{
  "bibcode": "2012GCN.13357....1P",
  "body": "C. Pagani (U Leicester), S. D. Barthelmy (GSFC),\nW. H. Baumgartner (GSFC/UMBC), J. R. Cummings (NASA/UMBC),\nS. T. Holland (STScI), J. A. Kennea (PSU), F. E. Marshall (NASA/GSFC),\nD. M. Palmer (LANL) and M. H. Siegel (PSU) report on behalf of the\nSwift Team:\n\nAt 02:05:19 UT, the Swift Burst Alert Telescope (BAT) triggered and\nlocated GRB 120612A (trigger=524128).  Swift slewed immediately to the burst. \nThe BAT on-board calculated location is \nRA, Dec 126.726, -17.578 which is \n   RA(J2000)  =  08h 26m 54s\n   Dec(J2000) = -17d 34' 39\"\nwith an uncertainty of 3 arcmin (radius, 90% containment, including \nsystematic uncertainty).  The BAT light curve shows s single broad peak\nwith a duration of about 30 sec.  The peak count rate\nwas ~1250 counts/sec (15-350 keV), at ~7 sec after the trigger. \n\nThe XRT began observing the field at 02:07:38.1 UT, 138.5 seconds after\nthe BAT trigger. Using promptly downlinked data we find a bright,\nfading, uncatalogued X-ray source located at RA, Dec 126.72350,\n-17.57649 which is equivalent to:\n   RA(J2000)  = 08h 26m 53.64s\n   Dec(J2000) = -17d 34' 35.4\"\nwith an uncertainty of 3.9 arcseconds (radius, 90% containment). This\nlocation is 10 arcseconds from the BAT onboard position, within the BAT\nerror circle. This position may be improved as more data are received;\nthe latest position is available at http://www.swift.ac.uk/sper. \n\nA power-law fit to a spectrum formed from promptly downlinked event\ndata gives a column density consistent with the Galactic value of 5.49\nx 10^20 cm^-2 (Kalberla et al. 2005). \n\nThe initial flux in the 2.5 s image was 5.98e-10 erg cm^-2 s^-1 (0.2-10\nkeV). \n\nUVOT took a finding chart exposure of 150 seconds with the White filter\nstarting 147 seconds after the BAT trigger. No credible afterglow candidate has\nbeen found in the initial data products. The 2.7'x2.7' sub-image covers 100% of\nthe XRT error circle. The typical 3-sigma upper limit has been about 19.6 mag. \nThe 8'x8' region for the list of sources generated on-board covers 100% of the\nXRT error circle. The list of sources is typically complete to about 18 mag. No\ncorrection has been made for the expected extinction corresponding to E(B-V) of\n0.07. \n\nBurst Advocate for this burst is C. Pagani (cp232 AT star.le.ac.uk). \nPlease contact the BA by email if you require additional information\nregarding Swift followup of this burst. In extremely urgent cases, after\ntrying the Burst Advocate, you can contact the Swift PI by phone (see\nSwift TOO web site for information: http://www.swift.psu.edu/too.html.)",
  "circularId": 13357,
  "createdOn": 1339467497000,
  "email": "scott@milkyway.gsfc.nasa.gov",
  "subject": "GRB 120612A: Swift detection of a burst",
  "submitter": "Scott Barthelmy at NASA/GSFC  <scott@milkyway.gsfc.nasa.gov>",
  "eventId": "GRB 120612A"
}