{
  "bibcode": "2005GCN..4190....1C",
  "body": "J. Cummings (GSFC/NRC), L. Barbier (GSFC), S. Barthelmy (GSFC),\nM. Chester (PSU), E. Fenimore (LANL), N. Gehrels (GSFC),\nD. Hullinger (UMD), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD),\nF. Marshall (GSFC), D. Palmer (LANL), A. Parsons (GSFC),\nT. Sakamoto (GSFC/NRC), G. Sato (ISAS), J. Tueller (GSFC),\non behalf of the Swift-BAT team:\n\nUsing the data set from T-60 to T+120 sec from the recent telemetry\ndownlink, we confirm the short duration of GRB 051105\n(trigger #162580)  (Mineo, et al., GCN 4188). The BAT ground position\nis (RA,Dec) =  265.288,+34.904 {17h 41m 09s,+34d 55' 15\"} [deg; J2000]\n+-1.3 arcmin, (radius, sys+stat, 90% containment).  The partial coding was 89%.\n\nThe light curve shows a single peak with a fast rise and a slower decay.\nT90 (15-350 keV) is (0.028 +- 0.004) sec. (estimated error including\nsystematics). All of the emission appears to be below 100 keV.\n\nSpectral analysis including flux values will follow in a later circular.",
  "circularId": 4190,
  "createdOn": 1131192186000,
  "email": "krimm@milkyway.gsfc.nasa.gov",
  "subject": "GRB 051105: Swift-BAT refined analysis",
  "submitter": "Hans Krimm at NASA-GSFC  <krimm@milkyway.gsfc.nasa.gov>",
  "eventId": "GRB 051105"
}