| Summary table |
|---|
| Variable |
Value |
Source |
| T0 |
17:36:11 UTC |
GCN_circulars,Fermi GBM final loc |
| ra |
59.2000° |
GCN_circulars,Fermi GBM final loc |
| decl |
51.7000° |
GCN_circulars,Fermi GBM final loc |
| GBM_located |
True |
|
| mjd |
59986.733460648145 |
GCN_circulars,Fermi GBM final loc |
| GCN 33316 table |
|---|
| GRB_name |
GRB230211A |
| GCN_number |
33316 |
| Detection_method |
Fermi GBM final loc |
| t_trigger |
17:36:11 UTC |
| ra |
59.2000° |
| decl |
51.7000° |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 33316
SUBJECT: GRB 230211A: Fermi GBM Final Real-time Localization
DATE: 23/02/11 17:46:37 GMT
FROM: Fermi GBM Team at MSFC/Fermi-GBM
The Fermi GBM team reports the detection of a likely LONG GRB
At 17:36:11 UT on 11 Feb 2023, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 230211A (trigger 697829776.865304 / 230211733).
The on-ground calculated location, using the Fermi GBM trigger data, is RA = 59.2, Dec = 51.7 (J2000 degrees, equivalent to J2000 03h 56m, 51d 42'), with a statistical uncertainty of 14.6 degrees.
The angle from the Fermi LAT boresight is 77.0 degrees.
The skymap can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2023/bn230211733/quicklook/glg_skymap_all_bn230211733.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/bn230211733/quicklook/glg_healpix_all_bn230211733.fit
The GBM light curve can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2023/bn230211733/quicklook/glg_lc_medres34_bn230211733.gif
|
| GCN 33317 table |
|---|
| GRB_name |
GRB230211A |
| GCN_number |
33317 |
| Detection_method |
Fermi GBM Other |
| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 33317
SUBJECT: 230211A is not a GRB
DATE: 23/02/11 20:05:44 GMT
FROM: Suraj Poolakkil at UAH
S. Poolakkil (UAH) reports on behalf of the Fermi Gamma-ray Burst Monitor
Team:
"The Fermi Gamma-ray Burst Monitor (GBM) trigger 697829776/230211733 at
17:36:11.87 UT
on 11 February 2023, tentatively classified as GRB 230211A (GCN 33316), is
in fact not due
to a GRB. This trigger is likely due to LS V +44 17 / RX J0440.9+4431."
--
Suraj Poolakkil
Fermi GBM Graduate Research Assistant
Dept. of Space Science
University of Alabama in Huntsville
|