EDP Sciences
Free access
Volume 383, Number 1, February III 2002
Page(s) 112 - 117
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20011716

A&A 383, 112-117 (2002)
DOI: 10.1051/0004-6361:20011716

Constraints on the optical afterglow emission of the short/hard burst GRB 010119

J. Gorosabel1, M. I. Andersen2, J. Hjorth3, H. Pedersen3, B. L. Jensen3, J. U. Fynbo4, H. J. Lehto5, 6, S. Katajainen5, K. Hurley7 and N. Lund1

1  Danish Space Research Institute, Juliane Maries Vej 30, 2100 Copenhagen Ø, Denmark
    e-mail: jgu@dsri.dk; nl@dsri.dk
2  Division of Astronomy, University of Oulu PO Box 3000, 90014 University of Oulu, Finland
    e-mail: michael.andersen@oulu.fi
3  Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen Ø, Denmark
    e-mail: jens@astro.ku.dk; holger@astro.ku.dk; brian_j@astro.ku.dk
4  European Southern Observatory, Karl-Schwarzschild-Straße 2, 85748 Garching, Germany
    e-mail: jfynbo@eso.org
5  Tuorla Observatory, Väisäläntie 20, 21500 Piikkiö, Finland
    e-mail: harry.lehto@astro.utu.fi; seppo.katajainen@astro.utu.fi
6  Department of Physics, University of Turku, 20140, Finland
7  University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA 94720-7450, USA
    e-mail: khurley@ssl.berkeley.edu

(Received 25 September 2001 / Accepted 3 December 2001 )

We report optical observations of the short/hard burst GRB 010119 error box, one of the smallest error boxes reported to date for short/hard GRBs. Limits of R > 22.3 and I > 21.2 are imposed by observations carried out 20.31 and 20.58 hours after the gamma-ray event, respectively. They represent the most constraining limits imposed to date on the optical emission from a short/hard gamma-ray burst afterglow.

Key words: gamma rays: bursts -- methods: observational -- techniques: photometric

Offprint request: J. Gorosabel, jgu@dsri.dk

SIMBAD Objects

© ESO 2002