GRB250619B

This page lists all entries on GRB250619B in GRBweb

Summary Fermi GBM GCN 40788 GCN 40795 GCN 40802

Summary table
Variable Value Source
GRB_name_Fermi GRB250619984
T0 23:36:16.144 UTC Fermi_GBM
ra 25.3700° Fermi_GBM
decl -24.7500° Fermi_GBM
pos_error 9.18e+00° Fermi_GBM
T90 28.928 s Fermi_GBM
T90_error 1.493 s Fermi_GBM
T90_start 23:36:16.144 UTC Fermi_GBM
fluence 1.49e-06 erg/cm² Fermi_GBM
fluence_error 2.85e-08 erg/cm² Fermi_GBM
T100 28.928 s
GBM_located True
mjd 60845.98352018518 Fermi_GBM
Fermi GBM table
GRB_name_Fermi GRB250619984
trigger_name bn250619984
ra 25.3700°
decl -24.7500°
pos_error 9.18e+00°
datum 2025-06-19
t_trigger 23:36:17.168 UTC
T90 28.928 s
T90_error 1.493 s
T90_start 23:36:16.144 UTC
fluence 1.49e-06 erg/cm²
fluence_error 2.85e-08 erg/cm²
flux_1024 2.22e+00 erg/cm²/s
flux_1024_error 2.25e-01 erg/cm²/s
flux_1024_time -3.20e-01 erg/cm²/s
flux_64 5.25e+00 erg/cm²/s
flux_64_error 1.22e+00 erg/cm²/s
GCN 40788 table
GRB_name GRB250619B
GCN_number 40788
Detection_method Fermi GBM final loc
t_trigger 23:36:17 UTC
ra 25.4000°
decl -24.8000°
Circular_text TITLE: GCN CIRCULAR NUMBER: 40788 SUBJECT: GRB 250619B: Fermi GBM Final Real-time Localization DATE: 25/06/19 23:46:58 GMT FROM: Fermi GBM Team at MSFC/Fermi-GBM The Fermi GBM team reports the detection of a likely LONG GRB At 23:36:17 UT on 19 Jun 2025, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 250619B (trigger 772068982.168064 / 250619984). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 25.4, Dec = -24.8 (J2000 degrees, equivalent to J2000 01h 41m, -24d 48'), with a statistical uncertainty of 13.4 degrees. The angle from the Fermi LAT boresight is 48.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn250619984/quicklook/glg_skymap_all_bn250619984.png The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn250619984/quicklook/glg_healpix_all_bn250619984.fit The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn250619984/quicklook/glg_lc_medres34_bn250619984.gif
GCN 40795 table
GRB_name GRB250619B
GCN_number 40795
Detection_method Swift Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 40795 SUBJECT: GRB 250619B: Swift/BAT-GUANO localization skymap of a burst DATE: 25/06/20 17:11:42 GMT FROM: Jimmy DeLaunay at Penn State James DeLaunay (PSU), Samuele Ronchini (PSU), Aaron Tohuvavohu (Caltech), Jamie A. Kennea (PSU), Tyler Parsotan (NASA GSFC), Maia Williams (PSU) report: Swift/BAT did not localize GRB 250619B onboard (T0: 2025-06-19T23:36:17.17 UTC, Fermi/GBM trig 772068982) 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), performed on the temporal window [T0-20 s, T0+20 s], detects the burst with a sqrt(TS) of 7.9 in a 8.192 s analysis time bin, starting at T0 - 2.048 s. Using the NITRATES analysis, parameter estimation was performed to obtain the localization of this burst in the form of a HEALPIX Multi-Order Coverage (MOC) skymap. This localization accounts for both statistical and systematic errors. More details in the creation and calibration of these maps will soon be published (DeLaunay et al. 2025. in prep) The 90% credible area is 10,760 deg2 and the 50% credible area is 1,197 deg2. The integrated probability inside the coded field of view is 30%. The NITRATES skymap is consistent with the Fermi localization reported in the final position notice (GCN 40788). The combined Fermi/GBM+NITRATES 90% credible area is 652 deg2 and the 50% credible area is 146 deg2. A plot of the probability skymap can be viewed here: [skymap_plot](https://guano.swift.psu.edu/trigger_report?id=772069012/#:~:text=Probability%20Skymap) The probability skymap and joint skymap files can be downloaded from the links here [skymap_fits_file](https://guano.swift.psu.edu/files/772069012/0_n_PROBMAP) [joint_skymap_fits_file](https://guano.swift.psu.edu/files/772069012/0_n_JOINTMAP) Instructions on how to read and manipulate this map can be found here: https://guano.swift.psu.edu/documentation More details about this burst can be found on the trigger report page here: https://guano.swift.psu.edu/trigger_report?id=772069012 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 40802 table
GRB_name GRB250619B
GCN_number 40802
Detection_method Fermi GBM Det
t_trigger 23:36:17.170 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 40802 SUBJECT: GRB 250619B: Fermi GBM Observation DATE: 25/06/21 01:38:07 GMT FROM: Jacob Smith at Fermi-GBM Team Jacob Smith (UAH) and C. Meegan (UAH) report on behalf of the Fermi Gamma-ray Burst Monitor Team: At 23:36:17.17 UT on 19 June 2025, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 250619B (trigger 772068982/250619984). which was also detected by Swift/BAT-GUANO (J. DeLaunay et al. 2025, GCN 40795). The Fermi GBM on-ground location is consistent with the Swift/BAT-GUANO position. The angle from the Fermi LAT boresight is 48 degrees. The GBM light curve consists of a double emission episode with a duration (T90) of about 29 s (50-300 keV). The time-averaged spectrum from T0-1 to T0+28.7 s is best fit by a power law function with an exponential high-energy cutoff. The power law index is -1.1 +/- 0.2 and the cutoff energy, parameterized as Epeak, is 67 +/- 9 keV. A Band function fits the spectrum equally well with Epeak = 57 +/- 13 keV, alpha = -1 +/- 0.4 and beta = -2.5 +/- 0.4. The event fluence (10-1000 keV) in this time interval is (1.4 +/- 0.1)E-06 erg/cm^2. The 1-sec peak photon flux measured starting from T0-0.32 s in the 10-1000 keV band is 2.2 +/- 0.2 ph/s/cm^2. 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/