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

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 γ–ray event, in the I-band. A bright optical transient (OT 000313) with $I = 9.4 \pm 0.1$ was found in the BOOTES-1 image, close to the...

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2002-10, Vol.393 (3), p.L55-L59
Hauptverfasser: Castro-Tirado, A. J., Castro Cerón, J. M., Gorosabel, J., Páta, P., Soldán, J., Hudec, R., Jelinek, M., Topinka, M., Bernas, M., Mateo Sanguino, T. J., A. de Ugarte Postigo, Berná, J. Á., Henden, A., Vrba, F., Canzian, B., Harris, H., Delfosse, X., de Pontieu, B., Polcar, J., Sánchez-Fernández, C., de la Morena, B. A., Más-Hesse, J. M., Torres Riera, J., Barthelmy, S.
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container_issue 3
container_start_page L55
container_title Astronomy and astrophysics (Berlin)
container_volume 393
creator Castro-Tirado, A. J.
Castro Cerón, J. M.
Gorosabel, J.
Páta, P.
Soldán, J.
Hudec, R.
Jelinek, M.
Topinka, M.
Bernas, M.
Mateo Sanguino, T. J.
A. de Ugarte Postigo
Berná, J. Á.
Henden, A.
Vrba, F.
Canzian, B.
Harris, H.
Delfosse, X.
de Pontieu, B.
Polcar, J.
Sánchez-Fernández, C.
de la Morena, B. A.
Más-Hesse, J. M.
Torres Riera, J.
Barthelmy, S.
description 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 γ–ray event, in the I-band. A bright optical transient (OT 000313) with $I = 9.4 \pm 0.1$ was found in the BOOTES-1 image, close to the error box (3σ) provided by BATSE. Late time $VRIK^\prime$-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.
doi_str_mv 10.1051/0004-6361:20021172
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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. 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source Bacon EDP Sciences France Licence nationale-ISTEX-PS-Journals-PFISTEX; EDP Sciences; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals
subjects cosmology: observations
gamma rays: bursts
optical transients
techniques: photometric
title Detection of an optical transient following the 13 March 2000 short/hard gamma-ray burst
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