, Norris JP, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Paneque D, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Pierbattista M, Piron F, Porter TA, Primack JR, Rainò S, Rando R, Ray PS, Razzano M, Rea N, Reimer A, Reimer O, Reposeur T, Ritz S, Rochester LS, Rodriguez AY, Romani RW, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Saz Parkinson PM, Scargle JD, Sgrò C, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Starck JL, Strickman MS, Suson DJ, Tajima H, Takahashi H, Takahashi T, Tanaka T, Thayer JG, Thompson DJ, Tibaldo L, Tibolla O, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Van Etten A, Vasileiou V, Vilchez N, Vitale V, Waite AP, Wang P, Watters K, Winer BL, Wolff MT, Wood KS, Ylinen T, Ziegler M. Detection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT. Science 2009; 325:840-4. [PMID: 19574346 DOI: 10.1126/science.1175558] [Citation(s) in RCA: 237] [Impact Index Per Article: 15.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Pulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants.
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Affiliation(s)
- A A Abdo
- Space Science Division, Naval Research Laboratory, Washington, DC 20375, USA
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Abdo AA, Ackermann M, Ajello M, Atwood WB, Axelsson M, Baldini L, Ballet J, Barbiellini G, Bastieri D, Battelino M, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bogaert G, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Caliandro GA, Cameron RA, Caraveo PA, Carlson P, Casandjian JM, Cecchi C, Charles E, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Cominsky LR, Conrad J, Cutini S, Dermer CD, de Angelis A, de Palma F, Digel SW, Di Bernardo G, do Couto E Silva E, Drell PS, Dubois R, Dumora D, Edmonds Y, Farnier C, Favuzzi C, Focke WB, Frailis M, Fukazawa Y, Funk S, Fusco P, Gaggero D, Gargano F, Gasparrini D, Gehrels N, Germani S, Giebels B, Giglietto N, Giordano F, Glanzman T, Godfrey G, Grasso D, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Hanabata Y, Harding AK, Hartman RC, Hayashida M, Hays E, Hughes RE, Jóhannesson G, Johnson AS, Johnson RP, Johnson WN, Kamae T, Katagiri H, Kataoka J, Kawai N, Kerr M, Knödlseder J, Kocevski D, Kuehn F, Kuss M, Lande J, Latronico L, Lemoine-Goumard M, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Madejski GM, Makeev A, Massai MM, Mazziotta MN, McConville W, McEnery JE, Meurer C, Michelson PF, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Moretti E, Morselli A, Moskalenko IV, Murgia S, Nolan PL, Norris JP, Nuss E, Ohsugi T, Omodei N, Orlando E, Ormes JF, Ozaki M, Paneque D, Panetta JH, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piron F, Pohl M, Porter TA, Profumo S, Rainò S, Rando R, Razzano M, Reimer A, Reimer O, Reposeur T, Ritz S, Rochester LS, Rodriguez AY, Romani RW, Roth M, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Saz Parkinson PM, Scargle JD, Schalk TL, Sellerholm A, Sgrò C, Smith DA, Smith PD, Spandre G, Spinelli P, Starck JL, Stephens TE, Strickman MS, Strong AW, Suson DJ, Tajima H, Takahashi H, Takahashi T, Tanaka T, Thayer JB, Thayer JG, Thompson DJ, Tibaldo L, Tibolla O, Torres DF, Tosti G, Tramacere A, Uchiyama Y, Usher TL, Van Etten A, Vasileiou V, Vilchez N, Vitale V, Waite AP, Wallace E, Wang P, Winer BL, Wood KS, Ylinen T, Ziegler M. Measurement of the cosmic ray e+ +e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope. Phys Rev Lett 2009; 102:181101. [PMID: 19518855 DOI: 10.1103/physrevlett.102.181101] [Citation(s) in RCA: 46] [Impact Index Per Article: 3.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/19/2009] [Indexed: 05/27/2023]
Abstract
Designed as a high-sensitivity gamma-ray observatory, the Fermi Large Area Telescope is also an electron detector with a large acceptance exceeding 2 m;{2} sr at 300 GeV. Building on the gamma-ray analysis, we have developed an efficient electron detection strategy which provides sufficient background rejection for measurement of the steeply falling electron spectrum up to 1 TeV. Our high precision data show that the electron spectrum falls with energy as E-3.0 and does not exhibit prominent spectral features. Interpretations in terms of a conventional diffusive model as well as a potential local extra component are briefly discussed.
