GRB250118B

This page lists all entries on GRB250118B in GRBweb

Summary GCN 39017 GCN 39019

Summary table
Variable Value Source
T0 3:38:27 UTC GCN_circulars,IPN Triangulation
ra 108.0060° GCN_circulars,IPN Triangulation
decl -29.5570° GCN_circulars,IPN Triangulation
GBM_located False
mjd 60693.15170138889 GCN_circulars,IPN Triangulation
GCN 39017 table
GRB_name GRB250118B
GCN_number 39017
Detection_method IPN Triangulation
t_trigger 3:38:27 UTC
ra 108.0060°
decl -29.5570°
Circular_text TITLE: GCN CIRCULAR NUMBER: 39017 SUBJECT: IPN triangulation of GRB 250118B DATE: 25/01/23 15:24:56 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, E. Burns on behalf of the IPN, 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 250118B was detected by Konus-Wind, INTEGRAL (SPI-ACS), Swift (BAT), and Mars-Odyssey (HEND) at about 13107 s UT (03:38:27). 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: 108.006 (07h 12m 01s) -29.557 (-29d 33' 25") Corners: 114.190 (07h 36m 46s) -29.989 (-29d 59' 21") 112.319 (07h 29m 17s) -30.334 (-30d 20' 03") 101.717 (06h 46m 52s) -28.434 (-28d 26' 02") 103.724 (06h 54m 54s) -28.453 (-28d 27' 11") --------------------------------------------- The error box area is 4.5 sq. deg, and its maximum dimension is 11.0 deg (the minimum one is 28.7 arcmin). The Sun distance was 128 deg. This localization may be improved. A triangulation map and HEALPix FITS file are posted at http://www.ioffe.ru/LEA/GRBs/GRB250118_T13107/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 39019 table
GRB_name GRB250118B
GCN_number 39019
Detection_method Konus-Wind Det
t_trigger 3:38:27.725 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 39019 SUBJECT: Konus-Wind detection of GRB 250118B DATE: 25/01/23 20:34:26 GMT FROM: Anna Ridnaia at Ioffe Institute A. Ridnaia, D. Frederiks, A. Lysenko, D. Svinkin, A. Tsvetkova, M. Ulanov, and T. Cline, on behalf of the Konus-Wind team, report: The long-duration GRB 250118B (IPN triangulation: Kozyrev et al., GCN 39017) triggered Konus-Wind at T0=13107.725 s UT (03:38:27.725). The burst light curve shows a multipeaked structure, which starts at ~T0-5.8 s and has a total duration of ~9.4 s. We note a weaker and softer pulse seen in the same KW detector before the main pulse, from ~T0-58.8 s to ~T0-55.9 s. Since this pulse was detected by KW only, its relation to GRB 250118B cannot be currently confirmed. The emission is seen up to ~2 MeV. The Konus-Wind light curve of this GRB is available at http://www.ioffe.ru/LEA/GRBs/GRB250118_T13107/ As observed by Konus-Wind, the burst had a fluence of 3.49(-0.35,+1.30)x10^-6 erg/cm^2 and a 64-ms peak flux, measured from T0-0.244 s, of 2.97(-0.60,+1.22)x10^-6 erg/cm^2/s (both in the 20 keV - 10 MeV energy range). Since a major part of the burst emission was detected before the trigger time, the spectral analysis was performed using the KW 3-channel light curve data. Modelling the KW 3-channel time-integrated spectrum (measured from T0-5.837 s to T0+3.552 s) by a power law with exponential cutoff (CPL) model: dN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep), yields alpha = -1.55(-0.14,+0.18) and Ep = 287(-95,+256) keV. All the quoted errors are estimated at the 68% confidence level. All the presented results are preliminary.