GRB250201A

This page lists all entries on GRB250201A in GRBweb

Summary Fermi GBM GCN 39113 GCN 39117 GCN 39151 GCN 39152

Summary table
Variable Value Source
GRB_name_Fermi GRB250201417
T0 9:59:46.667 UTC Fermi_GBM
ra 115.2870° GCN_circulars,IPN Triangulation
decl -54.2930° GCN_circulars,IPN Triangulation
T90 16.384 s Fermi_GBM
T90_error 0.362 s Fermi_GBM
T90_start 9:59:47.755 UTC Fermi_GBM
fluence 1.27e-05 erg/cm² Fermi_GBM
fluence_error 3.32e-08 erg/cm² Fermi_GBM
T100 17.472 s
GBM_located False
mjd 60707.41651234954 Fermi_GBM
Fermi GBM table
GRB_name_Fermi GRB250201417
trigger_name bn250201417
ra 115.8100°
decl -52.5700°
pos_error 2.60e+00°
datum 2025-02-01
t_trigger 9:59:46.667 UTC
T90 16.384 s
T90_error 0.362 s
T90_start 9:59:47.755 UTC
fluence 1.27e-05 erg/cm²
fluence_error 3.32e-08 erg/cm²
flux_1024 1.54e+01 erg/cm²/s
flux_1024_error 3.32e-01 erg/cm²/s
flux_1024_time 1.34e+01 erg/cm²/s
flux_64 1.90e+01 erg/cm²/s
flux_64_error 1.48e+00 erg/cm²/s
GCN 39113 table
GRB_name GRB250201A
GCN_number 39113
Detection_method Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 39113 SUBJECT: GRB 250201A: BALROG localization (Fermi Trigger 760096791 / GRB 250201417) DATE: 25/02/01 10:53:32 GMT FROM: Jochen Greiner at MPE T. Preis (University of Innsbruck) & J. Greiner (MPE Garching) report: The public trigdat data of the Fermi Gamma-ray Burst Monitor (GBM) trigger 760096791 at 09:59:46 on 01 Feb. 2025 were automatically fitted for spectrum and sky location with BALROG (Burgess et al. 2018, MNRAS 476, 1427; Berlato et al. 2019, ApJ 873, 60). The best-fit position is: RA(2000.0) = 112.5 deg Decl.(2000.0) = -54.7 deg The 1 sigma statistical error radius is 2.0 deg. We estimate an additional systematic error of 1 deg. Further details are available at: https://grb.mpe.mpg.de/grb/GRB250201417/ The Healpix map can be downloaded from: https://grb.mpe.mpg.de/grb/GRB250201417/healpix The location parameters are available as JSON at: https://grb.mpe.mpg.de/grb/GRB250201417/json
GCN 39117 table
GRB_name GRB250201A
GCN_number 39117
Detection_method INTEGRAL
Circular_text TITLE: GCN CIRCULAR NUMBER: 39117 SUBJECT: GRB 250201A: INTEGRAL SPI/ACS detection DATE: 25/02/01 19:34:25 GMT FROM: Aishwarya L Thakur at INAF-IAPS, Rome Patrizia Barria(a,b), Giulia Gianfagna(a), James Craig Rodi(a), Aishwarya Linesh Thakur(a), Lorenzo Natalucci(a,b), Luigi Piro(a) report: GRB 250201A was discovered by Fermi/GBM (GCN 39112) on 2025-02-01T09:59:46 (UTC). We searched for a corresponding counterpart in the INTEGRAL/SPI-ACS data. In an SPI-ACS light curve above 80 keV, we find a signal temporally coincident with the GBM detection, having an approximate duration of ~ 20 sec. The signal consists of two pulses over this duration. The approximate peak count rate in SPI-ACS is 77,500 cts/s for E>80 keV, over a median background rate of 62,800 cts/s. This work is based on observations with INTEGRAL, an ESA project with instruments and a science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland, and Spain), and with the participation of Russia and the USA. The SPI-ACS detector system has been provided by MPE Garching/Germany. ----- (a) INAF/IAPS-Rome (b) ICSC National Research Centre for High-Performance Computing
GCN 39151 table
GRB_name GRB250201A
GCN_number 39151
Detection_method IPN Triangulation
t_trigger 9:59:47 UTC
ra 115.2870°
decl -54.2930°