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Affiliation(s)
- A A Abdo
- National Research Council Research Associate and Space Science Division, Naval Research Laboratory, Washington, D.C. 20375, USA
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Abdo AA, Ackermann M, Arimoto M, Asano K, Atwood WB, Axelsson M, Baldini L, Ballet J, Band DL, Barbiellini G, Baring MG, Bastieri D, Battelino M, Baughman BM, Bechtol K, Bellardi F, Bellazzini R, Berenji B, Bhat PN, Bissaldi E, Blandford RD, Bloom ED, Bogaert G, Bogart JR, Bonamente E, Bonnell J, Borgland AW, Bouvier A, Bregeon J, Brez A, Briggs MS, Brigida M, Bruel P, Burnett TH, Burrows D, Busetto G, Caliandro GA, Cameron RA, Caraveo PA, Casandjian JM, Ceccanti M, Cecchi C, Celotti A, Charles E, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Cominsky LR, Connaughton V, Conrad J, Costamante L, Cutini S, DeKlotz M, Dermer CD, de Angelis A, de Palma F, Digel SW, Dingus BL, do Couto e Silva E, Drell PS, Dubois R, Dumora D, Edmonds Y, Evans PA, Fabiani D, Farnier C, Favuzzi C, Finke J, Fishman G, Focke WB, Frailis M, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giebels B, Giglietto N, Giommi P, Giordano F, Glanzman T, Godfrey G, Goldstein A, Granot J, Greiner J, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Haller G, Hanabata Y, Harding AK, Hayashida M, Hays E, Hernando Morat JA, Hoover A, Hughes RE, Jóhannesson G, Johnson AS, Johnson RP, Johnson TJ, Johnson WN, Kamae T, Katagiri H, Kataoka J, Kavelaars A, Kawai N, Kelly H, Kennea J, Kerr M, Kippen RM, Knödlseder J, Kocevski D, Kocian ML, Komin N, Kouveliotou C, Kuehn F, Kuss M, Lande J, Landriu D, Larsson S, Latronico L, Lavalley C, Lee B, Lee SH, Lemoine-Goumard M, Lichti GG, Longo F, Loparco F, Lott B, Lovellette MN, Lubrano P, Madejski GM, Makeev A, Marangelli B, Mazziotta MN, McBreen S, McEnery JE, McGlynn S, Meegan C, Mészáros P, Meurer C, Michelson PF, Minuti M, Mirizzi N, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Moretti E, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Nelson D, Nolan PL, Norris JP, Nuss E, Ohno M, Ohsugi T, Okumura A, Omodei N, Orlando E, Ormes JF, Ozaki M, Paciesas WS, Paneque D, Panetta JH, Parent D, Pelassa V, Pepe M, Perri M, Pesce-Rollins M, Petrosian V, Pinchera M, Piron F, Porter TA, Preece R, Rainò S, Ramirez-Ruiz E, Rando R, Rapposelli E, Razzano M, Razzaque S, Rea N, Reimer A, Reimer O, Reposeur T, Reyes LC, Ritz S, Rochester LS, Rodriguez AY, Roth M, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Saz Parkinson PM, Scargle JD, Schalk TL, Segal KN, Sgrò C, Shimokawabe T, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Stamatikos M, Starck JL, Stecker FW, Steinle H, Stephens TE, Strickman MS, Suson DJ, Tagliaferri G, Tajima H, Takahashi H, Takahashi T, Tanaka T, Tenze A, Thayer JB, Thayer JG, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Tramacere A, Turri M, Tuvi S, Usher TL, van der Horst AJ, Vigiani L, Vilchez N, Vitale V, von Kienlin A, Waite AP, Williams DA, Wilson-Hodge C, Winer BL, Wood KS, Wu XF, Yamazaki R, Ylinen T, Ziegler M. Fermi Observations of High-Energy Gamma-Ray Emission from GRB 080916C. Science 2009; 323:1688-93. [DOI: 10.1126/science.1169101] [Citation(s) in RCA: 478] [Impact Index Per Article: 31.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
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Affiliation(s)
- P D Smith
- St. Vincent's Hospital, 5th Floor Daly Wing, Melbourne, VIC Australia 3065.
