GCN Circular 35826
Subject
GRB 240225B: Mondy afterglow observations
Date
2024-02-28T07:44:44Z (9 months ago)
From
Alexei Pozanenko at IKI, Moscow <apozanen@iki.rssi.ru>
Via
legacy email
N. Pankov (HSE, IKI), A. Pozanenko (IKI), E. Klunko (ISTP), S. Belkin (IKI, HSE)
report on behalf of IKI-GRB-FuN:
We observed the field of GRB 240225B (Nakajima et al., GCN 35796; Evans, GCN 35797,
Joshi et al., GCN 35798; D'Ai et al., GCN 35810; Kawakubo et al., GCN 35811) with
AZT-33IK telescope of Sayan observatory (Mondy) equipped with CMOS-photometer
ANDOR NEO. We took 60x120 sec frames in the R-filter starting on 2024-02-26 (UT)
12:30:03. The optical afterglow (Gompertz et al., GCN 35805; Liu et al., GCN 35812;
Malesani et al., GCN 35819; Wise et al., GCN 35820; Gompertz & Malesani, GCN 35824)
is well detected in the stacked frame with a total exposure of 59x120 sec. Photometry
of the optical afterglow is following:
Date UT-start t-T0 Exp Filter OT Err UL FWHM
(UT) (mid.) (nxT) (3sigma) (arcsec)
2024-02-27 13:01:23 1.71919 59x120 R 19.16 0.09 22.8 2.1
The magnitudes were calibrated using nearby USNO-B1.0 stars (R2 magnitudes).