TITLE: GCN CIRCULAR NUMBER: 17519 SUBJECT: GRB 150301A: Swift-BAT refined analysis DATE: 15/03/01 22:13:47 GMT FROM: Amy Lien at GSFC T. Sakamoto (AGU), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), J. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL), M. Stamatikos (OSU), J. Tueller (GSFC), T. N. Ukwatta (LANL) (i.e. the Swift-BAT team): Using the data set from T-210 to T+962 sec from the recent telemetry downlink, we report further analysis of BAT GRB 150301A (trigger #632995) (Lien, et al., GCN Circ. 17510). The BAT ground-calculated position is RA, Dec = 244.281, -48.732 deg which is RA(J2000) = 16h 17m 07.5s Dec(J2000) = -48d 43' 56.2" with an uncertainty of 1.9 arcmin, (radius, sys+stat, 90% containment). The partial coding was 96%. The mask-weighted light curve shows a single short FRED peak that starts at ~ T0 and ends at ~ T+0.5 s. T90 (15-350 keV) is 0.48 +- 0.14 sec (estimated error including systematics). The time-averaged spectrum from T+0.00 to T+0.56 sec fit by a simple power-law model has a power law index of 1.44 +- 0.23 (chi squared 54.10 for 57 d.o.f.). The fluence in the 15-150 keV band is 7.4 +- 1.0 x 10^-8 erg/cm2. The 1-sec peak photon flux measured from T-0.22 sec in the 15-150 keV band is 1.0 +- 0.2 ph/cm2/sec. A single blackbody fit to the time-averaged spectrum shows a blackbody temperature of 15.11 +- 2.92 keV (chi squared 74.66 for 57 d.o.f.). A thermal bremsstrahlung model fit shows the temperature of 199.36 keV (chi squared 55.72 for 57 d.o.f.). Despite being near the Galactic Plane and Bulge (lat = 1.36, lon = 334), both the fast-decaying XRT light curve and Fermi/GBM observation (Connaughton et al., GCN Circ. 17511) suggests that this source is more likely to be a short GRB than a SGR. In addition, there are no other BAT detections of this source before or since this trigger. The results of the batgrbproduct analysis are available at http://gcn.gsfc.nasa.gov/notices_s/632995/BA/