GRB250118A

This page lists all entries on GRB250118A in GRBweb

Summary Fermi GBM GCN 38976 GCN 39004 GCN 39033

Summary table
Variable Value Source
GRB_name_Fermi GRB250118772
T0 18:31:11 UTC GCN_circulars,Fermi GBM final loc
ra 263.8200° Fermi_GBM
decl 38.8200° Fermi_GBM
pos_error 9.83e+00° Fermi_GBM
T90 0.272 s Fermi_GBM
T90_error 0.633 s Fermi_GBM
T90_start 18:31:11.807 UTC Fermi_GBM
fluence 1.32e-07 erg/cm² Fermi_GBM
fluence_error 9.16e-09 erg/cm² Fermi_GBM
T100 1.079 s
GBM_located True
mjd 60693.77165509259 GCN_circulars,Fermi GBM final loc
Fermi GBM table
GRB_name_Fermi GRB250118772
trigger_name bn250118772
ra 263.8200°
decl 38.8200°
pos_error 9.83e+00°
datum 2025-01-18
t_trigger 18:31:11.967 UTC
T90 0.272 s
T90_error 0.633 s
T90_start 18:31:11.807 UTC
fluence 1.32e-07 erg/cm²
fluence_error 9.16e-09 erg/cm²
flux_1024 1.17e+00 erg/cm²/s
flux_1024_error 2.05e-01 erg/cm²/s
flux_1024_time -7.04e-01 erg/cm²/s
flux_64 7.42e+00 erg/cm²/s
flux_64_error 9.31e-01 erg/cm²/s
GCN 38976 table
GRB_name GRB250118A
GCN_number 38976
Detection_method Fermi GBM final loc
t_trigger 18:31:11 UTC
ra 263.8000°
decl 38.8000°
Circular_text TITLE: GCN CIRCULAR NUMBER: 38976 SUBJECT: GRB 250118A: Fermi GBM Final Real-time Localization DATE: 25/01/18 18:41:33 GMT FROM: Fermi GBM Team at MSFC/Fermi-GBM The Fermi GBM team reports the detection of a likely SHORT GRB At 18:31:11 UT on 18 Jan 2025, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 250118A (trigger 758917876.966464 / 250118772). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 263.8, Dec = 38.8 (J2000 degrees, equivalent to J2000 17h 35m, 38d 47'), with a statistical uncertainty of 10.7 degrees. The angle from the Fermi LAT boresight is 14.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn250118772/quicklook/glg_skymap_all_bn250118772.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/bn250118772/quicklook/glg_healpix_all_bn250118772.fit The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2025/bn250118772/quicklook/glg_lc_medres34_bn250118772.gif
GCN 39004 table
GRB_name GRB250118A
GCN_number 39004
Detection_method Swift Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 39004 SUBJECT: GRB 250118A: Swift/BAT-GUANO localization skymap of a short burst DATE: 25/01/21 01:41:02 GMT FROM: Samuele Ronchini at PSU Samuele Ronchini (PSU), James DeLaunay (PSU), Aaron Tohuvavohu (Caltech), Gayathri Raman (PSU), Jamie A. Kennea (PSU), Tyler Parsotan (NASA GSFC) report: Swift/BAT did not localize GRB 250118A onboard (T0: 2025-11-18T18:31:11.97 UTC, Fermi GCN 38976) 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 13.4 in a 0.128 s analysis time bin, starting at T0 - 0.064 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 7,422 deg2 and the 50% credible area is 1,652 deg2. The integrated probability inside the coded field of view is <1%. The NITRATES skymap is consistent with the Fermi localization reported in GCN 38976. The joint NITRATES+Fermi 90% credible area is 565 deg2 and the 50% credible area is 111 deg2 A plot of the probability skymap can be viewed here: [skymap_plot](https://guano.swift.psu.edu/trigger_report?id=758917906/#:~:text=Probability%20Skymap) The probability skymap file can be downloaded from the link here [skymap_fits_file](https://guano.swift.psu.edu/files/758917906/0_n_PROBMAP) 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=758917906 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 39033 table
GRB_name GRB250118A
GCN_number 39033
Detection_method Fermi GBM Det
t_trigger 18:31:11.970 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 39033 SUBJECT: GRB 250118A: Fermi GBM Observation DATE: 25/01/25 20:29:13 GMT FROM: Peter Veres at University of Alabama in Huntsville P. Veres (UAH) and C. Meegan (UAH) report on behalf of the Fermi Gamma-ray Burst Monitor Team: "At 18:31:11.97 UT on 18 January 2025, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 250118A (trigger 758917876/250118772). which was also detected by Swift-BAT/GUANO (Ronchini et al. 2025, GCN 39004). The Fermi GBM on-ground location is consistent with the Swift position. The angle from the Fermi LAT boresight is 14 degrees. The GBM light curve consists of a single emission episode with a duration (T90) of about 0.3 s (50-300 keV). The time-averaged spectrum from T0-0.13 to T0+0.06 s is best fit by a simple power law function with index -1.18 +/- 0.06. The event fluence (10-1000 keV) in this time interval is (4.1 +/- 0.4)E-07 erg/cm^2. The 64-ms peak photon flux measured starting from T0-0.064 s in the 10-1000 keV band is 7.4 +/- 0.9 ph/s/cm^2. A power law function with an exponential high-energy cutoff gives an acceptable fit to the spectrum. The power law index is -0.73 +/- 0.22 and the cutoff energy, parameterized as Epeak, is 1100 +/- 500 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/"