TITLE: GCN CIRCULAR NUMBER: 40812 SUBJECT: GRB 250617B: Swift-BAT refined analysis DATE: 25/06/23 11:39:14 GMT FROM: Takanori Sakamoto at AGU <tsakamoto@phys.aoyama.ac.jp> S. Laha (GSFC/UMBC), S. D. Barthelmy (GSFC), R. Gupta (GSFC), H. A. Krimm (NSF), A. Y. Lien (U Tampa), C. B. Markwardt (GSFC), M. J. Moss (GSFC), K. L. Page (U Leicester), D. M. Palmer (LANL), T. Parsotan (GSFC), D. Sadaula (GSFC/UMBC), T. Sakamoto (AGU) (i.e. the Swift-BAT team): Using the data set from T-273 to T+962 sec from the recent telemetry downlink, we report further analysis of BAT GRB 250617B (trigger #1325580) (Page, et al., GCN Circ. 40760). The BAT ground-calculated position is RA, Dec = 332.883, 32.721 deg which is RA(J2000) = 22h 11m 31.8s Dec(J2000) = +32d 43' 14.5" with an uncertainty of 1.9 arcmin, (radius, sys+stat, 90% containment). The partial coding was 10%. The mask-weighted light curve shows two peaks. The emission starts at T-30 sec, peaks at T+1 sec, and ends at T+18 sec. T90 (15-350 keV) is 36.5 +- 6.9 sec (estimated error including systematics). The time-averaged spectrum from T-29.32 to T+14.30 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 2.13 +- 0.22. The fluence in the 15-150 keV band is 2.3 +- 0.3 x 10^-6 erg/cm2. The 1-sec peak photon flux measured from T+0.19 sec in the 15-150 keV band is 2.9 +- 0.8 ph/cm2/sec. All the quoted errors are at the 90% confidence level. The results of the batgrbproduct analysis are available at https://swift.gsfc.nasa.gov/results/batgrbcat/BAT_refined_circular/1325580 View this GCN Circular online at https://gcn.nasa.gov/circulars/40812. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...