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FERMI DETECTION DELAYED GeV EMISSION FROM THE SHORT GAMMA-RAY BURST 081024B
Abdo, A. A.1,2; Ackermann, M.3,4; Ajello, M.3,4; Asano, K.5; Atwood, W. B.6,7; Axelsson, M.8,9; Baldini, L.10; Ballet, J.11; Barbiellini, G.12,13; Bastieri, D.14,15; Baughman, B. M.16; Bechtol, K.3,4; Bellazzini, R.10; Berenji, B.3,4; Bhat, P. N.17; Bissaldi, E.18; Blandford, R. D.3,4; Bloom, E. D.3,4; Bonamente, E.19,20; Borgland, A. W.3,4; Bouvier, A.3,4; Bregeon, J.10; Brez, A.10; Briggs, M. S.17; Brigida, M.21,22,23; Bruel, P.24; Burgess, J. M.17; Burnett, T. H.25; Buson, S.15; Caliandro, G. A.26; Cameron, R. A.3,4; Caraveo, P. A.27; Carrigan, S.15; Casandjian, J. M.11; Cecchi, C.19,20; Celik, Oe28,29,30,31; Chaplin, V.17; Charles, E.3,4; Chekhtman, A.1,32; Chiang, J.3,4; Ciprini, S.20; Claus, R.3,4; Cohen-Tanugi, J.33; Cominsky, L. R.34; Connaughton, V.17; Conrad, J.9,35; Cutini, S.36; Dermer, C. D.1; de Angelis, A.37,38; de Palma, F.21,22,23; Digel, S. W.3,4; do Couto e Silva, E.3,4; Drell, P. S.3,4; Dubois, R.3,4; Dumora, D.39,40; Farnier, C.33; Favuzzi, C.21,22,23; Fegan, S. J.24; Fishman, G.41; Focke, W. B.3,4; Fortin, P.24; Frailis, M.37,38; Fukazawa, Y.42; Funk, S.3,4; Fusco, P.21,22,23; Gargano, F.23; Gasparrini, D.36; Gehrels, N.28,43,44,45; Germani, S.19,20; Giebels, B.24; Giglietto, N.21,22,23; Giommi, P.36; Giordano, F.21,22,23; Glanzman, T.3,4; Godfrey, G.3,4; Granot, J.46; Grenier, I. A.11; Grondin, M-H.39,40; Grove, J. E.1; Guillemot, L.47; Guiriec, S.17; Hanabata, Y.42; Harding, A. K.28; Hayashida, M.3,4; Haynes, R. H.48; Hays, E.28; Horan, D.24; Hughes, R. E.16; Jackson, M. S.9,49; Johannesson, G.3,4; Johnson, A. S.3,4; Johnson, W. N.1; Kamae, T.3,4; Katagiri, H.42; Kataoka, J.50; Kawai, N.51,52; Kerr, M.25; Kippen, R. M.53; Knoedlseder, J.54; Kocevski, D.3,4; Kocian, M. L.3,4; Komin, N.11,33; Kouveliotou, C.41; Kuehn, F.16; Kuss, M.10; Lande, J.3,4; Latronico, L.10; Lemoine-Goumard, M.39,40; Longo, F.12,13; Loparco, F.21,22,23; Lott, B.39,40; Lovellette, M. N.1; Lubrano, P.19,20; Madejski, G. M.3,4; Makeev, A.1,32; Mazziotta, M. N.23; McBreen, S.18,55; McEnery, J. E.28,44,45; McGlynn, S.9,49; Meegan, C.56; Meszaros, P.43; Meurer, C.9,35; Michelson, P. F.3,4; Mitthumsiri, W.3,4; Mizuno, T.42; Moiseev, A. A.28,29,44,45; Monte, C.21,22,23; Monzani, M. E.3,4; Moretti, E.12,13; Morselli, A.57; Moskalenko, I. V.3,4; Murgia, S.3,4; Nakamori, T.51; Nolan, P. L.3,4; Norris, J. P.58; Nuss, E.33; Ohno, M.59; Ohsugi, T.42; Omodei, N.10; Orlando, E.18; Ormes, J. F.58; Paciesas, W. S.17; Paneque, D.3,4; Panetta, J. H.3,4; Parent, D.39,40; Pelassa, V.33; Pepe, M.19,20; Pesce-Rollins, M.10; Piron, F.33; Porter, T. A.6,7; Preece, R.17; Raino, S.21,22,23; Rando, R.14,15; Razzano, M.10; Razzaque, S.1,2; Reimer, A.3,4,60,61; Reimer, O.3,4,60,61; Reposeur, T.39,40; Ripken, J.9,35; Ritz, S.6,7; Rochester, L. S.3,4; Rodriguez, A. Y.26; Roth, M.25; Ryde, F.9,49; Sadrozinski, H. F-W.6,7; Sanchez, D.24; Sander, A.16; Parkinson, P. M. Saz6,7; Scargle, J. D.62; Schalk, T. L.6,7; Sgro, C.10; Siskind, E. J.63; Smith, D. A.39,40; Smith, P. D.16; Spandre, G.10; Spinelli, P.21,22,23; Stamatikos, M.16,28; Strickman, M. S.1; Suson, D. J.64; Tagliaferri, G.65; Tajima, H.3,4; Takahashi, H.42; Tanaka, T.3,4; Thayer, J. B.3,4; Thayer, J. G.3,4; Thompson, D. J.28; Tibaldo, L.11,14,15; Toma, K.43; Torres, D. F.26,66; Tosti, G.19,20; Tramacere, A.3,4,67; Troja, E.28,51; Uchiyama, Y.3,4; Usher, T. L.3,4; van der Horst, A. J.41; Vasileiou, V.28,29,30,31; Vilchez, N.54; Vitale, V.57,68; von Kienlin, A.18; Waite, A. P.3,4; Wang, P.3,4; Wilson-Hodge, C.41; Winer, B. L.16; Wood, K. S.1; Wu, X. F.43,69,70; Yamazaki, R.42; Ylinen, T.9,49,71; Ziegler, M.6,7
