{
  "bibcode": "2020GCN.27428....1D",
  "body": "S. Dichiara (NASA/GSFC/UMCP), S. D. Barthelmy (GSFC),\nA. P. Beardmore (U Leicester), M. G. Bernardini (INAF-OAB),\nP. D'Avanzo (INAF-OAB), V. D'Elia (SSDC), J.D. Gropp (PSU),\nJ. A. Kennea (PSU), N. J. Klingler (PSU), S. Laha (GSFC/UMBC/CRESST),\nF. E. Marshall (NASA/GSFC), A. Melandri (INAF-OAB),\nK. L. Page (U Leicester), D. M. Palmer (LANL), T. Sbarrato (INAF-OAB),\nB. Sbarufatti (PSU) and T. N. Ukwatta (LANL) report on behalf of the\nNeil Gehrels Swift Observatory Team:\n\nAt 16:39:07 UT, the Swift Burst Alert Telescope (BAT) triggered and\nlocated GRB 200324A (trigger=963260).  Swift slewed immediately to the burst. \nThe BAT on-board calculated location is \nRA, Dec 222.685, +35.968 which is \n   RA(J2000) = 14h 50m 44s\n   Dec(J2000) = +35d 58' 06\"\nwith an uncertainty of 3 arcmin (radius, 90% containment, including \nsystematic uncertainty).  The BAT light curve showed a complex\nstructure with a duration of about 60 sec.  The peak count rate\nwas ~1200 counts/sec (15-350 keV), at ~2 sec after the trigger. \n\nThe XRT began observing the field at 16:42:11.8 UT, 183.9 seconds after\nthe BAT trigger. Using promptly downlinked data we find a bright,\nfading, uncatalogued X-ray source located at RA, Dec 222.67198,\n35.94100 which is equivalent to:\n   RA(J2000)  = 14h 50m 41.28s\n   Dec(J2000) = +35d 56' 27.6\"\nwith an uncertainty of 3.5 arcseconds (radius, 90% containment). This\nlocation is 104 arcseconds from the BAT onboard position, within the\nBAT error circle. This position may be improved as more data are\nreceived; the latest position is available at\nhttps://www.swift.ac.uk/sper. \n\nA power-law fit to a spectrum formed from promptly downlinked event\ndata gives a column density in excess of the Galactic value (1.07 x\n10^20 cm^-2, Willingale et al. 2013), with an excess column of 3.9\n(+2.21/-1.93) x 10^21 cm^-2 (90% confidence). \n\nThe initial flux in the 2.5 s image was 1.27e-09 erg cm^-2 s^-1 (0.2-10\nkeV). \n\nUVOT took a finding chart exposure of 150 seconds with the White filter\nstarting 194 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\n0.01. \n\nThis source lies within the current (Sector 23) field-of-view of TESS camera 2. \n\nBurst Advocate for this burst is S. Dichiara (dichiara AT umd.edu). \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/)",
  "circularId": 27428,
  "createdOn": 1585069022000,
  "email": "palmer@lanl.gov",
  "subject": "GRB 200324A: Swift detection of a burst",
  "submitter": "David Palmer at LANL  <palmer@lanl.gov>",
  "eventId": "GRB 200324A"
}