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Abdo AA, Ackermann M, Atwood WB, Baldini L, Ballet J, Barbiellini G, Baring MG, Bastieri D, Baughman BM, Bechtol K, Bellazzini R, Berenji B, Blandford RD, Bloom ED, Bogaert G, Bonamente E, Borgland AW, Bregeon J, Brez A, Brigida M, Bruel P, Burnett TH, Caliandro GA, Cameron RA, Caraveo PA, Carlson P, Casandjian JM, Cecchi C, Charles E, Chekhtman A, Cheung CC, Chiang J, Ciprini S, Claus R, Cohen-Tanugi J, Cominsky LR, Conrad J, Cutini S, Davis DS, Dermer CD, de Angelis A, de Palma F, Digel SW, Dormody M, do Couto E Silva E, Drell PS, Dubois R, Dumora D, Edmonds Y, Farnier C, Focke WB, Fukazawa Y, Funk S, Fusco P, Gargano F, Gasparrini D, Gehrels N, Germani S, Giebels B, Giglietto N, Giordano F, Glanzman T, Godfrey G, Grenier IA, Grondin MH, Grove JE, Guillemot L, Guiriec S, Harding AK, Hartman RC, Hays E, Hughes RE, Jóhannesson G, Johnson AS, Johnson RP, Johnson TJ, Johnson WN, Kamae T, Kanai Y, Kanbach G, Katagiri H, Kawai N, Kerr M, Kishishita T, Kiziltan B, Knödlseder J, Kocian ML, Komin N, Kuehn F, Kuss M, Latronico L, Lemoine-Goumard M, Longo F, Lonjou V, Loparco F, Lott B, Lovellette MN, Lubrano P, Makeev A, Marelli M, Mazziotta MN, McEnery JE, McGlynn S, Meurer C, Michelson PF, Mineo T, Mitthumsiri W, Mizuno T, Moiseev AA, Monte C, Monzani ME, Morselli A, Moskalenko IV, Murgia S, Nakamori T, Nolan PL, Nuss E, Ohno M, Ohsugi T, Okumura A, Omodei N, Orlando E, Ormes JF, Ozaki M, Paneque D, Panetta JH, Parent D, Pelassa V, Pepe M, Pesce-Rollins M, Piano G, Pieri L, Piron F, Porter TA, Rainò S, Rando R, Ray PS, Razzano M, Reimer A, Reimer O, Reposeur T, Ritz S, Rochester LS, Rodriguez AY, Romani RW, Roth M, Ryde F, Sadrozinski HFW, Sanchez D, Sander A, Parkinson PMS, Schalk TL, Sellerholm A, Sgrò C, Siskind EJ, Smith DA, Smith PD, Spandre G, Spinelli P, Starck JL, Strickman MS, Suson DJ, Tajima H, Takahashi H, Takahashi T, Tanaka T, Thayer JB, Thayer JG, Thompson DJ, Thorsett SE, Tibaldo L, Torres DF, Tosti G, Tramacere A, Usher TL, Van Etten A, Vilchez N, Vitale V, Wang P, Watters K, Winer BL, Wood KS, Yasuda H, Ylinen T, Ziegler M. The Fermi Gamma-Ray Space Telescope discovers the pulsar in the young galactic supernova remnant CTA 1. Science 2008; 322:1218-21. [PMID: 18927355 DOI: 10.1126/science.1165572] [Citation(s) in RCA: 80] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Energetic young pulsars and expanding blast waves [supernova remnants (SNRs)] are the most visible remains after massive stars, ending their lives, explode in core-collapse supernovae. The Fermi Gamma-Ray Space Telescope has unveiled a radio quiet pulsar located near the center of the compact synchrotron nebula inside the supernova remnant CTA 1. The pulsar, discovered through its gamma-ray pulsations, has a period of 316.86 milliseconds and a period derivative of 3.614 x 10(-13) seconds per second. Its characteristic age of 10(4) years is comparable to that estimated for the SNR. We speculate that most unidentified Galactic gamma-ray sources associated with star-forming regions and SNRs are such young pulsars.
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Affiliation(s)
- A A Abdo
- National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001, USA
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Abstract
Peripheral blood is the primary source of lymphoid cells for investigations of the human immune system. Its use is facilitated by the Ficoll-Hypaque density gradient centrifugation method described here. It is a simple and rapid method of purifying peripheral blood mononuclear cells (PBMC) that takes advantage of the density differences between mononuclear cells and other elements found in the blood sample. The mononuclear cell sample can be purified from monocytes by adherence or by exposure to L-leucine methyl ester; methods are described for both procedures. Cord blood and peripheral blood from infants contain immature cells, including nucleated red cells, that can result in significant contamination of the mononuclear cell layer, and removal of these cells requires additional steps that are described. The isolation procedures presented here can also be applied to cell populations derived from tissues.
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Affiliation(s)
- M E Kanof
- Massachusetts General Hospital and Harvard Medical School, Boston, Massachusetts, USA
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Abstract
An HIV-1 seronegative man presented with odynophagia, dysphagia, diarrhea, tenesmus and a 50-lb weight loss. A large esophageal ulcer and a rectal fissure were identified endoscopically. Stool samples and biopsy specimens from the esophageal ulcer, duodenum, colon and rectum were negative for pathogens. Seronegative AIDS was suspected, and high levels of HIV-1 mRNA (> 242,000 copies/mL) were detected. The esophageal ulcer responded to oral steroids and the HIV-1 infection to highly active anti-retroviral therapy (HAART). The virus isolated from the patient and an HIV-1 seropositive, asymptomatic, female sex worker with whom he had recently terminated a one-year heterosexual relationship showed sequence homology, indicating her as the source of his virus. The unusual presentation of severe gastrointestinal disease in an HIV-1 seronegative man with HIV-1 viremia underscores the importance of including AIDS in the differential diagnosis of wasting syndrome (i. e., B-type symptoms such as fever, night sweats, weight loss) in patients who are HIV-1 seronegative but at risk for AIDS.
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Affiliation(s)
- K Mönkemüller
- Division of Gastroenterology, Hepatology and Infectious Diseases, Otto-von-Guericke University, Magdeburg, Germany.