2010-03-20
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume712Issue:1Pages:558-564
AbstractWe report on the detailed analysis of the high-energy extended emission from the short gamma-ray burst (GRB) 081024B detected by the Fermi Gamma-ray Space Telescope. Historically, this represents the first clear detection of temporal extended emission from a short GRB. The light curve observed by the Fermi Gamma-ray Burst Monitor lasts approximately 0.8 s whereas the emission in the Fermi Large Area Telescope lasts for about 3 s. Evidence of longer lasting high-energy emission associated with long bursts has been already reported by previous experiments. Our observations, together with the earlier reported study of the bright short GRB 090510, indicate similarities in the high-energy emission of short and long GRBs and open the path to new interpretations.
KeywordGamma-ray Burst: General Gamma-ray Burst: Individual (Grb 081024b)
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1088/0004-637X/712/1/558
WOS KeywordMERGING NEUTRON-STARS ; HIGH-ENERGY NEUTRINOS ; 28 FEBRUARY 1997 ; BATSE OBSERVATIONS ; PROTONS ; SPECTRA ; CATALOG
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000275222900049
Citation statistics
Cited Times:54[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/1207
Collection南极天文中心
Affiliation1.USN, Res Lab, Div Space Sci, Washington, DC 20375 USA
2.Natl Acad Sci, Natl Res Council Res Associate, Washington, DC 20001 USA
3.Stanford Univ, Dept Phys, Stanford, CA 94305 USA
4.Stanford Univ, SLAC Natl Accelerator Lab, WW Hansen Expt Phys Lab, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
5.Tokyo Inst Technol, Interact Res Ctr Sci, Meguro, Tokyo 1528551, Japan
6.Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Dept Phys, Santa Cruz, CA 95064 USA
7.Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
8.Stockholm Univ, Dept Astron, SE-10691 Stockholm, Sweden
9.Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden
10.Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
11.Univ Paris Diderot, Lab AIM, CEA IRFU, CNRS,Serv Astrophys,CEA Saclay, F-91191 Gif Sur Yvette, France
12.Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy
13.Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy
14.Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy
15.Univ Padua, Dipartimento Fis G Galilei, I-35131 Padua, Italy
16.Ohio State Univ, Dept Phys, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA
17.Univ Alabama, CSPAR, Huntsville, AL 35899 USA
18.Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
19.Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
20.Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy
21.Univ Bari, Dipartimento Fis M Merlin, I-70126 Bari, Italy
22.Politecn Bari, I-70126 Bari, Italy
23.Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy
24.Ecole Polytech, CNRS, Lab Leprince Ringuet, IN2P3, F-91128 Palaiseau, France
25.Univ Washington, Dept Phys, Seattle, WA 98195 USA
