GCN Circular 5919
Subject
GRB 061214(?): ROTSE-III Optical Limits
Date
2006-12-14T13:07:05Z (18 years ago)
From
Fang Yuan at ROTSE <yuanfang@umich.edu>
F. Yuan (U Mich), B. E. Schaefer (Louisiana State), T. Guver (U
Istanbul), D.A. Smith (Guilford) report on behalf of the ROTSE
collaboration:
ROTSE-IIIa, located at Siding Spring Observatory, Australia, responded
to the possible burst GRB 061214 (Swift trigger 250908), producing
images beginning 7.0 s after the GCN notice time. An automated response
took the first image at 12:17:12.1 UT, 18.7 s after the burst, under
fair conditions. We took 10 5-sec, 10 20-sec and 20 60-sec exposures.
These unfiltered images are calibrated relative to USNO A2.0 (R).
Comparison to the DSS (second epoch) reveals no new sources within the
3-sigma error circle, for both single images and coadding into sets of
10. Individual images have limiting magnitudes ranging from 14.9-16.8;
we set the following specific limits.
start UT end UT t_exp(s) mlim t_start-tGRB(s) Coadd?
--------------------------------------------------------------------
12:17:12.1 12:19:32.0 139 17.1 18.7 Y
12:19:40.7 12:24:31.2 290 17.5 167.3 Y