{
  "bibcode": "2022GCN.32329....1D",
  "body": "A. D'Ai (INAF-IASFPA), E. Ambrosi (INAF-IASFPA),\nV. D'Elia (SSDC & INAF-OAR), J.D. Gropp (PSU), J. A. Kennea (PSU),\nN. J. Klingler (GSFC/UMBC/CRESSTII), S. Laha (GSFC/UMBC),\nF. E. Marshall (NASA/GSFC), K. L. Page (U Leicester),\nT. M. Parsotan (GSFC/UMBC/CRESSTII), M. H. Siegel (PSU) and\nM. A. Williams (PSU) report on behalf of the Neil Gehrels Swift\nObservatory Team:\n\nAt 16:09:14 UT, the Swift Burst Alert Telescope (BAT) triggered and\nlocated GRB 220706A (trigger=1114937).  Swift slewed immediately to the burst. \nThe BAT on-board calculated location is \nRA, Dec 0.587, -16.391 which is \n   RA(J2000) = 00h 02m 21s\n   Dec(J2000) = -16d 23' 28\"\nwith an uncertainty of 3 arcmin (radius, 90% containment, including \nsystematic uncertainty).  The BAT light curve showed a complex structure\n with a duration of about 50 sec.  The peak count rate\nwas ~1400 counts/sec (15-350 keV), at ~1 sec after the trigger. \n\nThe XRT began observing the field at 16:10:57.0 UT, 102.8 seconds after\nthe BAT trigger. Using promptly downlinked data we find an uncatalogued\nX-ray source located at RA, Dec 0.60368, -16.41065 which is equivalent\nto:\n   RA(J2000)  = 00h 02m 24.88s\n   Dec(J2000) = -16d 24' 38.3\"\nwith an uncertainty of 3.5 arcseconds (radius, 90% containment). This\nlocation is 91 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 https://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 (2.40 x\n10^20 cm^-2, Willingale et al. 2013), with an excess column of 6.6\n(+4.12/-3.33) x 10^21 cm^-2 (90% confidence). \n\nUVOT took a finding chart exposure of 150 seconds with the White filter\nstarting 107 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\n0.025. \n\nBurst Advocate for this burst is A. D'Ai (antonino.dai AT inaf.it). \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": 32329,
  "createdOn": 1657124839000,
  "email": "antonino.dai@inaf.it",
  "subject": "GRB 220706A: Swift detection of a burst",
  "submitter": "Antonino D'Ai at IASF-PA  <antonino.dai@inaf.it>",
  "eventId": "GRB 220706A"
}