GCN Circular 40270
Subject
GRB250427A/EP250427a GIT optical afterglow detection:
Date
2025-04-28T12:10:05Z (5 days ago)
From
V. Swain at IIT Bombay <vishwajeet.s@iitb.ac.in>
Via
Web form
V. Swain (IITB), A. Salgundi (IITB), Y. Wagh (IITB), A.P. Saikia (IITB), D. Eappachen (IIA), V. Bhalerao (IITB), G.C. Anupama (IIA), S. Barway (IIA) and K. Angail (IAO) report on behalf of the GIT team:
We observed the field of of EP 250427a (Wang et al., GCN #40257), also detected by Fermi-GBM (Ravasio et al., GCN #40262) with 0.7m GROWTH-India Telescope (GIT) in g and r filters. We started the observation at 2025-04-27 19:19:43 UT, i.e., 15.68 hrs after the EP trigger. The source is detected at EP position and the position reported by TRT network (Liu et al., GRB #40260) and the photometry result follows as:
| JD (mid) | t-t0 (hours) | Filter | Exposure (s) | Mag (AB) |
| ----------------- | ----------- |------- | ------------------ | -------------- |
| 2460793.305359 | 15.68 | r' | 360 | 19.66+/- 0.10 |
| 2460793.318148 | 15.98 | g' | 360 | 20.47+/- 0.10 |
| 2460793.366678 | 17.15 | r' | 360 | 20.00+/- 0.09 |
The measurement is calibrated against PanSTARRS DR1 (Chambers et al., 2016) and not corrected for Galactic extinction.
The object is decaying with powerlaw index of 1.15 +/- 0.04. Further observations are under way. Our result is consistent with BOOTES-7 (Perez-Garcia et al., GCN #40259), TRT (Liu et al., GCN #40260), COLIBRÍ (Becerra et al., GCN #40261), REM (Brivio et al., GCN #40264