GRB230803A

This page lists all entries on GRB230803A in GRBweb

Summary Fermi GBM IPN GCN 34325 GCN 34328 GCN 34330 GCN 34358

Summary table
Variable Value Source
GRB_name_Fermi GRB230803061
T0 1:27:08 UTC GCN_circulars,Fermi GBM final loc
ra 150.5083° IPN
decl -64.9833° IPN
pos_error 2.80e+00° IPN
T90 87.554 s Fermi_GBM
T90_error 27.141 s Fermi_GBM
T90_start 1:27:39.963 UTC Fermi_GBM
fluence 6.83e-05 erg/cm² Fermi_GBM
fluence_error 2.70e-08 erg/cm² Fermi_GBM
T100 119.517 s
GBM_located False
mjd 60159.06050925926 GCN_circulars,Fermi GBM final loc
Fermi GBM table
GRB_name_Fermi GRB230803061
trigger_name bn230803061
ra 158.4100°
decl -64.3800°
pos_error 3.39e+00°
datum 2023-08-03
t_trigger 1:27:08.154 UTC
T90 87.554 s
T90_error 27.141 s
T90_start 1:27:39.963 UTC
fluence 6.83e-05 erg/cm²
fluence_error 2.70e-08 erg/cm²
flux_1024 4.33e+01 erg/cm²/s
flux_1024_error 4.22e-01 erg/cm²/s
flux_1024_time 9.43e+01 erg/cm²/s
flux_64 5.24e+01 erg/cm²/s
flux_64_error 1.76e+00 erg/cm²/s
IPN table
GRB_name GRB230803A
ra 150.5083°
decl -64.9833°
pos_error 2.80e+00°
GCN 34325 table
GRB_name GRB230803A
GCN_number 34325
Detection_method Fermi GBM final loc
t_trigger 1:27:08 UTC
ra 158.4000°
decl -64.4000°
Circular_text TITLE: GCN CIRCULAR NUMBER: 34325 SUBJECT: GRB 230803A: Fermi GBM Final Real-time Localization DATE: 23/08/03 01:37:47 GMT FROM: Fermi GBM Team at MSFC/Fermi-GBM The Fermi GBM team reports the detection of a likely LONG GRB At 01:27:08 UT on 3 Aug 2023, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 230803A (trigger 712718833.154354 / 230803061). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 158.4, Dec = -64.4 (J2000 degrees, equivalent to J2000 10h 33m, -64d 24'), with a statistical uncertainty of 3.3 degrees. The angle from the Fermi LAT boresight is 66.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2023/bn230803061/quicklook/glg_skymap_all_bn230803061.png The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2023/bn230803061/quicklook/glg_healpix_all_bn230803061.fit The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2023/bn230803061/quicklook/glg_lc_medres34_bn230803061.gif
GCN 34328 table
GRB_name GRB230803A
GCN_number 34328
Detection_method AstroSat CZTI
Circular_text TITLE: GCN CIRCULAR NUMBER: 34328 SUBJECT: GRB 230803A: AstroSat CZTI detection DATE: 23/08/03 12:04:58 GMT FROM: Gaurav Waratkar at IIT Bombay P. K. Navaneeth (IUCAA), G. Waratkar (IITB), A. Vibhute (IUCAA), V. Bhalerao (IITB), D. Bhattacharya (Ashoka University/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 ML pipeline (Abraham et al., 2021, MNRAS, 504, 3084) and the CIFT framework (Sharma et al., 2021, JApA, 42, 73) showed the detection of a bright long GRB 230803A which was also detected by Fermi (Fermi GBM Team, GCN Circ. 34325). 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 2023-08-03 01:28:42.50 UTC. The measured peak count rate associated with the burst is 783 (+56, -59) counts/s above the background in the combined data of all quadrants, with a total of 5492 (+498, -481) counts. The local mean background count rate was 430 (+3, -3) counts/s. Using cumulative rates, we measure a T90 of 25 (+2, -1) s. In the preliminary analysis, we find 371 Compton events associated with this event. The source was also clearly detected in the CsI anticoincidence (Veto) detector in the 100-500 keV energy range. The light curve showed multiple peaks of emission with the strongest peak at 2023-08-03 01:28:42.63 UTC. The measured peak count rate associated with the burst is 2196 (+97, -102) counts/s above the background in the combined data of all quadrants, with a total of 15329 (+934, -934) counts. The local mean background count rate was 1365 (+7, -5) counts/s. We measure a T90 of 26 (+2, -1) s from the cumulative Veto light curve. CZTI is built by a TIFR-led consortium of institutes across India, including VSSC, URSC, IUCAA, SAC, and PRL. The Indian Space Research Organisation funded, managed, and facilitated the project. CZTI GRB detections are reported regularly on the payload site at: http://astrosat.iucaa.in/czti/?q=grb
