GRB210925B

This page lists all entries on GRB210925B in GRBweb

Summary Fermi GBM IPN GCN 30890 GCN 30892

Summary table
Variable Value Source
GRB_name_Fermi GRB210925056
T0 1:20:08.550 UTC Fermi_GBM
ra 48.8167° IPN
decl -52.8667° IPN
pos_error 2.30e+00° IPN
T90 4.544 s Fermi_GBM
T90_error 0.529 s Fermi_GBM
T90_start 1:20:08.550 UTC Fermi_GBM
fluence 5.79e-06 erg/cm² Fermi_GBM
fluence_error 3.12e-08 erg/cm² Fermi_GBM
T100 4.544 s
GBM_located False
mjd 59482.05565451389 Fermi_GBM
Fermi GBM table
GRB_name_Fermi GRB210925056
trigger_name bn210925056
ra 47.9900°
decl -51.4100°
pos_error 2.61e+00°
datum 2021-09-25
t_trigger 1:20:08.678 UTC
T90 4.544 s
T90_error 0.529 s
T90_start 1:20:08.550 UTC
fluence 5.79e-06 erg/cm²
fluence_error 3.12e-08 erg/cm²
flux_1024 1.79e+01 erg/cm²/s
flux_1024_error 4.29e-01 erg/cm²/s
flux_1024_time 1.09e+00 erg/cm²/s
flux_64 2.28e+01 erg/cm²/s
flux_64_error 1.85e+00 erg/cm²/s
IPN table
GRB_name GRB210925B
ra 48.8167°
decl -52.8667°
pos_error 2.30e+00°
GCN 30890 table
GRB_name GRB210925B
GCN_number 30890
Detection_method IPN Triangulation
t_trigger 1:20:09 UTC
ra 48.8170°
decl -52.8630°
Circular_text TITLE: GCN CIRCULAR NUMBER: 30890 SUBJECT: IPN triangulation of GRB 210925B DATE: 21/09/27 18:08:46 GMT FROM: Anna Ridnaia at Ioffe Institute K. Hurley, on behalf of the IPN, I. G. Mitrofanov, D. V. Golovin, A. S. Kozyrev, M. L. Litvak, and A. B. Sanin, on behalf of the HEND-Odyssey GRB team, A. Ridnaia, S. Golenetskii, D. Frederiks, D. Svinkin, A. Lysenko, and T. Cline on behalf of the Konus-Wind team, A. Goldstein, M. S. Briggs, and C. Wilson-Hodge on behalf of the Fermi-GBM team, A. von Kienlin, X. Zhang, A. Rau, V. Savchenko, 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, and R. Starr, on behalf of the GRS-Odyssey GRB team, report: The long-duration GRB 210925B was detected by Fermi (GBM trigger 654225613), Konus-Wind, Mars-Odyssey (HEND), INTEGRAL (SPI-ACS), and Swift-BAT at about 4809 s UT (01:20:09). 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: 48.817 (03h 15m 16s) -52.863 (-52d 51' 45") Corners: 47.551 (03h 10m 12s) -53.723 (-53d 43' 21") 50.006 (03h 20m 01s) -52.058 (-52d 03' 29") 50.027 (03h 20m 06s) -51.978 (-51d 58' 41") 47.579 (03h 10m 19s) -53.644 (-53d 38' 39") --------------------------------------------- The error box area is 335 sq. arcmin, and its maximum dimension is 2.3 deg (the minimum one is 2.5 arcmin). The Sun distance was 113 deg. This box may be improved. A triangulation map is posted at http://www.ioffe.ru/LEA/GRBs/GRB210925_T04810/IPN/ The time history and spectrum will be given in forthcoming GCN Circulars.
GCN 30892 table
GRB_name GRB210925B
GCN_number 30892
Detection_method AstroSat CZTI
Circular_text TITLE: GCN CIRCULAR NUMBER: 30892 SUBJECT: GRB 210925B: AstroSat CZTI detection DATE: 21/09/28 13:24:23 GMT FROM: Gaurav Waratkar at IIT,Bombay V. Prasad (IUCAA), P. Sawant (IUCAA), G. Waratkar (IITB), A. Vibhute (IUCAA), V. Bhalerao (IITB), D. Bhattacharya (IUCAA), A. R. Rao (IUCAA/TIFR), and S. Vadawale (PRL) report on behalf of the AstroSat CZTI collaboration: Analysis of AstroSat CZTI data with the CIFT framework (Sharma et al., 2021, JApA, 42, 73) showed detection of a long GRB 210925B for which the IPN triangulation (Hurley et al., GCN 30890) was reported. The source was clearly detected in the 20-200 keV energy range. The light curve showed multiple peaks of emission with the strongest peak at 2021-09-25 01:20:09.75 UT. The measured peak count rate associated with the burst is 887 (+190, -97) cts/s above the background in the combined data of four quadrants, with a total of 1482 (+214, -230) cts. The local mean background count rate was 471 (+5, -9) cts/s. Using cumulative rates, we measure a T90 of 6.3 (+1.9, -2.0) s. It was also clearly detected in the CsI anticoincidence (Veto) detector in the 100-500 keV energy range. CZTI GRB detections are reported regularly on the payload site at http://astrosat.iucaa.in/czti/?q=grb. CZTI is built by a TIFR-led consortium of institutes across India, including VSSC, ISAC, IUCAA, SAC, and PRL. The Indian Space Research Organisation funded, managed, and facilitated the project.