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Corripio-Miyar Y, Mazorra de Quero C, Treasurer JW, Ford L, Smith PD, Secombes CJ. Vaccination experiments in the gadoid haddock, Melanogrammus aeglefinus L., against the bacterial pathogen Vibrio anguillarum. Vet Immunol Immunopathol 2007; 118:147-53. [PMID: 17559945 DOI: 10.1016/j.vetimm.2007.04.011] [Citation(s) in RCA: 17] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/24/2007] [Revised: 04/16/2007] [Accepted: 04/26/2007] [Indexed: 11/21/2022]
Abstract
Vibrio anguillarum is one of the primary pathogens responsible for high levels of fish mortality in the aquaculture industry, and among gadoids O2a and b are the most common pathogenic serotypes. In this paper a variety of studies were performed to assess the optimal route by which to challenge haddock against this pathogen, and an optimal regime to vaccinate haddock. The most efficient method to challenge haddock with V. anguillarum in this study was immersion in a bath containing 10(7)cfu/ml, where 60% mortality was seen. Subsequent experiments showed that juvenile haddock could be protected against bacterial challenge with V. anguillarum, with a significant reduction in mortalities observed amongst the vaccination treatments when compared to the unvaccinated controls. However, as seen previously in cod studies, vaccination did not induce a specific antibody response.
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Affiliation(s)
- Y Corripio-Miyar
- Scottish Fish Immunology Research Centre, University of Aberdeen, Aberdeen, Scotland, UK.
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Wang YY, Sang Q, Smith PD, Murphy MA, Cook M, Tan SS. NS15P TRANSCRIPTIONAL REPRESSION IN A MOUSE MODEL OF EPILEPTOGENESIS. ANZ J Surg 2007. [DOI: 10.1111/j.1445-2197.2007.04124_15.x] [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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Camidge DR, Davies MJ, Laud PJ, Marshall AL, Cockerill M, Smith PD, Hughes AM. Factors determining the optimal body site and method for obtaining punch biopsies of human skin as a tissue in which to assess pharmacodynamic and pharmacokinetic endpoints in drug development studies. Cancer Chemother Pharmacol 2005; 57:52-8. [PMID: 16032432 DOI: 10.1007/s00280-005-0024-5] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/17/2004] [Accepted: 03/02/2005] [Indexed: 11/29/2022]
Abstract
There are potential advantages to detecting pharmacodynamic (PD) and pharmacokinetic (PK) endpoints in a tissue-based compartment such as the skin during the development of molecularly targeted drugs. We explored regional differences between inner arm, inner thigh, lower back and buttocks in 12 healthy male Caucasian volunteers in the tolerability of skin biopsy procedures; the Ki67 proliferation index; the frequency of detecting hair follicles and sweat glands; and the percentage of melanocytes. We also explored the amounts of tissue and protein obtained, and two separate methods of splitting biopsies for processing in mutually exclusive media. Biopsies from all body sites were well tolerated. The subjective ranking order was inner arm > buttocks = back > thigh. There were no statistically significant differences in the Ki67 labelling index (P > 0.05). The frequency of detecting sweat glands was the same in all body sites, but the frequency of detecting hair follicles was higher in back and buttock, compared to arm and thigh. The percentage of melanocytes was significantly lower in the buttocks compared to the back and thigh (P < 0.05), but not compared to the arm (P = 0.07). A 4-mm punch biopsy yielded a mean of 16.8 mg of tissue (range: 9-28 mg) and 160 microg of protein (range: 80-270 microg). In vivo sample splitting, by following a 2-mm punch with a 4-mm overpunch, had a shorter time from devascularisation to immersion into processing medium than ex vivo dissection of a 4-mm sample, which may be of importance to the assessment of labile endpoints. We conclude that multiple punch biopsies of the skin are feasible, with the buttocks representing the studied body site with the optimal balance between tolerability, hair follicle density and melanocyte density for obtaining tissue in which to assess PD and PK endpoints during drug development studies.
