GCN Circular 15488
Subject
GRB 131110A: Swift-XRT and UVOT upper limits
Date
2013-11-15T15:29:45Z (10 years ago)
From
Kim Page at U.of Leicester <klp5@leicester.ac.uk>
K.L. Page, P.A. Evans (U. Leicester) and N.P.M. Kuin (UCL-MSSL) report on
behalf of the Swift-XRT and UVOT teams:
The Swift-XRT began observing the field of GRB 131011A 397 ks after the
event (Cummings & Palmer, GCN Circ. 15483). In 2.8 ks of Photon Counting
(PC) mode data, no source was found in the BAT error circle; the 3-sigma
upper limit (0.3-10 keV) is 3.6e-3 count s^-1
The Swift-UVOT also began observations of the field of GRB 131110A�at the
same time. No optical afterglow was found in the image. Preliminary
3-sigma upper limits using the UVOT photometric system (Breeveld et al.
2011, AIP Conf. Proc. 1358, 373) for the� initial exposures are:
Filter � � � � T_start(s) � T_stop(s) � � �Exp(s) � � � � Mag
white � � � � � 397556 � � � 409058 � � � � 892 � � � � �>20.2
v � � � � � � � 398095 � � � 409489 � � � � 938 � � � � �>18.6
u � � � � � � � 397018 � � � 408678 � � � � 892 � � � � �>19.2
This circular is an official product of the Swift team.