Astron. Astrophys. Suppl. Ser. 138, 461-462
J. Hjorth1 - H. Pedersen1 - A.O. Jaunsen2 - M.I. Andersen3
Send offprint request: J. Hjorth; jens@astro.ku.dk
1 -
Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, DK-2100
Copenhagen Ø, Denmark
2 -
Institute of Theoretical Astrophysics, University of Oslo, Blindern, N-0315 Oslo,
Norway
3 -
Nordic Optical Telescope, Ap. 474, St. Cruz de La Palma, E-38700 Canarias, Spain
Received December 29, 1998; accepted April 21, 1999
Using the 2.56-m Nordic Optical Telescope (NOT) on La Palma we have observed
most of the known optical afterglows to gamma-ray bursts (GRBs). We here
briefly report on the discoveries of the optical afterglows of two
recent SAX GRBs (GRB 980519 and GRB 980613) and the detection of their host
galaxies. GRB 980519 was bright upon discovery () and occurred in
a faint () galaxy whereas GRB 980613 was faint upon discovery
() but occurred in a bright galaxy (). Both host
galaxies may show signs of interaction. GRB 980519 led to the earliest reported
optical identification to date. We describe our continued efforts to produce
optical identifications soon after optical observations have begun.
Key words:
cosmology: observations --
gamma-rays: bursts
Copyright The European Southern Observatory (ESO)