{
  "bibcode": "2014GCN.17140....1M",
  "body": "C. B. Markwardt (GSFC), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC),\nJ. R. Cummings, N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), A. Y. Lien (GSFC/UMBC),\nD. M. Palmer (LANL), T. Sakamoto (AGU), M. Stamatikos (OSU), J. Tueller (GSFC),\nT. N. Ukwatta (LANL), A. Vargas (PSU)\n(i.e. the Swift-BAT team):\n\nWe report further analysis of GRB 141205A (Cummings, GCN 17137).  The best\nBAT position is RA, Dec  92.859, +37.876, which is:\n\nRA (J2000)    06 11 26.1s\nDec (J2000)  +37d 52' 32.2\"\n\nwith an estimated position uncertainty of 2 arcmin radius.  The source was\n41% coded in BAT.\n\nThe unweighted lightcurve shows multiple weak peaks.  T90 was 1.1 +- 0.2\nseconds.\n\nThe total spectrum in  BAT is best fit by a simple power-law function with\na photon index of 0.985 +- 0.002.  The fluence in 1.4 seconds was\n(1.2 +- 0.3) x 10^-7 ergs/cm^2.  Errors are 90% confidence.\n\nBecause this burst was found in ground analysis, the normal automated burst\nanalysis products are not available.",
  "circularId": 17140,
  "createdOn": 1417797724000,
  "email": "james.r.cummings@nasa.gov",
  "subject": "GRB 141205A Swift-BAT refined analysis",
  "submitter": "Jay R. Cummings at NASA/GSFC/Swift  <james.r.cummings@nasa.gov>",
  "eventId": "GRB 141205A"
}