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Affiliation(s)
- D R Camidge
- Edinburgh Cancer Centre, Western General Hospital, Edinburgh, EH4 2XU, UK
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Smith PD, McLean KJ, Murphy MA, Turnley AM, Cook MJ. Seizures, not hippocampal neuronal death, provoke neurogenesis in a mouse rapid electrical amygdala kindling model of seizures. Neuroscience 2005; 136:405-15. [PMID: 16226389 DOI: 10.1016/j.neuroscience.2005.07.055] [Citation(s) in RCA: 36] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/20/2005] [Revised: 06/01/2005] [Accepted: 07/21/2005] [Indexed: 11/15/2022]
Abstract
PURPOSE Proliferation of neural precursors adjacent to the granule cell layer of the dentate gyrus has been identified in previous epilepsy models. Convincingly demonstrating that seizure activity is the stimulant for neurogenesis, rather than neuronal death or other insults inherent to seizure models, is difficult. To address this we derived a rapid electrical amygdala kindling model in mice known to be resistant to seizure-induced neuronal death as an experimental model of focal seizures and to analyze subsequent neurogenesis. METHODS Mice were implanted with bipolar electrodes in the left amygdala and given electrical stimulation (3 s, 100 Hz, 1 ms monophasic square wave pulses every 5 min, 40 in total) while being observed and graded for the development of seizures. Neurogenesis in the hippocampus was assessed by counting bromodeoxyuridine-immunoreactive cells co-labeled for astrocyte (glial fibrillary acidic protein) and neuronal nuclear markers. RESULTS Bromodeoxyuridine-reactive cell numbers were three-fold higher in stimulated mice compared with controls at 1 week in the subgranular region and at three weeks extensive co-labeling with neuronal nuclear was noted in cells which had migrated into the body of the granule cell layer, while mice receiving stimulation but failing to kindle did not differ significantly from controls. No increase in neuronal death was detected by terminal deoxynucleotidyl transferase-mediated digoxigenin-11-dUTP nick end labeling, Fluorojade or fluorescent examination of hematoxylin and eosin-stained sections in any inter-group comparison. CONCLUSIONS We propose that this kindling paradigm, not previously applied to mice, demonstrates more convincingly than previously the surge in neurogenesis in response to seizures, and the effects of seizures alone in regard to neuronal injury and regeneration.
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Affiliation(s)
- P D Smith
- Centre for Clinical Neurosciences and Neurological Research, St. Vincent's Hospital, Melbourne, Victoria, Australia.
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Camidge DR, Randall KR, Foster JR, Sadler CJ, Wright JA, Soames AR, Laud PJ, Smith PD, Hughes AM. Plucked human hair as a tissue in which to assess pharmacodynamic end points during drug development studies. Br J Cancer 2005; 92:1837-41. [PMID: 15886708 PMCID: PMC2361775 DOI: 10.1038/sj.bjc.6602558] [Citation(s) in RCA: 17] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/05/2022] Open
Abstract
We have demonstrated the feasibility of detecting and quantifying six cell-cycle-related nuclear markers (Ki67, pRb, p27, phospho-p27 (phosphorylated p27), phospho-pRb (phosphorylated pRb), phospho-HH3 (phosphorylated histone H3)) in plucked human scalp and eyebrow hair. Estimates of the proportion of plucked hairs that are lost or damaged during processing plus the intra- and intersubject variability of each nuclear marker with these techniques are provided to inform sizing decisions for intervention studies with drugs potentially impacting on these markers in the future.
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Affiliation(s)
- D R Camidge
- Edinburgh Cancer Centre, Western General Hospital, Edinburgh EH4 2XU, UK
| | - K R Randall
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
| | - J R Foster
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
| | - C J Sadler
- Syngenta, CTL, Alderley Park, Macclesfield, Cheshire SK10 4TJ, UK
| | - J A Wright
- Syngenta, CTL, Alderley Park, Macclesfield, Cheshire SK10 4TJ, UK
| | - A R Soames
- Syngenta, CTL, Alderley Park, Macclesfield, Cheshire SK10 4TJ, UK
| | - P J Laud
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
| | - P D Smith
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK. E-mail:
| | - A M Hughes
- AstraZeneca, Alderley Park, Macclesfield, Cheshire SK10 4TG, UK
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Abstract
BACKGROUND Patients with lipodermatosclerosis (LDS) due to chronic venous disease (CVD) of the lower limb show proliferation and convolution of their skin capillaries. There has been no previous attempt to quantify the severity of venous disease according to the extent of morphological change. AIM To quantify capillary damage in patients with CVD using capillary microscopy. METHOD 132 patients attending the vascular clinic for management of CVD were examined clinically and by duplex ultrasonography; they were assigned to the appropriate CEAP clinical stage by a surgeon. Ten control subjects with no arterial or venous disease of the lower limb were also studied. Digital images of the skin microcirculation were obtained using a CAM1 microscope. In patients with skin changes the most severe regions of LDS were studied. In all other subjects the region 5 cm proximal to the medial malleolus was investigated. The total number of visible capillaries and capillary convolutions was counted in a 2.4 mm2 region. RESULTS The more advanced stages are associated with the reduced numbers of capillaries. The number of convolutions is greatly increased in the more severe stages, C4b and C5. These have been graded in four classes. The capillary counts (per square mm) and convolutions per capillary in C0, C2 and C5 patients are 8(6-11), 1(1-1); 6(4-9), 1(1-2); 3(3-4), 7(6-8), respectively. CONCLUSIONS Amongst patients with venous disease, capillary convolution is strongly associated with the more severe stages (LDS and healed ulceration), which can reliably be reproduced by capillary microscope.
