TITLE: GCN CIRCULAR NUMBER: 36769 SUBJECT: GRB 240624A: Swift-BAT refined analysis DATE: 24/06/26 22:29:41 GMT FROM: Amy <yarleen@gmail.com> D. M. Palmer (LANL), S. D. Barthelmy (GSFC), R. Gupta (GSFC), H. A. Krimm (NSF), S. Laha (GSFC/UMBC), A. Y. Lien (U Tampa), C. B. Markwardt (GSFC), M. J. Moss (GSFC), T. Parsotan (GSFC), D. Sadaula (GSFC/UMBC), T. Sakamoto (AGU) (i.e. the Swift-BAT team): Using the data set from T-240 to T+962 sec from the recent telemetry downlink, we report further analysis of BAT GRB 240624A (trigger #1238732) (Klingler et al., GCN Circ. 36743). The BAT ground-calculated position is RA, Dec = 102.473, -6.534 deg which is RA(J2000) = 06h 49m 53.6s Dec(J2000) = -06d 32' 02.8" with an uncertainty of 1.8 arcmin, (radius, sys+stat, 90% containment). The partial coding was 49%. The mask-weighted light curve shows a main structure with some overlapping pulses that starts at ~T-2 s and ends at ~T+6 s. The main peak occurs at ~T+1.5 s. T90 (15-350 keV) is 5.89 +- 2.25 sec (estimated error including systematics). The time-averaged spectrum from T-0.06 to T+7.04 sec is best fit by a power law with an exponential cutoff. This fit gives a photon index 0.07 +- 0.94, and Epeak of 78.3 +- 36.0 keV (chi squared 45.64 for 56 d.o.f.). For this model the total fluence in the 15-150 keV band is 4.5 +- 0.6 x 10^-7 erg/cm2 and the 1-sec peak flux measured from T+0.88 sec in the 15-150 keV band is 2.2 +- 0.3 ph/cm2/sec. A fit to a simple power law gives a photon index of 1.33 +- 0.18 (chi squared 52.69 for 57 d.o.f.). 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/1238732 View this GCN Circular online at https://gcn.nasa.gov/circulars/36769. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...