GCN Circular 4503
Subject
GRB 060108: IR observations of afterglow
Date
2006-01-14T00:32:39Z (18 years ago)
From
Andrew Levan at U.of Leicester <anl@star.le.ac.uk>
A.J. Levan, N.R. Tanvir (U. Hertfordshire), L. Fuhrman (JACH) report
on behalf of a larger collaboration.
Our UKIRT K-band observations of GRB 060108 reported originally
in GCN 4457 also show an object at the location of the revised X-ray
afterglow position suggested by Butler & Bloom (GCN 4500). The source is
point like and has a magnitude of approximately K=18.4. The implied i-K
colour based on the optical detection at 35 minutes (Monfardini et al. GCN
4502) is i-K ~ 3.
We note that inspection of the SDSS g-band pre-image of the field of GRB
060108 also reveals a marginal detection at the location of this source,
presumably the host galaxy.
Further observations are planned.