GCN Circular 5345
Subject
GRB060719: FRAM early follow-up limit
Date
2006-07-19T10:56:18Z (19 years ago)
Edited On
2024-11-18T09:54:32Z (2 months ago)
From
Martin Jelinek at Inst.Astrophys.Andalucia,Granada <mates@iaa.es>
Edited By
Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov> on behalf of Leo P. Singer at NASA/GSFC <leo.p.singer@nasa.gov>
Martin Jelínek (IAA Granada, Spain),
Petr Kubánek (ISDC Versoix, Switzerland and ASU Ondrejov, Czech Rep.) and
Michael Prouza (Columbia University New York, USA and FZU Praha, Czech Rep.)
on behalf of the FRAM team, coordinated by FZU Praha, Czech Rep.
report
"Robotic telescope FRAM followed the Swift trigger #220020. 5x
20s R-band (lambda_eff = 640nm) images were obtained starting
112.4s after the GRB (99.5s after receiving the notification).
On the coadded frame with exposure mean time 180s after the GRB
we do not detect any new source down to the limiting magnitude
R=~16.2."
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