GCN 34330 table
GRB_name GRB230803A
GCN_number 34330
Detection_method IPN Triangulation
t_trigger 1:27:08 UTC
ra 150.5100°
decl -64.9870°
Circular_text TITLE: GCN CIRCULAR NUMBER: 34330 SUBJECT: IPN triangulation of GRB 230803A DATE: 23/08/03 20:39:17 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, D. Svinkin, A. Lysenko, 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, 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 230803A (Fermi GBM detection: Fermi GBM team, GCN 34325; AstroSat CZTI detection: Navaneeth et al., GCN 34328) has been detected by Fermi (GBM), Konus-Wind, INTEGRAL (SPI-ACS), AstroSat (CZTI), and Mars-Odyssey (HEND), so far, at about 5228 s UT (01:27:08). We have triangulated it to a preliminary, 3 sigma error box whose coordinates are: --------------------------------------------- RA(2000), deg Dec(2000), deg --------------------------------------------- Center: 150.510 (10h 02m 02s) -64.987 (-64d 59' 12") Corners: 147.455 (09h 49m 49s) -64.554 (-64d 33' 15") 147.329 (09h 49m 19s) -64.581 (-64d 34' 51") 153.688 (10h 14m 45s) -65.347 (-65d 20' 50") 153.812 (10h 15m 15s) -65.315 (-65d 18' 54") --------------------------------------------- The error box area is 431 sq. arcmin, and its maximum dimension is 2.8 deg (the minimum one is 3 arcmin). The Sun distance was 83 deg. The IPN localization is consistent with, but reduces the area of, the Fermi-GBM final localization (GCN 34325). This localization may be improved. A triangulation map and HEALPix FITS file are posted at http://www.ioffe.ru/LEA/GRBs/GRB230803_T05229/IPN/ The Konus-Wind time history and spectrum will be given in a forthcoming GCN Circular.
GCN 34358 table
GRB_name GRB230803A
GCN_number 34358
Detection_method Konus-Wind Det
t_trigger 1:27:09.064 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 34358 SUBJECT: Konus-Wind detection of GRB 230803A DATE: 23/08/07 15:47:20 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 230803A (Fermi GBM detection: Fermi GBM team, GCN 34325; AstroSat CZTI detection: Navaneeth et al., GCN 34328; IPN triangulation: Kozyrev et al., GCN 34330) triggered Konus-Wind (KW) at T0=5229.064 s UT (01:27:09.064). The burst light curve shows a multi-peaked structure with a total duration of ~126 s. 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/GRB230803_T05229/ As observed by Konus-Wind, the burst had a fluence of (7.59 ± 0.88)x10^-5 erg/cm^2 and a 64-ms peak energy flux, measured from T0 + 93.760 s, of (1.43 ± 0.13)x10^-5 erg/cm^2/s (both in the 20 keV - 10 MeV energy range). The time-integrated spectrum (measured from T0+57.600 to T0+128.256 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 = -1.30 (-0.06,+0.08), the high energy photon index beta = -2.65 (-0.82,+0.30), the peak energy Ep = 256 (-31,+32) keV, chi2 = 112/97 dof. The spectrum near the peak count rate (measured from T0+90.368 to T0+95.488 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 = -0.93 (-0.06,+0.07), the high energy photon index beta = -2.32 (-0.20,+0.14), the peak energy Ep = 284 (-38,+40) keV, chi2 = 66/77 dof. All the quoted errors are estimated at the 90% confidence level. All the presented results are preliminary.