GRB200224B

This page lists all entries on GRB200224B in GRBweb

Summary Fermi GBM GCN 27174 GCN 27181 GCN 27215

Summary table
Variable Value Source
GRB_name_Fermi GRB200224212
T0 5:05:07.294 UTC Fermi_GBM
ra 177.9000° Fermi_GBM
decl -28.8700° Fermi_GBM
pos_error 4.03e+00° Fermi_GBM
T90 299.525 s Fermi_GBM
T90_error 2.862 s Fermi_GBM
T90_start 5:05:07.294 UTC Fermi_GBM
fluence 3.68e-05 erg/cm² Fermi_GBM
fluence_error 5.78e-08 erg/cm² Fermi_GBM
T100 299.525 s
GBM_located True
mjd 58903.211889976854 Fermi_GBM
Fermi GBM table
GRB_name_Fermi GRB200224212
trigger_name bn200224212
ra 177.9000°
decl -28.8700°
pos_error 4.03e+00°
datum 2020-02-24
t_trigger 5:05:49.279 UTC
T90 299.525 s
T90_error 2.862 s
T90_start 5:05:07.294 UTC
fluence 3.68e-05 erg/cm²
fluence_error 5.78e-08 erg/cm²
flux_1024 7.73e+00 erg/cm²/s
flux_1024_error 2.89e-01 erg/cm²/s
flux_1024_time 2.14e+02 erg/cm²/s
flux_64 1.10e+01 erg/cm²/s
flux_64_error 1.35e+00 erg/cm²/s
GCN 27174 table
GRB_name GRB200224B
GCN_number 27174
Detection_method Fermi GBM final loc
t_trigger 5:05:49 UTC
ra 177.9000°
decl -28.9000°
Circular_text TITLE: GCN CIRCULAR NUMBER: 27174 SUBJECT: GRB 200224B: Fermi GBM Final Real-time Localization DATE: 20/02/24 05:16:06 GMT FROM: Fermi GBM Team at MSFC/Fermi-GBM The Fermi GBM team reports the detection of a likely LONG GRB At 05:05:49 UT on 24 Feb 2020, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 200224A (trigger 604213554.278888 / 200224212). The on-ground calculated location, using the Fermi GBM trigger data, is RA = 177.9, Dec = -28.9 (J2000 degrees, equivalent to J2000 11h 51m, -28d 53'), with a statistical uncertainty of 3.1 degrees. The angle from the Fermi LAT boresight is 23.0 degrees. The skymap can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2020/bn200224212/quicklook/glg_skymap_all_bn200224212.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/bn200224212/quicklook/glg_healpix_all_bn200224212.fit The GBM light curve can be found here: https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2020/bn200224212/quicklook/glg_lc_medres34_bn200224212.gif [GCN OPS NOTE(24feb20): This is the third Circular in the sequence of 8 circulars which were all labeled A because of the sequence assigner being offline. This circular was orginally, incorrectly labelled A, but the true letter identity is B.]
GCN 27181 table
GRB_name GRB200224B
GCN_number 27181
Detection_method Fermi GBM Other
Circular_text TITLE: GCN CIRCULAR NUMBER: 27181 SUBJECT: Correction in name: GRB 200224B and GRB 200224C (not GRB 200224A) DATE: 20/02/24 21:32:30 GMT FROM: Stephen Lesage at Fermi-GBM Team S. Lesage (UAH) reports on behalf of the Fermi GBM Team: “The Fermi Gamma-ray Burst Monitor (GBM) triggers 604213554/200224212 at 05:05:49 UT and 604231129/200224416 at 09:58:44 on 24 Feb 2020, originally named GRB 200224A in GCN 27174 and GCN 27178, should be GRB 200224B and GRB 200224C respectively. We apologize for any confusion caused."
GCN 27215 table
GRB_name GRB200224B
GCN_number 27215
Detection_method Optical
Circular_text TITLE: GCN CIRCULAR NUMBER: 27215 SUBJECT: GRB 200224B: DDOTI/OAN optical observations report DATE: 20/02/26 00:30:12 GMT FROM: Emma Margarita Pereyra Talamantes at IA-UNAM Ensenada Margarita Pereyra (UNAM), Nat Butler (ASU), Alan M. Watson (UNAM), Eleonora Troja (GSFC/UMD), Simone Dichiara (GSFC/UMD), Rosa L. Becerra (UNAM), William H. Lee (UNAM), Diego Gonzalez (UNAM), Alexander Kutyrev (GSFC/UMD), and Tanner Wolfram (ASU), report: We observed the field of GRB 200224B detected by the Fermi Gamma-ray Burst Monitor (GCN 27174, Fermi trigger 604213554), with the DDOTI/OAN wide-field imager at the Observatorio Astronómico Nacional on Sierra San Pedro Mártir ( http://ddoti.astroscu.unam.mx) from 2020-02-24 06:47 to 2020-02-24 12:16 UTC (1.68 to 7.16 hours after the event). We observed a region of 13.6 degrees in RA by 20.4 degrees in declination, with a 2 x 2 grid, centered on the Fermi GBM Final Position +11:51:36 -28:52:11 J2000. This region contains about 277 square degrees. We obtained 2040 to 2520 seconds exposure across the region. We calibrated our images against the APASS catalog. Our 10-sigma limiting magnitude is around w = 19.45. Comparing to the USNO-B1, DSS DR2 and Pan-STARRS DR1 catalogs, we do not detect any uncataloged source with significant fading within the 90% probability radius of 6.3 degrees. We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir. -- *Dr. Margarita Pereyra * *FFTF, Schlumberger Foundation Alumnae* ---------------------------------------------------------------------------------------------------------------- *Catedrático Conacyt* *Instituto de Astronomía de la UNAM,* *Km. 107 Carretera Tijua**na-Ensenada, * *Ensenada Baja California, México. C.P. 22860* Oficina: 405 Skype: margarita-pereyra