A search for optical afterglow from GRB 970828

被引:112
|
作者
Groot, PJ
Galama, TJ
van Paradijs, J
Kouveliotou, C
Wijers, RAMJ
Bloom, J
Tanvir, N
Vanderspek, R
Greiner, J
Castro-Tirado, AJ
Gorosabel, J
von Hippel, T
Lehnert, M
Kuijken, K
Hoekstra, H
Metcalfe, N
Howk, C
Conselice, C
Telting, J
Rutten, RGM
Rhoads, J
Cole, A
Pisano, DJ
Naber, R
Schwarz, R
机构
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[2] Ctr High Energy Astrophys, NL-1098 SJ Amsterdam, Netherlands
[3] Univ Alabama, Dept Phys, Huntsville, AL 35899 USA
[4] NASA, Univ Space Res Assoc, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA
[5] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[6] CALTECH, Div Phys Math & Astron 105 24, Pasadena, CA 91125 USA
[7] MIT, Ctr Space Res, Cambridge, MA 02139 USA
[8] Astrophys Inst Postdam, Potsdam, Germany
[9] INTA, Lab Astrofis Espacial & Fis Fundamental, E-28080 Madrid, Spain
[10] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA
[11] Sterrewacht Leiden, NL-2300 RA Leiden, Netherlands
[12] Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands
[13] Univ Durham, Dept Phys, Durham, England
[14] ING Telescopes NFRA, Tenerife 38780, Spain
[15] Natl Opt Astron Observ, Tucson, AZ 85726 USA
关键词
dust; extinction; galaxies; general; gamma rays; bursts; observations radiation; mechanisms; nonthermal;
D O I
10.1086/311125
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the results of R-band observations of the error box of the gamma-ray burst of 1997 August 28 made between 4 hr and 8 days after this burst occurred. No counterpart was found varying by more than 0.2 mag down to R = 23.8. We discuss the consequences of this nondetection for relativistic blast wave models of gamma-ray bursts and the possible effect of redshift on the relation between optical absorption and the low-energy cutoff in the X-ray afterglow spectrum.
引用
收藏
页码:L27 / L30
页数:4
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