GRB201222B

This page lists all entries on GRB201222B in GRBweb

Summary Fermi GBM GCN 29126 GCN 29127 GCN 29143

Summary table
Variable Value Source
GRB_name_Fermi GRB201222461
T0 11:03:22.230 UTC Fermi_GBM
ra 95.6700° Fermi_GBM
decl 27.8900° Fermi_GBM
pos_error 4.40e+00° Fermi_GBM
T90 7.872 s Fermi_GBM
T90_error 3.328 s Fermi_GBM
T90_start 11:03:22.230 UTC Fermi_GBM
fluence 1.99e-06 erg/cm² Fermi_GBM
fluence_error 6.84e-08 erg/cm² Fermi_GBM
T100 7.872 s
GBM_located True
mjd 59205.46067395833 Fermi_GBM
Fermi GBM table
GRB_name_Fermi GRB201222461
trigger_name bn201222461
ra 95.6700°
decl 27.8900°
pos_error 4.40e+00°
datum 2020-12-22
t_trigger 11:03:25.686 UTC
T90 7.872 s
T90_error 3.328 s
T90_start 11:03:22.230 UTC
fluence 1.99e-06 erg/cm²
fluence_error 6.84e-08 erg/cm²
flux_1024 6.64e+00 erg/cm²/s
flux_1024_error 3.86e-01 erg/cm²/s
flux_1024_time 2.56e-01 erg/cm²/s
flux_64 9.38e+00 erg/cm²/s
flux_64_error 1.75e+00 erg/cm²/s
GCN 29126 table
GRB_name GRB201222B
GCN_number 29126
Detection_method Fermi GBM final loc
t_trigger 11:03:25 UTC
ra 95.7000°
decl 27.9000°
Circular_text TITLE: GCN CIRCULAR NUMBER: 29126 SUBJECT: GRB 201222B: Fermi GBM Final Real-time Localization DATE: 20/12/22 11:10:57 GMT FROM: Fermi GBM Team at MSFC/Fermi-GBM The Fermi GBM team reports the detection of a likely LONG GRB At 11:03:25 UT on 22 Dec 2020, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 201222B (trigger 630327810.6864 / 201222461). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 95.7, Dec = 27.9 (J2000 degrees, equivalent to J2000 06h 22m, 27d 53'), with a statistical uncertainty of 5.0 degrees. The angle from the Fermi LAT boresight is 107.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2020/bn201222461/quicklook/glg_skymap_all_bn201222461.png The HEALPix FITS file, including the estimated localization systematic, can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2020/bn201222461/quicklook/glg_healpix_all_bn201222461.fit The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2020/bn201222461/quicklook/glg_lc_medres34_bn201222461.gif
GCN 29127 table
GRB_name GRB201222B
GCN_number 29127
Detection_method Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 29127 SUBJECT: GRB 201222B: BALROG localization (Fermi Trigger / GRB 201222461) DATE: 20/12/22 11:45:58 GMT FROM: Jochen Greiner at MPE,Garching F. Kunzweiler, B. Biltzinger, F. Berlato, J. Burgess & J. Greiner (all MPE Garching) report: The public trigdat data of the Fermi Gamma-ray Burst Monitor (GBM) trigger at 11:03:25 on 22 Dec. 2020 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 (1 sigma statistical errors) is: RA(2000.0) = 99.7+/-3.0 deg Decl.(2000.0) = 27.7+/-4.7 deg We estimate an additional systematic error of 1 deg. Further details are available at: https://grb.mpe.mpg.de/grb/GRB201222461/ The Healpix map can be downloaded from: https://grb.mpe.mpg.de/grb/GRB201222461/healpix The location parameters are available as JSON at: https://grb.mpe.mpg.de/grb/GRB201222461/json
GCN 29143 table
GRB_name GRB201222B
GCN_number 29143
Detection_method Fermi GBM Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 29143 SUBJECT: Fermi GRB 201222B: Global MASTER-Net observations report DATE: 20/12/23 01:15:28 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs V. Lipunov, E. Gorbovskoy, V.Kornilov, N.Tyurina, P.Balanutsa, A.Kuznetsov, F.Balakin, V.Vladimirov, D. Vlasenko, I.Gorbunov, D.Zimnukhov, V.Senik, T.Pogrosheva, D.Kuvshinov, D. Cheryasov (Lomonosov Moscow State University, SAI, Physics Department), R. Podesta, C.Lopez, F. Podesta, C.Francile (Observatorio Astronomico Felix Aguilar OAFA), R. Rebolo, M. Serra (The Instituto de Astrofisica de Canarias), D. Buckley (South African Astronomical Observatory), O.A. Gres, N.M. Budnev, O.Ershova (Irkutsk State University, API), A. Tlatov, D. Dormidontov (Kislovodsk Solar Station of the Pulkovo Observatory), V. Yurkov, A. Gabovich, Yu. Sergienko (Blagoveschensk Educational State University) MASTER-OAFA robotic telescope (Global MASTER-Net: http://observ.pereplet.ru, Lipunov et al., 2010, Advances in Astronomy, vol. 2010, 30L) located in Argentina (OAFA observatory of San Juan National University) started inspect of the Fermi GRB 201222B ( Fermi GBM team, GCN 29126) errorbox 49075 sec after notice time and 49125 sec after trigger time at 2020-12-23 00:42:11 UT, with upper limit up to 17.3 mag. Observations started at twilight. The observations began at zenith distance = 77 deg. The sun altitude is -12.3 deg. The galactic latitude b = 7 deg., longitude l = 185 deg. Real time updated cover map and OT discovered available here: https://master.sai.msu.ru/site/master2/observ.php?id=1509240 We obtain a following upper limits. Tmid-T0 | Date Time | Site | Coord (J2000) |Filt.| Expt. | Limit| Comment _________|_____________________|_____________________|____________________________________|_____|_______|_______|________ 49156 | 2020-12-23 00:42:11 | MASTER-OAFA | (06h 02m 01.37s , +23d 18m 10.6s) | C | 60 | 16.0 | 49315 | 2020-12-23 00:44:50 | MASTER-OAFA | (06h 13m 54.23s , +21d 18m 00.8s) | C | 60 | 16.4 | 49635 | 2020-12-23 00:50:11 | MASTER-OAFA | (05h 56m 25.50s , +27d 17m 21.2s) | C | 60 | 16.4 | 49874 | 2020-12-23 00:54:09 | MASTER-OAFA | (06h 07m 58.78s , +25d 17m 26.6s) | C | 60 | 16.5 | 50033 | 2020-12-23 00:56:48 | MASTER-OAFA | (06h 19m 26.67s , +23d 18m 41.9s) | C | 60 | 16.8 | 50113 | 2020-12-23 00:58:08 | MASTER-OAFA | (06h 01m 56.11s , +23d 19m 19.9s) | C | 60 | 17.1 | 50193 | 2020-12-23 00:59:28 | MASTER-OAFA | (06h 10m 47.69s , +23d 18m 33.8s) | C | 60 | 17.0 | 50356 | 2020-12-23 01:02:11 | MASTER-OAFA | (05h 59m 04.32s , +25d 17m 30.8s) | C | 60 | 17.2 | 50436 | 2020-12-23 01:03:31 | MASTER-OAFA | (06h 13m 54.45s , +21d 19m 15.0s) | C | 60 | 17.3 | 50516 | 2020-12-23 01:04:51 | MASTER-OAFA | (06h 22m 32.36s , +21d 18m 24.3s) | C | 60 | 17.2 | Filter C is a clear (unfiltred) band. The observation and reduction will continue. The message may be cited.