[vsnet-grb-info 3936] GRB061025: ROTSE-III Confirmation of Optical
Counterpart
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Fri Oct 27 04:56:23 JST 2006
TITLE: GCN CIRCULAR
NUMBER: 5759
SUBJECT: GRB061025: ROTSE-III Confirmation of Optical Counterpart
DATE: 06/10/26 19:56:13 GMT
FROM: Fang Yuan at ROTSE <yuanfang at umich.edu>
F. Yuan (U Mich), E.S. Rykoff (U Mich) report on behalf of the ROTSE
collaboration:
Further analysis of the early ROTSE-IIIc images (Rykoff, et al, GCN
5752) reveals a faint, fading afterglow at the XRT position (Mineo, et
al, GCN 5753) consistent with the position of the i-band candidate
reported by Berger (GCN 5754). This source was not detected in the
original analysis because of source confusion with a nearby star, and
because the afterglow is near our detection threshold.
In our initial 5 s image beginning at 18:36:46.6 UT, 44.7 s after the
burst, the afterglow is at 15.6+/-0.2 mag calibrated relative to USNO
B1.0 (R). It decays with a power law index ~ -0.9 up to ~155 s after
the burst when it is no longer detected.
start UT end UT t_exp(s) mag t_start-tGRB(s) Coadd?
--------------------------------------------------------------------
18:36:46.6 18:36:51.6 5 15.6+/-0.2 44.7 N
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