{
  "bibcode": "2011GCN.12199....1S",
  "body": "M.H. Siegel (PSU) and C. A. Wolf (PSU) report on behalf\nof the Swift/UVOT team:\n\nSwift/UVOT began observations of the field of GRB 110726A (Wolf et al. 2011,\nGCN 12196) 59 seconds after the BAT trigger.  The 150 second finding chart\nin the White filter reveals a candidate afterglow in the rapidly available\n2.7'x2.7' sub-image at:\n\n RA(J2000) =     19:06:52.06 = 286.71693\n DEC(J2000) = +56:04:16.6  = 56.0713\n\nwith a 90%-confidence error radius of about 0.6 arc sec. This is consistent\nwith the afterglow reported by both the XRT (Wolf et al.) and ROTSE (Schaefer\net al., 2011, GCN 12197).  The estimated magnitude is 17.80 with a 1-sigma\nerror of about  0.06. No correction has been made for the expected extinction\ncorresponding to E(B-V) of 0.08.",
  "circularId": 12199,
  "createdOn": 1311652960000,
  "email": "siegel@astro.psu.edu",
  "subject": "GRB 110726A: Swift/UVOT Detection",
  "submitter": "Mike Siegel at PSU/Swift MOC  <siegel@astro.psu.edu>",
  "eventId": "GRB 110726A"
}