Skip to main content
Testing. You are viewing the public testing version of GCN. For the production version, go to https://gcn.nasa.gov.
New Announcement Feature, Code of Conduct, Circular Revisions. See news and announcements

GCN Circular 8639

Subject
GRB 081128: afterglow observations
Date
2008-12-08T08:35:39Z (15 years ago)
From
Daniele Malesani at Dark Cosmology Centre, Niels Bohr Inst <malesani@astro.ku.dk>
D. Malesani, J.P.U. Fynbo, G. Leloudas (DARK/NBI), H. Pedersen (NBI), P. 
Jakobsson (Univ. Iceland), S.-M. Niemi, H. Uthas, and C. Villforth 
(NOT), report on behalf of a larger collaboration:

We observed the field of GRB 081128 (Margutti et al., GCN 8571) with the 
Nordic Optical Telescope equipped with ALFOSC. Observations were carried 
out on two epochs, first on 2008 Nov 28.962 (0.24 days after the GRB) in 
the V, R and i bands and then on Dec 7.827 (9.10 days after the GRB) in 
the R band. In the first epoch we detect the afterglow candidate 
reported by Wang et al. (GCN 8572) in all filters. We estimate R=22.3 +- 
0.1 assuming R=17.91 for the USNO star at RA = 01:23:11.73, Dec = 
+38:07:43.58 (consistent with the calibration of Guidorzi et al., GCN 
8577; C. Guidorzi, priv. comm.). In the second epoch, the afterglow 
candidate remains undetected to a limit R > 23.5, and we hence confirm 
that this source is the GRB afterglow. We note that the V-band detection 
sets a limit on the GRB redshift, z <~ 5.

We also detect in both epochs a second object at the border of the XRT 
error circle (RA = 01:23:12.98, Dec = +38:07:38.4), which is likely the 
one reported by Guidorzi et al. (GCN 8577), with a magnitude R = 22.7. 
The angular separation from the afterglow is 1.2".
Looking for U.S. government information and services? Visit USA.gov