GCN Circular 1429
Subject
GRB 020604, optical observations
Date
2002-06-13T18:38:21Z (23 years ago)
From
Javier Gorosabel at LAEFF-INTA, Madrid <jgu@laeff.esa.es>
J. Gorosabel (IAA-CSIC Granada), J. Hjorth, B. L. Jensen, H. Pedersen,
P. Jakobsson (Univ. of Copenhagen), J. Fynbo (IFA Aarhus),
M. I. Andersen (Univ. of Oulu), report:
We have carried out optical observations of the GRB 020604 IPN error box
(GCN 1417) with the 1.54 Danish Telescope (+DFOSC) on three epochs;
June 8, 9 and 10. The observations were done following a mosaic as
detailed below:
=====================================================================
Date UT Filter R.A. Dec Seeing Time since ExpTime
June 2002 (J2000) (J2000) (") GRB (days) (s)
---------------------------------------------------------------------
8.07874--8.11230 R 16:27:42.0 -29:48:43 1.2 3.50 4x600
8.11259--8.14516 R 16:28:39.8 -29:43:44 1.2 3.54 4x600
8.14642--8.16250 R 16:29:19.8 -29:39:44 1.1 3.56 2x600
8.16629--8.21525 R 16:28:01.7 -29:48:22 1.2 3.60 6x600**
8.21554--8.23159 R 16:27:18.4 -29:55:38 1.1 3.63 2x600
8.23186--8.23973 R 16:26:45.4 -29:52:52 1.0 3.64 600
8.27211--8.31829 I 16:28:01.7 -29:48:22 1.1 3.70 6x500**
8.32037--8.34111 I 16:28:39.8 -29:43:44 1.4 3.74 3x500
8.34216--8.36298 I 16:27:18.4 -29:55:38 1.8 3.76 3x500
---------------------------------------------------------------------
9.12684--9.21986 R 16:28:01.7 -29:48:22 1.1 4.58 10x600**
9.22098--9.26678 R 16:28:39.8 -29:43:44 1.2 4.65 4x600
9.27909--9.30354 R 16:27:18.4 -29:55:38 1.3 4.70 4x600
9.30392--9.31180 R 16:26:45.4 -29:52:52 1.3 4.72 600
9.31378--9.32165 R 16:27:42.0 -29:48:43 1.2 4.72 600
9.32416--9.33202 R 16:29:19.8 -29:39:44 1.5 4.74 600
---------------------------------------------------------------------
10.16572--10.24745 R 16:28:01.7 -29:48:22 1.0 5.61 6x900**
10.26606--10.30406 R 16:28:39.8 -29:43:44 1.3 5.69 3x900
10.30569--10.34051 R 16:27:18.4 -29:55:38 1.5 5.73 4x600
---------------------------------------------------------------------
** Central part
=====================================================================
The first and the second epoch observations cover the whole error box,
whereas the third epoch images contain ~80% of it.
A gif of the performed mosaic can be seen at:
http://www.dsri.dk/~jgu/grb020604/FCs/grb020604.R.8-9.06.02.1.54D.gif
The limiting magnitude depends on the error box position. For the central
pointing (covering ~50% of the error box), the R-band limiting magnitude
(3 sigma) at the three epochs are R=24.5, R=24.7 and R=24.9. For the rest
of the error box the limiting magnitude are R=23.8, R=23.6 and R=24.0,
respectively. In the I-band the limiting magnitude ranges from I=22.5 to
I=23.4.
Albeit the severe Galactic extinction (AR=1.18, AI=0.86 mag), many
extragalactic objects are detected in our images. Among the unsaturated
objects, marginal variability (< 0.2 mag) is detected for 12 of them.
None of these objects shows flux variability consistent with a decay, as
expected for an optical afterglow 3.5-5.7 days after the gamma ray event.