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Affiliation(s)
- M H Howlader
- Department of Surgery, Royal Free and University College Medical School, Middlesex Hospital, Mortimer Street, London W1N 8AA, U.K
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Wright TE, Hill DP, Ko F, Soler PM, Smith PD, Franz M, Nichols EH, Robson MC. The effect of TGF-beta2 in various vehicles on incisional wound healing. Int J Surg Investig 2003; 2:133-43. [PMID: 12678511] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 03/01/2023]
Abstract
BACKGROUND The isoforms of transforming growth factor beta (TGF-beta) have been shown to be deficient in models of impaired wound healing. Exogenous application of the growth factor to enhance healing as been investigated. TGF-beta1 has been shown to enhance incisional wound strength, but to be dependent on the vehicle used to carry the cytokine. Because TGF-beta2 has shown safety in human trials of chronic wound healing, this study evaluates TGF-beta2 in acute incisional healing using a variety of vehicles. METHODS Using an acute incisional wound model in healthy rats, rhTGF-beta2 was suspended in various vehicles including fibrin sealant (normal commercial concentration), fibrin sealant (dilute concentration), phosphate buffered saline/serum albumin, and a carboxymethycellulose gel. A single dose of the agent was instilled into the incisions at the time of wound closure and breaking strength analyses and histology performed periodically from days 3-14. RESULTS TGF-beta2 enhanced the gain of incisional strength in all vehicles during the first two weeks of healing. This was most noticeable by day three with the carboxymethycellulose gel, but by day 7 with the other vehicles. Like reports with TGF-beta1, TGF-beta2 accelerated the gain of wound strength by about three days by day 11. Normal density fibrin sealant delayed incisional healing; whereas, the other vehicles without TGF-beta2 had no significant effect. CONCLUSIONS The use of TGF-beta2 appears to be of value in increasing incisional wound strength in the first 14 days post-wounding in healthy rats and this effect is demonstrated in a variety of vehicles. These data support the hypothesis that the "normal" incisional wound healing curve can he shifted to the left. Shortening the time for gain of incisional wound strength may have potential clinical use.
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Affiliation(s)
- T E Wright
- The Institute of Tissue Regeneration, Repair and Rehabilitation, Bay Pines VA Medical Center, Bay Pines, Florida 33744, USA
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Crocker SJ, Liston P, Anisman H, Lee CJ, Smith PD, Earl N, Thompson CS, Park DS, Korneluk RG, Robertson GS. Attenuation of MPTP-induced neurotoxicity and behavioural impairment in NSE-XIAP transgenic mice. Neurobiol Dis 2003; 12:150-61. [PMID: 12667469 DOI: 10.1016/s0969-9961(02)00020-7] [Citation(s) in RCA: 45] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/21/2022] Open
Abstract
X-linked IAP protein is a potent inhibitor of cell death. Here, we describe a novel transgenic mouse in which the human XIAP gene is expressed under the control of the neuron-specific enolase promoter (NSE-xiap). We demonstrate that nigrostriatal dopamine neurons of NSE-xiap mice were resistant to the damaging effects of the dopaminergic neurotoxin MPTP. MPTP-induced reduction of striatal dopamine metabolism was also attenuated in NSE-xiap mice. Furthermore, NSE-xiap mice treated with MPTP did not exhibit deficits in exploratory behaviour in an open-field test. Taken together, these findings suggest that strategies to enhance neuronal expression of XIAP may provide therapeutic benefit for the treatment of neurodegeneration in Parkinson's disease.
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Affiliation(s)
- S J Crocker
- Neuroscience Research Institute, University of Ottawa, Ottawa, Ontario K1H 8M5, Canada.
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Abstract
STAT proteins constitute a family of transcription factors whose activation by cytokine and non-cytokine receptors leads to tyrosine phosphorylation, dimerization and translocation from the cytoplasm to the nucleus. In the nucleus they activate the transcription of specific genes by binding to consensus DNA elements. STATs 1 and 3 can be activated by both cytokine and non-cytokine receptors, and bind as homodimers or heterodimers to viral simian sarcoma virus (sis)-inducible elements such as that found in the c-fos promoter. Activation of c-Src and EGF receptor tyrosine kinases is associated with progression of breast cancer. Both these events lead to activation of STAT proteins, Src kinases activate STAT3 dependent transcription in mammary epithelial cells and EGF receptor activation can lead to activation of STATs 1 and 3. STAT3 activation has been demonstrated to have a role in oncogenesis and increasingly, activated STAT proteins are found to be activated in human cancer. In this study we describe detailed immunohistochemical analysis of nuclear and cytoplasmic STATs 1 and 3 expression in primary breast carcinomas and correlate this with EGFR, HER2, p53, ER, PR, p21/waf1, Bcl-XL and Ki-67 expression. We also compared expression between normal and tumor tissue. We report here a highly significant correlation between nuclear STAT3 expression and breast cancers compared to normal tissue. We also report a very strong correlation between nuclear STAT3 and EGFR expression in breast cancers. These data clearly demonstrate a strong association between STAT3 activation and breast tumorigenesis and strengthen the assertion that STAT3 activation may play an important role in the tumorigenic conversion of breast tissue mediated by tyrosine kinase signaling pathways.