Circular_text TITLE: GCN CIRCULAR NUMBER: 39151 SUBJECT: IPN triangulation of GRB 250201A DATE: 25/02/05 15:21:26 GMT FROM: Anna Ridnaia at Ioffe Institute A.S. Kozyrev, D.V. Golovin, M.L. Litvak, I.G. Mitrofanov, and A.B. Sanin on behalf of the HEND/Mars Odyssey team, A. Ridnaia, D. Frederiks, A. Lysenko, D. Svinkin, and T. Cline on behalf of the Konus-Wind team, A. Goldstein, M. S. Briggs, C. Wilson-Hodge, and E. Burns on behalf of the Fermi GBM team, E. Bozzo and C. Ferrigno, on behalf of the INTEGRAL SPI-ACS GRB team, S. Barthelmy, J. Cummings, H. Krimm, D. Palmer, and A. Tohuvavohu on behalf of the Swift-BAT team, and W. Boynton, C. Fellows, K. Harshman, H. Enos, R. Starr, and A.S. Gardner on on behalf of the GRS-Odyssey GRB team, report: The long-duration GRB 250201A (Fermi-GBM detection: Fermi GBM team, GCN 39112; BALROG localization: Preis & Greiner, GCN 39113; INTEGRAL SPI/ACS detection: Barria et al., GCN 39117) was detected by Fermi (GBM), Konus-Wind, INTEGRAL (SPI-ACS), Swift (BAT), and Mars-Odyssey (HEND) at about 35987 s UT (09:59:47). The burst was outside the coded field of view of the BAT. We have triangulated it to a preliminary, 3 sigma error box whose coordinates are: ------------------------------- RA(2000), deg Dec(2000), deg ------------------------------- Center: 115.287 -54.293 Corners: 137.464 -51.378 137.379 -51.074 93.570 -52.488 93.601 -52.814 ------------------------------- The error box area is 6.8 sq. deg, and its maximum dimension is 26.3 deg (the minimum one is 21 arcmin). The Sun distance was 101 deg. A triangulation map and HEALPix FITS file are posted at http://www.ioffe.ru/LEA/GRBs/GRB250201_T35989/IPN The HEALPix triangulation map is the multi-order HEALPix in units of probability density. The Konus-Wind time history and spectrum will be given in a forthcoming GCN Circular.
GCN 39152 table
GRB_name GRB250201A
GCN_number 39152
Detection_method Konus-Wind Det
t_trigger 9:59:49.814 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 39152 SUBJECT: Konus-Wind detection of GRB 250201A DATE: 25/02/05 16:18:27 GMT FROM: Dmitry Frederiks at Ioffe Institute D. Frederiks, A.Lysenko, A. Ridnaia, D. Svinkin, A. Tsvetkova, M. Ulanov, and T. Cline, on behalf of the Konus-Wind team, report: The long GRB 250201A (Fermi-GBM detection: Fermi GBM team, GCN 39112; BALROG localization: Preis & Greiner, GCN 39113; INTEGRAL SPI/ACS detection: Barria et al., GCN 39117; IPN triangulation: Kozyrev et al., GCN 39151) triggered Konus-Wind (KW) at T0=35989.814 s UT (09:59:49.814). The burst light curve shows a double-peaked emission pulse with the total duration of ~21 s. The emission is seen up to ~8 MeV. The Konus-Wind light curve of this GRB is available at http://www.ioffe.ru/LEA/GRBs/GRB250201_T35989/ As observed by Konus-Wind, the burst had a fluence of (1.21 ± 0.08)x10^-5 erg/cm^2 and a 64-ms peak energy flux, measured from T0 + 12.160 s, of (2.97 ± 0.34)x10^-6 erg/cm^2/s (both in the 20 keV - 10 MeV energy range). The time-integrated spectrum (measured from T0 to T0+16.640 s) is best fit in the 20 keV - 15 MeV range by a GRB (Band) function with the following model parameters: the low-energy photon index alpha = -0.72 (-0.12,+0.13), the high energy photon index beta = -3.07 (-0.54,+0.27), the peak energy Ep = 134 (-7,+8) keV, chi2 = 118/97 dof. The spectrum near the peak count rate (measured from T0+8.448 s to T0+16.640 s) is best fit in the 20 keV - 15 MeV range by a GRB (Band) function with the following model parameters: the low-energy photon index alpha = -0.76 (-0.11,+0.13), the high energy photon index beta = -2.95 (-0.34,+0.23), the peak energy Ep = 138 (-8,+8) keV, chi2 = 94/78 dof. All the quoted errors are estimated at the 68% confidence level. All the presented results are preliminary.