GRB200920B

This page lists all entries on GRB200920B in GRBweb

Summary Fermi GBM GCN 28464 GCN 28467 GCN 28514

Summary table
Variable Value Source
GRB_name_Fermi GRB200920831
T0 19:56:54.617 UTC GCN_circulars,Konus-Wind Det
ra 160.5209° GCN_circulars,IPN Triangulation
decl 13.4321° GCN_circulars,IPN Triangulation
T90 0.384 s Fermi_GBM
T90_error 0.968 s Fermi_GBM
T90_start 19:56:59.506 UTC Fermi_GBM
fluence 1.40e-06 erg/cm² Fermi_GBM
fluence_error 2.80e-08 erg/cm² Fermi_GBM
T100 5.273 s
GBM_located False
mjd 59112.83118769676 GCN_circulars,Konus-Wind Det
Fermi GBM table
GRB_name_Fermi GRB200920831
trigger_name bn200920831
ra 158.0100°
decl 7.1200°
pos_error 6.25e+00°
datum 2020-09-20
t_trigger 19:56:59.570 UTC
T90 0.384 s
T90_error 0.968 s
T90_start 19:56:59.506 UTC
fluence 1.40e-06 erg/cm²
fluence_error 2.80e-08 erg/cm²
flux_1024 4.18e+00 erg/cm²/s
flux_1024_error 2.18e-01 erg/cm²/s
flux_1024_time -1.92e-01 erg/cm²/s
flux_64 1.20e+01 erg/cm²/s
flux_64_error 1.03e+00 erg/cm²/s
GCN 28464 table
GRB_name GRB200920B
GCN_number 28464
Detection_method Fermi GBM Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 28464 SUBJECT: GRB 200920B: AGILE/MCAL detection of a burst DATE: 20/09/21 08:35:02 GMT FROM: Alessandro Ursi at INAF/IAPS A. Ursi (INAF/IAPS), F. Verrecchia (SSDC, and INAF/OAR), M. Tavani (INAF/IAPS, and Univ. Roma Tor Vergata), A. Argan, M. Cardillo, C. Casentini, Y. Evangelista, G. Piano (INAF/IAPS), F. Lucarelli, C. Pittori (SSDC, and INAF/OAR), A. Bulgarelli, V. Fioretti, F. Fuschino, N. Parmiggiani (INAF/OAS-Bologna), M. Marisaldi (INAF/OAS-Bologna, and Bergen University), M. Pilia, A. Trois (INAF/OA-Cagliari), I. Donnarumma (ASI), F. Longo (Univ. Trieste and INFN Trieste), A. Giuliani (INAF/IASF-Mi), report on behalf of the AGILE Team: The AGILE Mini-CALorimeter (MCAL) detected the short GRB 200920B at T0 = 2020-09-20 19:56:59.52 +/- 0.01 s (UTC), detected also by Fermi/GBM (trigger 622324624 / 200920651). The event lasted about 0.42 s and released a total number of ~505 counts in the detector (in the 0.4-100 MeV energy range), above an average background rate of 540 Hz. The time-integrated spectrum of the burst can be fitted in the energy range 0.4-5 MeV with a single power-law with ph.ind. = 2.41 -0.30/+0.37, resulting in a reduced chi-squared of 1.14 (36 d.o.f.) and a fluence of 3.46e-7 ergs/cm^2 (90% confidence level), in the same energy range. The MCAL light curve can be found at http://www.agilescienceapp.it/notices/GRB200920B_069656_527716619.529166.png . The event is also clearly visible in the AGILE scientific ratemeters of the SuperAGILE (SA; 18-60 keV), MCAL (0.4-100 MeV), and AntiCoincidence (50-200 keV) detectors. Their light curves can be found at: http://www.agilescienceapp.it/notices/GRB200920B_AGILE_RM.png . The AGILE-MCAL detector is a CsI detector with a 4 pi FoV, sensitive in the energy range 0.4-100 MeV. Additional analysis of AGILE data is in progress. Automatic MCAL GRB alert Notice
GCN 28467 table
GRB_name GRB200920B
GCN_number 28467
Detection_method IPN Triangulation
t_trigger 19:56:55 UTC
ra 160.5209°
decl 13.4321°