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MESH Headings
- Adenocarcinoma, Mucinous/diagnosis
- Adenocarcinoma, Mucinous/metabolism
- Adult
- Aged
- Aged, 80 and over
- Breast Neoplasms/diagnosis
- Breast Neoplasms/metabolism
- Carcinoma, Ductal, Breast/diagnosis
- Carcinoma, Ductal, Breast/metabolism
- Carcinoma, Lobular/diagnosis
- Carcinoma, Lobular/metabolism
- DNA-Binding Proteins/metabolism
- ErbB Receptors/metabolism
- Female
- Humans
- Immunoenzyme Techniques
- Ki-67 Antigen/metabolism
- Middle Aged
- Neoplasm Staging
- Prognosis
- Proto-Oncogene Proteins c-bcl-2/metabolism
- Receptor, ErbB-2/metabolism
- Receptors, Estrogen/metabolism
- Receptors, Progesterone/metabolism
- STAT1 Transcription Factor
- STAT3 Transcription Factor
- Trans-Activators/metabolism
- Tumor Suppressor Protein p53/metabolism
- bcl-X Protein
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Affiliation(s)
- G Berclaz
- Department of Obstetrics and Gynecology, Inselspital, CH-3012 Berne, Switzerland.
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Crocker SJ, Lamba WR, Smith PD, Callaghan SM, Slack RS, Anisman H, Park DS. c-Jun mediates axotomy-induced dopamine neuron death in vivo. Proc Natl Acad Sci U S A 2001; 98:13385-90. [PMID: 11687617 PMCID: PMC60880 DOI: 10.1073/pnas.231177098] [Citation(s) in RCA: 77] [Impact Index Per Article: 3.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/18/2022] Open
Abstract
Expression of the transcription factor c-Jun is induced in neurons of the central nervous system (CNS) in response to injury. Mechanical transection of the nigrostriatal pathway at the medial forebrain bundle (MFB) results in the delayed retrograde degeneration of the dopamine neurons in the substantia nigra pars compacta (SNc) and induces protracted expression and phosphorylation of c-Jun. However, the role of c-Jun after axotomy of CNS neurons is unclear. Here, we show that adenovirus-mediated expression of a dominant negative form of c-Jun (Ad.c-JunDN) inhibited axotomy-induced dopamine neuron death and attenuated phosphorylation of c-Jun in nigral neurons. Ad.c-JunDN also delayed the degeneration of dopaminergic nigral axons in the striatum after MFB axotomy. Taken together, these findings suggest that activation of c-Jun mediates the loss of dopamine neurons after axotomy injury.
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Affiliation(s)
- S J Crocker
- Neuroscience Research Institute, University of Ottawa, Ottawa, ON K1H 8M5, Canada
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Smith PD, Smythies LE, Mosteller-Barnum M, Sibley DA, Russell MW, Merger M, Sellers MT, Orenstein JM, Shimada T, Graham MF, Kubagawa H. Intestinal macrophages lack CD14 and CD89 and consequently are down-regulated for LPS- and IgA-mediated activities. J Immunol 2001; 167:2651-6. [PMID: 11509607 DOI: 10.4049/jimmunol.167.5.2651] [Citation(s) in RCA: 255] [Impact Index Per Article: 11.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/19/2022]
Abstract
The intestinal mucosa normally displays minimal inflammation despite the close proximity between mucosal macrophages and lumenal bacteria. Macrophages interact with bacteria and their products through CD14, a surface receptor involved in the response to LPS, and CD89, the receptor for IgA (FcalphaR). Here we show that resident macrophages isolated from normal human intestine lack CD14 and CD89. The absence of CD14 and CD89 was not due to the isolation procedure or mucosal cell products, but was evident at the transcriptional level, as the macrophages expressed neither CD14- nor CD89-specific mRNAs, but did express Toll-like receptor 2 and 4 transcripts. Consistent with their CD14(-) phenotype, lamina propria macrophages displayed markedly reduced LPS-induced cytokine production and LPS-enhanced phagocytosis. In addition, IgA-enhanced phagocytosis was sharply reduced in lamina propria macrophages. Thus, the absence of CD14 and CD89 on resident intestinal macrophages, due to down-regulated gene transcription, causes down-modulated LPS- and IgA-mediated functions and probably contributes to the low level of inflammation in normal human intestinal mucosa.
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Affiliation(s)
- P D Smith
- Department of Medicine, University of Alabama, and Veterans Affairs Medical Center, Birmingham, AL 35294, USA.
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Abstract
OBJECTIVES To evaluate the prevalence of reported physical and sexual abuse among youths with substance use problems, to explore whether youths report relying on substances to cope with the abuse, and to examine whether individual factors related to substance use were associated with the outcome measures of reported physical abuse, sexual abuse, and using substances to cope. METHOD We assessed 287 male and female youths (age 14 to 24 years) who presented for help for substance use problems, using a semistructured interview that focused on substance use, history of previous sexual and physical abuse, and coping strategies. RESULTS One-half of the female youth substance abusers reported having been sexually abused (50.0%), while male youth substance users reported a significantly lower rate (10.4%). Similarly, one-half of the female youths had a history of physical abuse (50.5%), and males again had a lower rate (26.0%). Of those who endorsed a history of abuse, more females (64.7%) than males (37.9%) reported using substances to cope with the trauma. Specific associations between the outcome measures and substance use variables were found for youths in both sexes. CONCLUSION These findings underscore the importance of why clinicians should explore abuse issues with substance-using youth of both sexes. Identifying concurrent factors will help provide better intervention strategies. Suggestions for assessing sexual and physical abuse in youths with substance use disorders are provided.
