CONSTRAINTS ON VERY HIGH ENERGY EMISSION FROM GRB 130427A

被引：25

作者：

Aliu, E. ^{[1
]}

Aune, T. ^{[2
]}

Barnacka, A. ^{[3
]}

Beilicke, M. ^{[4
]}

Benbow, W. ^{[5
]}

Berger, K. ^{[6
,7
]}

Biteau, J. ^{[8
,9
]}

Buckley, J. H. ^{[4
]}

Bugaev, V. ^{[4
]}

Byrum, K. ^{[10
]}

Cardenzana, J. V. ^{[11
]}

Cerruti, M. ^{[5
]}

Chen, X. ^{[12
,13
]}

Ciupik, L. ^{[14
]}

Connaughton, V. ^{[15
]}

Cui, W. ^{[16
]}

Dickinson, H. J. ^{[11
]}

Eisch, J. D. ^{[11
]}

Errando, M. ^{[1
]}

Falcone, A. ^{[17
]}

Federici, S. ^{[12
,13
]}

Feng, Q. ^{[16
]}

Finley, J. P. ^{[16
]}

Fleischhack, H. ^{[13
]}

Fortin, P. ^{[5
]}

Fortson, L. ^{[18
]}

Furniss, A. ^{[8
,9
]}

Galante, N. ^{[5
]}

Gillanders, G. H. ^{[19
]}

Griffin, S. ^{[20
]}

Griffiths, S. T. ^{[21
]}

Grube, J. ^{[14
]}

Gyuk, G. ^{[14
]}

Hakansson, N. ^{[12
]}

Hanna, D. ^{[20
]}

Holder, J. ^{[6
,7
]}

Hughes, G. ^{[13
]}

Humensky, T. B. ^{[22
]}

Johnson, C. A. ^{[8
,9
]}

Kaaret, P. ^{[21
]}

Kar, P. ^{[23
]}

Kertzman, M. ^{[24
]}

Khassen, Y. ^{[25
]}

Kieda, D. ^{[23
]}

Krawczynski, H. ^{[4
]}

Krennrich, F. ^{[11
]}

Lang, M. J. ^{[19
]}

Madhavan, A. S. ^{[11
]}

Maier, G. ^{[13
]}

McArthur, S. ^{[26
]}

机构：

[1] Columbia Univ Barnard Coll, Dept Phys & Astron, New York, NY 10027 USA

[2] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA

[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[4] Washington Univ, Dept Phys, St Louis, MO 63130 USA

[5] Harvard Smithsonian Ctr Astrophys, Fred Lawrence Whipple Observ, Amado, AZ 85645 USA

[6] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA

[7] Univ Delaware, Bartol Res Inst, Newark, DE 19716 USA

[8] Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA

[9] Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA

[10] Argonne Natl Lab, Argonne, IL 60439 USA

[11] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA

[12] Univ Potsdam, Inst Phys & Astron, D-14476 Potsdam, Germany

[13] DESY, D-15738 Zeuthen, Germany

[14] Adler Planetarium & Astron Museum, Dept Astron, Chicago, IL 60605 USA

[15] Univ Alabama, Ctr Space Plasma & Aeron Res, Huntsville, AL 35899 USA

[16] Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA

[17] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[18] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA

[19] Natl Univ Ireland Galway, Sch Phys, Galway, Ireland

[20] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada

[21] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA

[22] Columbia Univ, Dept Phys, New York, NY 10027 USA

[23] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA

[24] Depauw Univ, Dept Phys & Astron, Greencastle, IN 46135 USA

[25] Natl Univ Ireland Univ Coll Dublin, Sch Phys, Dublin 4, Ireland

[26] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA

[27] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[28] Georgia Inst Technol, Sch Phys, Atlanta, GA 30332 USA

[29] Georgia Inst Technol, Ctr Relativist Astrophys, Atlanta, GA 30332 USA

[30] Anderson Univ, Dept Phys, Anderson, IN 46012 USA

[31] Galway Mayo Inst Technol, Dept Life & Phys Sci, Galway, Ireland

[32] Calif Polytech State Univ San Luis Obispo, Dept Phys, San Luis Obispo, CA 94307 USA

[33] Cork Inst Technol, Dept Appl Phys & Instrumentat, Bishopstown, Cork, Ireland

[34] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[35] Univ Maryland, Dept Phys, College Pk, MD 20742 USA

[36] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[37] George Washington Univ, Dept Phys, Washington, DC 20052 USA

[38] Penn State Univ, Dept Phys, University Pk, PA 16802 USA

[39] Penn State Univ, Ctr Particle & Gravitat Astrophys, University Pk, PA 16802 USA

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2014年 / 795卷 / 01期

基金：

美国国家科学基金会; 加拿大自然科学与工程研究理事会; 爱尔兰科学基金会;

关键词：

gamma-ray burst: individual (GRB 130427A); GAMMA-RAY BURSTS; COMPONENT; AFTERGLOWS; SWIFT; TELESCOPE; SPECTRA; MISSION; LIMITS; TEV;

D O I：

10.1088/2041-8205/795/1/L3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Prompt emission from the very fluent and nearby (z = 0.34) gamma-ray burst GRB130427A was detected by several orbiting telescopes and by ground-based, wide-field-of-view optical transient monitors. Apart from the intensity and proximity of this GRB, it is exceptional due to the extremely long-lived high-energy (100 MeV to 100 GeV) gamma-ray emission, which was detected by the Large Area Telescope on the Fermi Gamma-Ray Space Telescope for similar to 70 ks after the initial burst. The persistent, hard-spectrum, high-energy emission suggests that the highest-energy gamma rays may have been produced via synchrotron self-Compton processes though there is also evidence that the high-energy emission may instead be an extension of the synchrotron spectrum. VERITAS, a ground-based imaging atmospheric Cherenkov telescope array, began follow-up observations of GRB130427A similar to 71 ks (similar to 20 hr) after the onset of the burst. The GRB was not detected with VERITAS; however, the high elevation of the observations, coupled with the low redshift of the GRB, make VERITAS a very sensitive probe of the emission from GRB130427A for E > 100 GeV. The non-detection and consequent upper limit derived place constraints on the synchrotron self-Compton model of high-energy gamma-ray emission from this burst.

引用

页数：6

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