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

来源：

ASTROPHYSICAL JOURNAL | 1998年 / 493卷 / 01期

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

页码：L27 / L30

页数：4

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