[AAVSO-HEN] GRB 060111: possible UVOT counterpart

grb at aavso.org grb at aavso.org
Wed Jan 11 08:38:15 EST 2006


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:  4482
SUBJECT: GRB 060111: possible UVOT counterpart
DATE:    06/01/11 13:31:24 GMT
FROM:    Alexander Blustin at MSSL-UCL  <ajb at mssl.ucl.ac.uk>

A. J. Blustin (UCL-MSSL), S. Zane (UCL-MSSL), S. R. Rosen (UCL-MSSL)
on behalf of the Swift/UVOT team

Further analysis of the initial UVOT data for GRB 060111 (Zane et al.,
GCN 4479) reveals a potential afterglow candidate at

RA,Dec (J2000) = 18:24:49.132  +37:36:14.47

within the refined XRT error circle (Goad et al., GCN 4481). The
source, significant at 8 sigma in an 3 arcsec radius aperture, has a
V band magnitude of 18.9 +/- 0.4 in a 200 s exposure starting at 72 s
after the BAT trigger. This magnitude is uncorrected for Galactic
extinction (E(B-V) ~0.1).



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