TITLE: GCN CIRCULAR NUMBER: 37146 SUBJECT: EP240801a: Assy-Turgen optical observations DATE: 24/08/12 06:35:28 GMT FROM: Alexei Pozanenko at IKI, Moscow N. Pankov (HSE, IKI), V. Kim (FAI), M. Krugov (FAI), S. Belkin (IKI, HSE), A. Pozanenko (IKI) report on behalf of GRB-IKI-FuN: We observed the field of EP240801a (Zhou et al, GCN 36997) with AZT-20 telescope of Assy-Turgen observatory. The observation were conducted on epochs 2024-08-04 17:16, 2024-08-07 19:03, and 2024-08-08 19:36 (UT, starting time). The optical source (Fu et al, GCN 36998; Li et al, GCN 36999; Zheng et al, GCN 37000; Aryan et al, GCN 37002; An et al, GCN 37004; Pérez-Fournon et al, GCN 37007; Malesani et al, GCN 37008; Zhu et al, GCN 37010; Moskvitin & Spiridonova, GCN 37012; Quirola-Vásquez et al, GCN 37013; Moretti et al, GCN 37014; Turpin et al, GCN 37015; Pankov et al, GCN 37016; Moskvitin & Spiridonova, GCN 37017; Ruocco et al, GCN 37024; Pankov et al, GCN 37040; Moskvitin et al, GCN 37049) is detected only on the first epoch. Preliminary photometry is the following: Date UT start t-T0 Exp. Filter OT Err. UL (mid, days) (s) (3sigma) 2024-08-04 17:16:21 3.373472 95*60 r' 23.29 0.14 23.6 2024-08-07 19:03:15 6.437292 65*60 r' n/d n/d 23.9 2024-08-08 19:36:10 7.458070 59*60 r' n/d n/d 24.0 The magnitudes were calibrated using nearby stars from SDSS-DR12 catalog and are not corrected for the expected Galactic extinction A(r) = 0.252 mag (S&F 2011) towards the EP240801a source. The light curve in the r and R filters (AB mags) can be fitted with a smoothed broken power law (Beuermann et al, 1999) with parameters: alpha_1 = 1.1, alpha_2 = 0.33, t_break = 1.5 days with fixed smoothing parameter omega = 1.0. We also note, that there is a point-like source in the LS DR10 at the position of EP240801a. The source magnitudes are g = 25.14, r = 24.40, and the photometric redshift of 0.995 +- 0.352, which is marginally consistent with the redshift of 1.673 obtained with GTC spectroscopy (Quirola-Vásquez et al, GCN 37013).