GCN Circular 38612
T. Mohan, V. Swain, R. Kumar, A.P. Saikia, V. Bhalerao (IITB), D. Eappachen, A. Balasubramanian, G.C. Anupama, S. Barway (IIA) and K. Angail (IAO) report on behalf of the GIT team:
We observed the field of EP241217a reported by EP-WXT (Zhou et al., GCN 38586) with 0.7m GROWTH-India Telescope (GIT). We started the observation at 2024-12-17T15:31:11 UT, i.e., 9.9 hours after trigger time. We obtained multiple exposures of 360 seconds in the r', i' and z' filters. We detected the source in i'-band at the coordinates given by Gemini North (Levan et al., GCN 38587). The obtained photometry are as follow:
| MJD (mid) | tmid-t0 (in hours) | Filter | Total Exposure (s) | Magnitude (AB) | Lim Mag (5-sigma) |
|---|---|---|---|---|---|
| 60661.77892 | 13.09 | r' | 5x360 | - | 20.8 |
| 60661.69600 | 11.10 | i' | 3x360 | 19.53 +/- 0.10 | 20.4 |
| 60661.75717 | 12.57 | i' | 5x360 | 19.92 +/- 0.11 | 20.4 |
| 60661.73551 | 12.05 | z' | 5x360 | - | 19.2 |
The measurement is calibrated against PanSTARRS DR1 (Chambers et al., 2016) and not corrected for Galactic extinction. The i band flux at the epoch of our observation is higher than the reported r and z band fluxes at earlier epochs in other optical detections (Levan et al., GCN 38587