Detection of an optical transient following the 13 March 2000 short/hard gamma-ray burst

被引:20
作者
Castro-Tirado, AJ
Cerón, JMC
Gorosabel, J
Páta, P
Soldán, J
Hudec, R
Jelinek, M
Topinka, M
Bernas, M
Sanguino, TJM
Postigo, AD
Berná, JA
Henden, A
Vrba, F
Canzian, B
Harris, H
Delfosse, X
de Pontieu, B
Polcar, J
Sánchez-Fernández, C
de la Morena, BA
Más-Hesse, JM
Riera, JT
Barthelmy, S
机构
[1] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
[2] INTA, LAEFF, Madrid 28080, Spain
[3] Real Inst, Cadiz 11110, Spain
[4] Observ Armada, Secc Astron, Cadiz 11110, Spain
[5] Danish Space Res Inst, DK-2100 Copenhagen O, Denmark
[6] Czech Tech Univ, Fac Elect Engn, Dept Radioelect, Prague 16627, Czech Republic
[7] Acad Sci Czech Republ, Inst Astron, CS-25165 Ondrejov, Czech Republic
[8] INTA, CEDEA, Mazagon 21130, Huelva, Spain
[9] Univ Complutense, Dept Astrofis, E-28040 Madrid, Spain
[10] Univ Alicante, Dept Fis Ingn Sistemas & Teoria Senal, E-03080 Alicante, Spain
[11] Univ Space Res Assoc, Flagstaff Stn, Flagstaff, AZ USA
[12] USN Observ, Flagstaff Stn, Flagstaff, AZ USA
[13] Observ Grenoble, Astrophys Lab, Grenoble, France
[14] Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA
[15] Masaryk Univ, Dept Theoret Phys & Astrophys, Brno, Czech Republic
[16] INTA, DCE, Madrid 28850, Spain
[17] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
关键词
gamma rays : bursts; optical transients; techniques : photometric; cosmology : observations;
D O I
10.1051/0004-6361:20021172
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We imaged the error box of a gamma-ray burst of the short (0.5 s), hard type (GRB 000313), with the BOOTES-1 experiment in southern Spain, starting 4 min after the gamma-ray event, in the I-band. A bright optical transient (OT 000313) with I = 9.4 +/- 0.1 was found in the BOOTES-1 image, close to the error box (3sigma) provided by BATSE. Late time VRI K'-band deep observations failed to reveal an underlying host galaxy. If the OT 000313 is related to the short, hard GRB 000313, this would be the first optical counterpart ever found for this kind of events (all counterparts to date have been found for bursts of the long, soft type). The fact that only prompt optical emission has been detected (but no afterglow emission at all, as supported by theoretical models) might explain why no optical counterparts have ever been found for short, hard GRBs. This fact suggests that most short bursts might occur in a low-density medium and favours the models that relate them to binary mergers in very low-density environments.
引用
收藏
页码:L55 / L59
页数:5
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