26.CSIC, Inst Ciencias Espai, IEEC, Barcelona 08193, Spain
27.Ist Astrofis Spaziale & Fis Cosm, INAF, I-20133 Milan, Italy
28.NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
29.CRESST, Greenbelt, MD 20771 USA
30.Univ Maryland Baltimore Cty, Dept Phys, Baltimore, MD 21250 USA
31.Univ Maryland Baltimore Cty, Ctr Space Sci & Technol, Baltimore, MD 21250 USA
32.George Mason Univ, Fairfax, VA 22030 USA
33.Univ Montpellier 2, Lab Phys Theor & Astroparticules, CNRS, IN2P3, Montpellier, France
34.Sonoma State Univ, Dept Phys & Astron, Rohnert Pk, CA 94928 USA
35.Stockholm Univ, Dept Phys, SE-10691 Stockholm, Sweden
36.Sci Data Ctr, ASI, I-00044 Frascati, Roma, Italy
37.Univ Udine, Dipartimento Fis, I-33100 Udine, Italy
38.Ist Nazl Fis Nucl, Sez Trieste, Grp Collegato Udine, I-33100 Udine, Italy
39.Univ Bordeaux, Ctr Etud Nucl Bordeaux Gradignan, UMR 5797, F-33175 Gradignan, France
40.Ctr Etud Nucl Bordeaux Gradignan, CNRS, IN2P3, UMR 5797, F-33175 Gradignan, France
41.NASA, Marshall Space Flight Ctr, Duluth, MN 55812 USA
42.Hiroshima Univ, Dept Phys Sci, Hiroshima 7398526, Japan
43.Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
44.Univ Maryland, Dept Phys, College Pk, MD 20742 USA
45.Univ Maryland, Dept Astron, College Pk, MD 20742 USA
46.Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England
47.Max Planck Inst Radioastron, D-53121 Bonn, Germany
48.Univ Virginia, Charlottesville, VA 22904 USA
49.Royal Inst Technol KTH, Dept Phys, SE-10691 Stockholm, Sweden
50.Waseda Univ, Shinjuku Ku, Tokyo 1698050, Japan
51.Tokyo Inst Technol, Dept Phys, Meguro, Tokyo 1528551, Japan
52.RIKEN, Cosm Radiat Lab, Inst Phys & Chem Res, Wako, Saitama 3510198, Japan
53.Los Alamos Natl Lab, Los Alamos, NM 87545 USA
54.UPS, Ctr Etud Spatiale Rayonnements, CNRS, F-30128 Toulouse 4, France
55.Natl Univ Ireland Univ Coll Dublin, Dublin 4, Ireland
56.USRA, Columbia, MD 21044 USA
57.Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy
58.Univ Denver, Dept Phys & Astron, Denver, CO 80208 USA
59.JAXA, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
60.Leopold Franzens Univ Innsbruck, Inst Astro & Teilchenphys, A-6020 Innsbruck, Austria
61.Leopold Franzens Univ Innsbruck, Inst Theoret Phys, A-6020 Innsbruck, Austria
62.NASA, Ames Res Ctr, Div Space Sci, Moffett Field, CA 94035 USA
63.NYCB Real Time Comp Inc, Lattingtown, NY 11560 USA
64.Purdue Univ Calumet, Dept Chem & Phys, Hammond, IN 46323 USA
65.INAF Osservatorio Astron Brera, I-23807 Merate, Italy
66.ICREA, Barcelona, Spain
67.CIFS, I-10133 Turin, Italy
68.Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy
69.J CPNPC, Nanjing 210093, Peoples R China
70.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
71.Univ Kalmar, Sch Pure & Appl Nat Sci, SE-39182 Kalmar, Sweden
Recommended Citation
GB/T 7714
Abdo, A. A.,Ackermann, M.,Ajello, M.,et al. FERMI DETECTION DELAYED GeV EMISSION FROM THE SHORT GAMMA-RAY BURST 081024B[J]. ASTROPHYSICAL JOURNAL,2010,712(1):558-564.
APA Abdo, A. A..,Ackermann, M..,Ajello, M..,Asano, K..,Atwood, W. B..,...&Ziegler, M..(2010).FERMI DETECTION DELAYED GeV EMISSION FROM THE SHORT GAMMA-RAY BURST 081024B.ASTROPHYSICAL JOURNAL,712(1),558-564.
MLA Abdo, A. A.,et al."FERMI DETECTION DELAYED GeV EMISSION FROM THE SHORT GAMMA-RAY BURST 081024B".ASTROPHYSICAL JOURNAL 712.1(2010):558-564.
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