GRB240521B

This page lists all entries on GRB240521B in GRBweb

Summary Fermi GBM IPN GCN 36532 GCN 36535

Summary table
Variable Value Source
GRB_name_Fermi GRB240521631
T0 15:08:40.418 UTC Fermi_GBM
ra 355.6875° IPN
decl -32.7167° IPN
pos_error 5.00e-02° IPN
T90 33.792 s Fermi_GBM
T90_error 4.782 s Fermi_GBM
T90_start 15:08:40.418 UTC Fermi_GBM
fluence 2.80e-06 erg/cm² Fermi_GBM
fluence_error 4.33e-08 erg/cm² Fermi_GBM
T100 33.792 s
GBM_located False
mjd 60451.63102335648 Fermi_GBM
Fermi GBM table
GRB_name_Fermi GRB240521631
trigger_name bn240521631
ra 9.3800°
decl -43.6000°
pos_error 7.10e+00°
datum 2024-05-21
t_trigger 15:08:57.058 UTC
T90 33.792 s
T90_error 4.782 s
T90_start 15:08:40.418 UTC
fluence 2.80e-06 erg/cm²
fluence_error 4.33e-08 erg/cm²
flux_1024 4.05e+00 erg/cm²/s
flux_1024_error 4.07e-01 erg/cm²/s
flux_1024_time -9.92e+00 erg/cm²/s
flux_64 7.86e+00 erg/cm²/s
flux_64_error 1.81e+00 erg/cm²/s
IPN table
GRB_name GRB240521B
ra 355.6875°
decl -32.7167°
pos_error 5.00e-02°
GCN 36532 table
GRB_name GRB240521B
GCN_number 36532
Detection_method Swift Other
ra 355.6879°
decl -32.7215°
Circular_text TITLE: GCN CIRCULAR NUMBER: 36532 SUBJECT: GRB 240521B: Swift/BAT-GUANO arcminute localization of a long burst DATE: 24/05/22 17:41:14 GMT FROM: Samuele Ronchini at PSU Samuele Ronchini (PSU), James DeLaunay (PSU), Aaron Tohuvavohu (U Toronto), Gayathri Raman (PSU), Jamie A. Kennea (PSU), Tyler Parsotan (NASA GSFC) report: Swift/BAT did not localize GRB 240521B onboard (T0: 2024-05-21T15:08:57.06 UTC, Fermi trigger 737996942). The Fermi notice, distributed in near real-time, triggered the Swift Mission Operations Center operated Gamma-ray Urgent Archiver for Novel Opportunities (GUANO; Tohuvavohu et al. 2020, ApJ, 900, 1). Upon trigger by this notice, GUANO sent a command to the Swift Burst Alert Telescope (BAT) to save 200 seconds of BAT event-mode data from [-50,+150] seconds around the time of the burst. All the requested event mode data was delivered to the ground. The BAT likelihood search, NITRATES (DeLaunay + Tohuvavohu 2022, ApJ, 941, 169), detects the burst in a 16.384 s analysis time bin starting at T0 - 12.3 s with a sqrt(TS) of 74.6. An arcminute localization is found with DeltaLLHOut of 984.5 and a DeltaLLHPeak of 1282.7. See Section 9.1 and Figures 10 and 17 in the NITRATES paper for brief descriptions and interpretations of sqrt(TS), DeltaLLHPeak, and DeltaLLHOut. The BAT position is RA, Dec = 355.6879, -32.7215 deg which is RA(J2000) = 23h 42m 45.10s Dec(J2000) = -32° 43’ 17.4’’ with an estimated uncertainty of 3 arcmin radius. Follow-up observations from other instruments are requested. Swift ToO request has been submitted. GUANO is a fully autonomous, extremely low latency, spacecraft commanding pipeline designed for targeted recovery of BAT event mode data around the times of compelling astrophysical events to enable more sensitive GRB searches. A live reporting of Swift/BAT event data recovered by GUANO can be found at: https://www.swift.psu.edu/guano/
GCN 36535 table
GRB_name GRB240521B
GCN_number 36535
Detection_method Fermi GBM Det
t_trigger 15:08:57.060 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 36535 SUBJECT: GRB 240521B: Fermi GBM Observation DATE: 24/05/23 01:21:12 GMT FROM: Sarah Dalessi at UAH S. Dalessi (UAH), C. Fletcher (USRA), and C. Meegan (UAH) report on behalf of the Fermi Gamma-ray Burst Monitor Team: "At 15:08:57.06 UT on 21 May 2024, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 240521B (trigger 737996942/240521631). which was also detected by Swift/BAT-GUANO (Ronchini et al. 2024, GCN 36532). The Fermi GBM on-ground location is consistent with the Swift/BAT-GUANO position. The angle from the Fermi LAT boresight is 101 degrees. The GBM light curve single emission episode with a duration (T90) of about 34 s (50-300 keV). The time-averaged spectrum from T0-16 to T0+17 s is best fit by a simple power law function with index -1.64 +/- 0.04. The event fluence (10-1000 keV) in this time interval is (4 +/- 0.5)E-06 erg/cm^2. The 1-sec peak photon flux measured starting from T0-9.9 s in the 10-1000 keV band is 4.1 +/- 0.4 ph/s/cm^2. A power law function with an exponential high-energy cutoff fits the spectrum equally well. The power law index is -1.48 +/- 0.11 and the cutoff energy, parameterized as Epeak, is 222 +/- 94 keV. The spectral analysis results presented above are preliminary; final results will be published in the GBM GRB Catalog: https://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html For Fermi GBM data and info, please visit the official Fermi GBM Support Page: https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/"