[AAVSO-HEN] GRB 060115: Swift/UVOT upper limits

[grb at aavso.org]

The following is a GCN Circular circulated via the AAVSO network.
For an archive and more information on circulars visit:
http://lheawww.gsfc.nasa.gov/docs/gamcosray/legr/bacodine/gcn3_archive.html

TITLE:   GCN GRB OBSERVATION REPORT
NUMBER:  4516
SUBJECT: GRB 060115: Swift/UVOT upper limits
DATE:    06/01/16 00:13:52 GMT
FROM:    Patricia Schady at MSSL/Swift  <ps at mssl.ucl.ac.uk>

P. Schady (UCL-MSSL/PSU),  A. Cucchiara (PSU), M. De Pasquale (UCL-MSSL), F. 
Marshall (GSFC), N. Gehrels (GSFC) on behalf of the Swift/UVOT team

The Swift/UVOT began observing the field of GRB 060115 at 13:09:59 on 
2006-01-15 whilst settling on the target, 119 s after the BAT trigger 
(Tagliagerri et al., GCN 4509). No new source is detected either at the XRT 
position (Perri et al., GCN 4514) or at the position of the candidate afterglow 
reported by Yanagisawa et al. (GCN 4510) in coadded images with any of the 
filters. The following 3-sigma magnitude upper limits are not corrected for 
Galactic extinction; E(B-V) = 0.133.

Filter   T_range(s)  Exp(s)  3sigUL(mag)

V        104-1585    488.1   19.5
B        326-1042    199.7   20.4
U        651-1657    99.0    19.3
W1       627-1788    105.9   19.4
M2       603-1777    118.8   19.5
W2       556-1730    99.0    19.7
White    531-1705    99.0    19.8

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