TITLE: GCN CIRCULAR NUMBER: 17516 SUBJECT: GRB 150301C : (Swift trigger 633105) Swift observations DATE: 15/03/01 20:31:02 GMT FROM: Jay R. Cummings at NASA/GSFC/Swift M. Stamatikos (OSU), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), J. R. Cummings (CPI), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL), T. Sakamoto (AGU), J. Tueller (GSFC), T. N. Ukwatta (LANL), F. Marshall (NASA/GSFC), D. Malesani (DARK/NBI), L. Hagen (PSU), M. de Pasquale (INAF-IASFPA), A. Maselli (INAF-IASFPA), D.N. Burrows (PSU), K. Page (U. Leicester), N. P. M. Kuin (UCL-MSSL) Using the data set from T-60 to T+243 sec from the recent telemetry downlink, we report further analysis of possible GRB 150301C (trigger #633105) (Lien, et al., GCN Circ. 17512). The BAT ground-calculated position is RA, Dec = 11.319, 41.861 deg which is RA(J2000) = 00h 45m 16.6s Dec(J2000) = +41d 51' 40.0" with an uncertainty of 2.2 arcmin, (radius, sys+stat, 90% containment). The significance in the BAT image was 10.1, so we are sure that this was a real astrophysical source. The partial coding was 69%. The location is well within the visible light of M31. A more distant galaxy, [JSD2012] 170, which has a size of 0.11 arcmin, is within the BAT error circle. In 1.9 ks of data, the Swift XRT found only a single very weak source (2.8 sigma), consistent with the position of a known source within the BAT error circle, [PFH2005] 622, with a count rate of (5.3+/-1.9) x 10^-03 c/s. We cannot state whether there is any variability of this source at this time. The XRT position of this source is: RA (J2000) 00h 45m 14.4s Dec (J2000) +41d 50' 37.7" The BAT mask-weighted light curve shows a single weak FRED peak. T90 (15-350 keV) is 14 +- 3 sec (estimated error including systematics). The time-averaged BAT spectrum from T-0.6 to T+15.0 sec is best fit by a power- law model with an exponential cutoff. The power law index of the time-averaged spectrum is poorly defined but is nominally -0.8 +- 2. The peak energy is 38 +- 7 keV. The fluence in the 15-150 keV band is 2.1 +- 0.4 x 10^-07 erg/cm2. The 1-sec peak photon flux measured from T+1.32 sec in the 15-150 keV band is 0.6 +- 0.2 ph/cm2/sec. A simple power-law fit has a photon index of 1.96 +- 0.25. All the quoted errors are at the 90% confidence level. If this source was in M31, its isotropic energy output was 1.5 x 10^43 ergs in 15.6 seconds in the range 15-150 keV. It is very possible, given the softness of the source, that this is a non-GRB in M31. The color:duration is within the distribution of long GRBs. No XRT source was seen in the initial observations, whereas we might expect most sources in M31 bright enough to be seen in BAT would be very bright in XRT. Therefore the source is likely to be highly absorbed. The results of the batgrbproduct analysis are available at http://gcn.gsfc.nasa.gov/notices_s/633105/BA/ The Swift/UVOT began settled observations of the field 102 s after the BAT trigger (Lien et al., GCN Circ. 17512). No new source within the BAT error circle is detected in the initial UVOT exposures. Preliminary 3-sigma upper limits using the UVOT photometric system (Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the first exposures are: Filter T_start(s) T_stop(s) Exp(s) Mag white 102 4151 369 >20.39 v 592 4562 216 >18.55 b 518 5241 96 >19.08 u 261 5177 461 >19.69 uvw1 641 4973 216 >19.27 uvm2 617 4768 216 >19.20 uvw2 568 4357 216 >19.41 The magnitudes in the table are not corrected for the Galactic extinction due to the reddening of E(B-V) = 0.06 in the direction of the burst (Schlegel et al. 1998). Further Swift observations are planned. [GCN OPS NOTE(01mar15): Per author's request, the affiliation was corrected for KP.]