Circular_text TITLE: GCN CIRCULAR NUMBER: 28467 SUBJECT: IPN triangulation of GRB 200920B (short) DATE: 20/09/21 20:34:34 GMT FROM: Anna Ridnaia at Ioffe Institute A. Ridnaia, S. Golenetskii, R. Aptekar, D. Frederiks, D. Svinkin, and T. Cline on behalf of the Konus-Wind team, K. Hurley, on behalf of the IPN, 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, and A. Ursi, F. Verrecchia, M. Tavani, N. Parmiggiani, C. Pittori, A. Bulgarelli, on behalf of the AGILE team, report: The short-duration GRB 200920B (AGILE/MCAL detection: Ursi et al., GCN Circ. 28464) has been detected by Fermi (GBM trigger 622324624), Konus-Wind, INTEGRAL (SPI-ACS), and AGILE (MCAL), so far, at about 71815 s UT (19:56:55). We have triangulated it to a Konus-GBM annulus centered at RA(2000)=157.135 deg (10h 28m 32s) Dec(2000)=+10.976 deg (+10d 58' 33"), whose radius is 4.834 +/- 1.787 deg (3 sigma), to a Konus-INTEGRAL annulus centered at RA(2000)=154.111 deg (10h 16m 27s) Dec(2000)=+8.715 deg (+8d 42' 54"), whose radius is 7.120 +/- 1.815 deg (3 sigma), and to a GBM-INTEGRAL annulus centered at RA(2000)=77.242 deg (05h 08m 58s) Dec(2000)=-35.743 deg (-35d 44' 36"), whose radius is 90.000 +/- 4.602 deg (3 sigma). The preliminary, 3 sigma error box is: --------------------------------------------- RA(2000), deg Dec(2000), deg --------------------------------------------- Center: 160.5209 +13.4321 Corners: 161.4146 +14.0653 155.8758 +17.4839 150.6190 +12.7611 155.8316 +13.7440 159.6319 +12.7958 159.4728 +8.9807 157.1525 +4.3546 163.1097 +7.9563 --------------------------------------------- The error box area is 51.5 sq. deg, and its maximum dimension is 13.2 deg (the minimum one is 2.1 deg). The Sun distance was 123 deg. This box may be improved. A triangulation map is posted at http://www.ioffe.ru/LEA/GRBs/GRB200920_T71814/IPN/ The Konus-Wind time history and spectrum will be given in a forthcoming GCN Circular.
GCN 28514 table
GRB_name GRB200920B
GCN_number 28514
Detection_method Konus-Wind Det
t_trigger 19:56:54.617 UTC
Circular_text TITLE: GCN CIRCULAR NUMBER: 28514 SUBJECT: Konus-Wind detection of GRB 200920B DATE: 20/09/27 19:50:30 GMT FROM: Anna Ridnaia at Ioffe Institute A. Ridnaia, S. Golenetskii, R. Aptekar, D. Frederiks, M. Ulanov, D. Svinkin, A. Tsvetkova, A. Lysenko, and T. Cline on behalf of the Konus-Wind team, report: The short-duration GRB 200920B (AGILE/MCAL detection: Ursi et al., GCN Circ. 28464; IPN triangulation: Ridnaia et al., GCN Circ. 28467) triggered Konus-Wind at T0=71814.617 s UT (19:56:54.617). The burst light curve shows a multi-peaked structure which started at ~T0-0.368 s and had a total duration of ~0.37 s. The K-W light curve of this burst is available at http://www.ioffe.ru/LEA/GRBs/GRB200920_T71814/ As observed by Konus-Wind, the burst had a fluence of 3.12(-0.61,+0.94)x10^-6 erg/cm2 and a 16-ms peak flux, measured from ~T0-0.260 s, of 1.74(-0.52,+0.65)x10^-5 erg/cm2/s (both in the 20 keV - 10 MeV energy range). Since the bulk of the burst emission was detected before the trigger, the spectral analysis was performed using the KW 3-channel light curve data. Modelling the K-W 3-channel spectrum of the burst (measured from T0-0.368 s to T0) by the cutoff power law yields the following model parameters: the photon index alpha = 0.15(-0.51,+0.95), and the peak energy Ep = 935(-241,+401) keV. All the quoted errors are estimated at the 1 sigma confidence level. All the presented results are preliminary.