TITLE: GCN CIRCULAR NUMBER: 36776 SUBJECT: GRB 240627A: AstroSat CZTI detection DATE: 24/06/28 05:56:16 GMT FROM: Gaurav Waratkar at IIT Bombay gauravwaratkar@iitb.ac.in
J. Joshi (IUCAA), G. Waratkar (IITB), A. Vibhute (IUCAA), V. Bhalerao (IITB), D. Bhattacharya (Ashoka University/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., 2021, JApA, 42, 73) showed the detection of a long-duration GRB 240627A. Inspection of INTEGRAL/SPI-ACS data also showed the detection of the burst. We also note that this trigger is ~13 min after a solar flare in NASA/GOES X-ray flux data. While we cannot accurately localize this GRB because of low counts in our detectors, the relative intensities in different quadrants of CZT and Veto detectors indicate a different source direction.
The source was clearly detected in the CZT detectors in the 20-200 keV energy range. The light curve showed multiple peaks of emission with the strongest peak at 2024-06-27 23:59:01.50 UTC. The measured peak count rate associated with the burst is 502 (+47, -44) counts/s above the background in the combined data of all quadrants, with a total of 2665 (+211, -223) counts. We caution that there is a 0.3 s readout dead time in CZT data during the burst which affects the calculated total counts. The local mean background count rate was 320 (+3, -4) counts/s. Using cumulative rates, we measure a T90 of 11 (+1, -2) s.
The source 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 2024-06-27 23:59:00.62 UTC. The measured peak count rate associated with the burst is 1745 (+92, -99) counts/s above the background in the combined data of all quadrants, with a total of 9056 (+393, -439) counts. The local mean background count rate was 1452 (+7, -8) counts/s. We measure a T90 of 12 (+1, -1) s from the cumulative Veto light curve.
CZTI is built by a TIFR-led consortium of institutes across India, including VSSC, URSC, IUCAA, SAC, and PRL. The Indian Space Research Organisation funded, managed, and facilitated the project.
CZTI GRB detections are reported regularly on the payload site at: http://astrosat.iucaa.in/czti/?q=grb
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