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Affiliation(s)
- B C Ballon
- Youth Addiction Service, University of Toronto, Centre for Addiction and Mental Health Toronto, Ontario.
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Abstract
The causes of venous ulceration remain unclear. Twentieth-century hypotheses concentrated on the possibility that this problem was caused by failure of oxygen delivery to the skin. However, it has been difficult to substantiate these predictions in practice. Although the presence of tissue hypoxia has been suggested by studies in which transcutaneous oxygen tension has been assessed with transducers heated to unphysiological temperatures, when oxygen measurements are made at room temperature there is little evidence of tissue hypoxia. This has led to the assessment of alternative mechanisms of ulcer development. There has been considerable interest in recent years in the inflammatory processes that surround venous ulceration. A complex sequence of events appears to surround the development of leg ulceration. Increased leukocyte activation has been shown in patients with venous disease as well as increased expression of soluble endothelial adhesion molecules. Histologic studies of the skin in patients with chronic venous disease show a perivascular infiltration of the capillaries of the papillary plexus (the most superficial part of the dermis) with monocytes, macrophages, and connective tissue proteins including fibrin. Fibrosis of the skin and subcutaneous tissues may be initiated by increased gene expression and production of transforming growth factor-beta1. Vascular endothelial growth factor may be involved in the capillary proliferation that has been reported in the skin by a number of authors. Increased expression of several tissue metalloproteinases has been reported both in liposclerotic skin and periulcer skin. The tissue inhibitors of metalloproteinases are also increased and the net result is unclear. Treatment of venous disease using micronized purified flavonoid fraction moderates some of the inflammatory markers, including leukocyte ligand expression and endothelial adhesion molecule shedding. These compounds have also been shown to reduce leukocyte-endothelial adhesion in animal models of ischemia-reperfusion injury. Many inflammatory processes have now been shown to be involved in the development of the skin changes in patients with chronic venous disease. However, the precise sequence of events that leads to leg ulceration is still unclear. Pharmacologic treatments aimed at moderating some of these inflammatory processes are now under investigation as potential ways of treating patients with the more advanced stages of venous disease.
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Affiliation(s)
- P D Smith
- Department of Surgery, Royal Free and University College Medical School, The Middlesex Hospital, London, UK.
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López-Dóriga MV, Smail DA, Smith RJ, Doménech A, Castric J, Smith PD, Ellis AE. Isolation of salmon pancreas disease virus (SPDV) in cell culture and its ability to protect against infection by the 'wild-type' agent. Fish Shellfish Immunol 2001; 11:505-22. [PMID: 11556480 DOI: 10.1006/fsim.2000.0330] [Citation(s) in RCA: 23] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/13/2023]
Abstract
A Scottish salmon pancreas disease virus (SPDV) has been isolated and its optimum growth conditions determined. Although several fish cell lines have been tested, successful culture was achieved only with CHSE-214 cells. Cytopathic effects were observed after 5 days. The highest virus titres, calculated by microtitration assay, were reached at 15 degrees C. After 7-9 days post-inoculation, CHSE-214 cell supernatants contained between 10(7)-10(5) TCID50 ml(-1) The cultured isolate is chloroform- and pH 3.0-sensitive, and virions are 50-60 nm in diameter. These characteristics are similar to the Irish SPDV isolates. The culture isolate induced typical pancreas disease (PD) lesions in experimentally infected Atlantic salmon and convalescent fish were resistant to experimental infection with PD-infective kidney homogenates obtained by serial in vivo passages from a PD-infected farmed salmon (termed wild-type SPDV). Furthermore, fish immunised with the inactivated cultured virus were protected against a cohabitation challenge with the wild-type virus. Immunised fish sera showed virus-neutralising activity before challenge (7 weeks post-immunisation) and from 3-6 weeks post-challenge, when sera from non-immunised fish did not neutralise the virus. At 6 weeks post-cohabitation challenge, previously immunised fish had neutralising titres of up to 1:65. Following intraperitoneal (i.p.) challenge, immunised fish showed neutralising titres as high as 1:226 at 8 weeks post-challenge. Non-immunised fish injected i.p. with the wild-type virus developed serum-neutralising activity against the cultured isolate when sampled 8 weeks after infection, confirming an antigenic relationship between the wild-type and cultured virus. The results demonstrate that the tissue culture-adapted isolate of SPDV could be successfully used to protect against challenge by the wild-type virus and could therefore have potential use as an inactivated vaccine against PD.
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