GCN Circular 15514
Subject
GRB 131122A: Upper limit from NOT imaging
Date
2013-11-23T10:49:11Z (10 years ago)
From
Antonio de Ugarte Postigo at IAA-CSIC <deugarte@iaa.es>
A. de Ugarte Postigo (IAA-CSIC, DARK/NBI), J. Gorosabel (IAA-CSIC/UPV-EHU),
D. Xu (DARK/NBI), S. Schulze (PUC, MCSS), N.R. Tanvir (U. Leicester),
O. Smirnova (NOT, U. Latvia), J. K�re (U. Oslo), E. Pakstiene (Vilnius U.),
A.B. Aksnes, C. Eide, E.N. Traore, J. Joberg, L.K. Seljebotn, N. Von Huth,
M. Lapadatu, R.W. Cale, M Heger (Horten videreg�ende skole) report on
behalf of a larger collaboration:
Further analysis of our i-band imaging from the 2.5 m NOT (Gorosabel et al.,
GCN 15512) of GRB 131122A (Gotz et al., GCN 15510), with mean epoch
00:49 UT (3.40 hr after the burst), shows no new source within the Swift-XRT
error box (Maselli et al., GCN 15513) down to a 3-sigma magnitude limit of
i=23.5 (AB).