TITLE: GCN GRB OBSERVATION REPORT NUMBER: 2987 SUBJECT: GRB050126: Burst Parameters Measured by BAT DATE: 05/01/26 18:19:56 GMT FROM: Goro Sato at ISAS/JAXA G. Sato (ISAS), P. Boyd (GSFC-UMBC), S. Barthelmy, L. Barbier (GSFC), J. Cummings (GSFC), E. Fenimore (LANL), N. Gehrels (GSFC), D. Hullinger (GSFC/UMD), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), C. Milvia (ASDC), K. McLean (LANL), J. Nousek (PSU), D. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC), M. Suzuki (Saitama), J. Tueller (GSFC) on behalf of the Swift-BAT team: At 12:00:53 UT, the Swift Burst Alert Telescope (BAT) triggered and located on-board GRB050126. The spacecraft autonomously slewed to the burst and was detected by Swift/XRT as well (Kinnea et al., GCN #2984). The burst is a FRED-type single broad peak, with a rapid rise (~1 sec) and total duration ~30 seconds (T50 = 14 sec, T90 = 26 sec). The total fluence is 1.1e-6 erg/cm2 (15-350 keV), and the peak five second flux is 0.4 ph/cm2/sec (15-350 keV). The spectrum is consistent with a power law with photon index 1.3 +/- 0.1 in the 20-150 keV band. The spacecraft slew occurred between times 12:01:41 and 12:02:32 UT, with a subsequent settling period until 12:03:02 UT. From 12:02:32 onward, there is no detectable gamma ray emission with an approximate 2 sigma upper limit of 7e-9 erg/cm2/s (15-350 keV) based on the above spectrum. The BAT ground-derived position is RA,Dec = 278.111, 42.384 (J2000) with an estimated uncertainty of 4 arcmin (radius, 3-sigma, including a systematic uncertainty). This is within 62 arcsec of the XRT position (GCN #2984), and within 22 arcsec of the BAT on-board derived position.