RAPID SEARCHES FOR COUNTERPARTS OF GRB-930131

被引:25
作者
SCHAEFER, BE
BARTHELMY, SD
PALMER, DM
CLINE, TL
HURLEY, KC
SOMMER, M
BOER, M
NIEL, M
FISHMAN, GJ
KOUVELIOTOU, C
MEEGAN, CA
COE, MJ
ELMEGREEN, BG
MCNAMARA, BJ
HARRISON, T
OWENS, A
SOLLEE, N
STULL, J
PALERMITI, M
SCHWARTZ, R
BROOKS, J
VANDERSPEK, R
RICKER, GR
KRIMM, HA
WENZEL, W
GREINER, J
HUDEC, R
NOVAK, M
BOROVICKA, J
PREDOTA, M
BAILYN, CD
HANLON, LO
BENNETT, K
SPOELSTRA, TAT
SMETTE, A
PEDERSEN, H
FLORENTIN, R
POLLAS, C
STEINLE, H
SCHRAMM, KJ
IYENGAR, KVK
PRABHU, TP
机构
[1] NASA, GODDARD SPACE FLIGHT CTR, GREENBELT, MD 20771 USA
[2] UNIV CALIF BERKELEY, SPACE SCI LAB, BERKELEY, CA 94720 USA
[3] NASA, GEORGE C MARSHALL SPACE FLIGHT CTR, HUNTSVILLE, AL 35812 USA
[4] UNIV SOUTHAMPTON, SOUTHAMPTON SO9 5NH, HANTS, ENGLAND
[5] IBM CORP, THOMAS J WATSON RES CTR, YORKTOWN HTS, NY 10598 USA
[6] NEW MEXICO STATE UNIV, DEPT ASTRON, LAS CRUCES, NM 88003 USA
[7] UNIV LEICESTER, LEICESTER LE1 7RH, ENGLAND
[8] SANTA BARBARA ASTRON GRP, SANTA BARBARA, CA USA
[9] ALFRED UNIV, ALFRED, NY 14802 USA
[10] MIT, CAMBRIDGE, MA 02139 USA
[11] SONNEBERG OBSERV, W-6400 SONNEBERG, GERMANY
[12] ASTRON INST, CS-25165 ONDREJOV, CZECH REPUBLIC
[13] YALE UNIV, DEPT ASTRON, NEW HAVEN, CT 06511 USA
[14] HAMBURG OBSERV, W-2050 HAMBURG 80, GERMANY
[15] UNIV SPACE RES ASSOC, HUNTSVILLE, AL USA
[16] MAX PLANCK INST EXTRATERR PHYS, W-8046 GARCHING, GERMANY
[17] UPS, CNRS, CTR ETUDE SPATIALE RAYONNEMENTS, F-31029 TOULOUSE, FRANCE
[18] PALERMITI OBSERV, JUPITER, FL 33478 USA
[19] METEOROL STN CHURANOV, CHURANOV, CZECH REPUBLIC
[20] ESA, ESTEC, DIV ASTROPHYS, 2200 AG NOORDWIJK, NETHERLANDS
[21] NFRA, RADIO OBSERV, 7990 AA DWINGELOO, NETHERLANDS
[22] EUROPEAN SO OBSERV, LA SERENA, CHILE
[23] COPENHAGEN UNIV OBSERV, DK-1350 COPENHAGEN K, DENMARK
[24] CERGA, OBSERVA COTE AZUR, OBSERV CALERN, F-06460 ST VALLIER DE THIEY, FRANCE
[25] INDIAN INST ASTROPHYS, BANGALORE 560034, INDIA
关键词
GAMMA RAYS; BURSTS;
D O I
10.1086/187215
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A fading counterpart to a gamma-ray burst (GRB) would appear as a point source inside a GRB error region soon after the burst which dims on a timescale from minutes to days. The favorable circumstances of the burst GRB 930131 allowed for an international campaign to search for fading counterparts starting 6.8 hr after the burst. We report observations from many optical sites, two radio telescopes, and archival ROSAT data, including deep Schmidt exposures 35, 44, and 64 hr after the burst. No fading counterparts were detected with our observations.
引用
收藏
页码:L71 / L74
页数:4
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