GCN Circular 22795
Subject
GRB 180611A: AstroSat CZTI detection
Date
2018-06-18T16:37:30Z (7 years ago)
From
Vidushi Sharma at IUCAA <vidushi@iucaa.in>
V. Sharma and D. Bhattacharya (IUCAA), V. Bhalerao (IIT-B), A. R. Rao (TIFR) and S. Vadawale (PRL) report on behalf of the Astrosat CZTI collaboration:
Analysis of Astrosat CZTI data showed the detection of a long GRB 180611A, which was also detected by IPN Triangulation (Hurley K. et al., GCN 22767), Fermi-GBM (Bissaldi E. et al., GCN 22768), Konus-Wind (Tsvetkova A. et al., GCN 22770).
The source was clearly detected in the 40-200 keV energy range. The light curve shows multiple peaks of emission with strongest peak at 03:29:02.5 UT. The measured peak count rate is 265.9 cts/s above the background in combined data of four quadrants, with a total of 1173 cts. The local mean background count rate was 478.1 cts/s. Using cumulative rates, we measure a T90 of 11.5 s.
It was also clearly detected in the CsI anticoincidence (Veto) detector in the 100-500 keV energy range.
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.