GRB 241011A
GCN Circular 37775
A. Myers (NPP/GSFC) reports on behalf of the Fermi Gamma-ray Burst Monitor Team:
"The Fermi Gamma-ray Burst Monitor (GBM) trigger 750372658/241011869 (GRB 241011A; GCN 37774) at 20:50:53.89 UT on 11 October 2024, tentatively classified as a GRB, is in fact not due to a GRB. This trigger is likely due to local particles."
GCN Circular 37774
The Fermi GBM team reports the detection of a likely LONG GRB
At 20:50:53 UT on 11 Oct 2024, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 241011A (trigger 750372658.888186 / 241011869).
The on-ground calculated location, using the Fermi GBM trigger data, is RA = 68.6, Dec = -29.9 (J2000 degrees, equivalent to J2000 04h 34m, -29d 53'), with a statistical uncertainty of 7.0 degrees.
The angle from the Fermi LAT boresight is 73.0 degrees.
The skymap can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2024/bn241011869/quicklook/glg_skymap_all_bn241011869.png
The HEALPix FITS file, including the estimated localization systematic, can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2024/bn241011869/quicklook/glg_healpix_all_bn241011869.fit
The GBM light curve can be found here:
https://heasarc.gsfc.nasa.gov/FTP/fermi/data/gbm/triggers/2024/bn241011869/quicklook/glg_lc_medres34_bn241011869.gif