GCN Circular 38025

T. M. Parsotan (GSFC), S. Dichiara (PSU), R. Gupta (NASA GSFC),
T. Sakamoto (AGU) and T. Sbarrato (INAF-OAB) report on behalf of the
Neil Gehrels Swift Observatory Team:

At 05:41:45 UT, the Swift Burst Alert Telescope (BAT) triggered and
located GRB 241101A (trigger=1264304).  The BAT on-board calculated location is 
RA, Dec 204.333, +28.264 which is 

  RA(J2000)  = 13h 37m 20s
  Dec(J2000) = +28d 15' 49"

with an uncertainty of 3 arcmin (radius, 90% containment, including 
systematic uncertainty).  The BAT light curve showed a double-peaked 
structure with a duration of about 15 sec.  The peak count rate
was ~2300 counts/sec (15-350 keV), at ~1 sec after the trigger.

Due to a Sun observing constraint, Swift cannot slew to the BAT
position until 17:57 UT on 2024 November 05. There will thus be no XRT
or UVOT data for this trigger before this time.

Burst Advocate for this burst is T. M. Parsotan (tyler.parsotan AT nasa.gov).
Please contact the BA by email if you require additional information
regarding Swift followup of this burst. In extremely urgent cases, after
trying the Burst Advocate, you can contact the Swift PI by phone (see
Swift TOO web site for information: http://www.swift.psu.edu/)