TITLE: GCN CIRCULAR NUMBER: 40356 SUBJECT: GRB 250430A: Swift-BAT refined analysis DATE: 25/05/06 02:50:20 GMT FROM: Mike Moss at NASA GSFC mikejmoss3@gmail.com
M. J. Moss (GSFC), S. D. Barthelmy (GSFC), R. Gupta (GSFC), H. A. Krimm (NSF), S. Laha (GSFC/UMBC), A. Y. Lien (U Tampa), C. B. Markwardt (GSFC), 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-61 to T+242 sec from the recent telemetry downlink, we report further analysis of BAT GRB 250430A (trigger #1308754) (Parsotan, et al., GCN Circ. 40292). The BAT ground-calculated position is RA, Dec = 233.395, -18.101 deg which is RA(J2000) = 15h 33m 34.7s Dec(J2000) = -18d 06' 03.2" with an uncertainty of 1.1 arcmin, (radius, sys+stat, 90% containment). The partial coding was 72%.
The mask-weighted light curve displays a double peaked structure. The T90 (15-350 keV) is 9.17 +- 1.70 sec (estimated error including systematics).
The time-averaged spectrum from T+0.10 to T+11.86 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.66 +- 0.11. The fluence in the 15-150 keV band is 8.9 +- 0.6 x 10^-07 erg/cm2. The 1-sec peak photon flux measured from T+0.31 sec in the 15-150 keV band is 2.3 +- 0.2 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/1308754
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