GCN Circular 29366
Subject
GRB 210123A: AstroSat CZTI detection
Date
2021-01-29T05:46:19Z (4 years ago)
From
Gaurav Waratkar at IIT,Bombay <gauravwaratkar@iitb.ac.in>
D. Nadella (NITK), G. Waratkar (IITB), A. Vibhute (IUCAA), S. Gupta
(IUCAA), P. Sawant (IUCAA), V. Bhalerao (IITB), D. Bhattacharya (IUCAA),
A. R. Rao (IUCAA/TIFR), and S. Vadawale (PRL) report on behalf of the
AstroSat CZTI collaboration:
Analysis of AstroSat CZTI data with the CIFT framework (Sharma et al,
2020, arxiv:2011.07067) showed detection of a long GRB 210123A, which
was also detected by Insight-HXMT/HE (GCN #29349) and Fermi-GBM (GCN
#29351).
The source was detected in the 20-200 keV energy range. The light curve
showed a single peak of emission at 2021-01-23 07:19:08.5 UT. Quadrant A
was noisy, and we exclude it from further analysis. The measured peak
count rate associated with the burst is 205 (+40, -38) cts/s above the
background in the combined data of three quadrants (out of four), with a
total of 996 (+259, -237) cts. The local mean background count rate was
394 (+3, -3) cts/s. Using cumulative rates, we measure a T90 of 14 (+5,
-4) s.
It was also clearly detected in the CsI anticoincidence (Veto) detector
in the 100-500 keV energy range. The light curve showed multiple peaks
of emission with the strongest peak at 2021-01-23 07:19:09.1 UT in all
four quadrants. The measured peak count rate is 1710 (+95, -102) cts/s
above the background in the combined Veto data of four quadrants, with a
total of 8982 (+648, -679) cts. The local mean background count rate was
1817 (+5, -7) cts/s. We measure a T90 of 14 (+5, -1) s from the
cumulative Veto light curve.
CZTI GRB detections are reported regularly on the payload site at
http://astrosat.iucaa.in/czti/?q=grb. CZTI is built by a TIFR-led
consortium of institutes across India, including VSSC, ISAC, IUCAA, SAC
and PRL. The Indian Space Research Organisation funded, managed and
facilitated the project.