GCN Circular 1460
Subject
GRB020331: Late-time Optical Light Curve (re-submission)
Date
2002-07-24T19:13:51Z (22 years ago)
From
Alicia Soderberg at Caltech <ams@astro.caltech.edu>
In the previous submission (GCN 1459), there is a misprint
in the table of magnitudes. We report the correct values below.
The revised version of the GCN follows:
HST Epoch T (days since burst) R (mag)
1 23.9 24.54 +/- 0.07
2 36.6 24.86 +/- 0.10
3 42.7 25.01 +/- 0.09
4 49.3 24.76 +/- 0.11
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A. M. Soderberg, D. W. Fox, and S. R. Kulkarni (Caltech) report
on behalf of the larger Caltech-NRAO-CARA GRB collaboration.
"We have observed the optical afterglow associated with GRB 020331
(GCN 1334) with HST+STIS (Clear) at four epochs spanning the period
25-50 days following the burst (one orbit per epoch).
Registration of the STIS data against ground-based images allows us to
identify the afterglow amidst a complex of at least three galaxies,
including the presumed host galaxy which lies under the afterglow
itself. Aperture photometry on the optical transient + host yields
the following R-equivalent magnitudes for the four epochs:
HST Epoch T (days since burst) R (mag)
1 23.9 24.54 +/- 0.07
2 36.6 24.86 +/- 0.10
3 42.7 25.01 +/- 0.09
4 49.3 24.76 +/- 0.11
We have derived our R-equivalent magnitudes by assuming
(R-Clear)=-0.67 as given by the STIS Exposure Time Calculator for
a source with power-law spectrum (index=-1).
The first three epochs imply a power-law flux decay index over this
interval with index alpha=0.75, compatible with previous ground-based
estimates (Ricker et al., GCN 1382).
Preliminary analysis of the fourth epoch, T=50 days, indicates a
rebrightening of the optical afterglow by 0.2 +/- 0.1 mag as compared
with our Epoch 3. We have requested additional HST observations to
help us clarify whether this rebrightening is statistically significant.
A finding chart of the field can be found at:
http://www.astro.caltech.edu/~ams/grb020331.html
This message may be cited."