TITLE: GCN CIRCULAR NUMBER: 21210 SUBJECT: GRB 170531B: Zeiss-1000/CrAO optical observations DATE: 17/06/07 21:38:36 GMT FROM: Alexei Pozanenko at IKI, Moscow E. Mazaeva (IKI), A. Pozanenko (IKI), D. Chestnov (ISON), A. Novichonok (ISON), V. Agletdinov (KIAM), I. Nikolenko (CrAO), A. Volnova (IKI), report on behalf of larger GRB follow-up collaboration: We report refined analysis of Zeiss-1000/CrAO observations. Results reported below supersede GCN cir. 21174. We observed the field of the GRB 170531B (Evans et al., GCN 21171) with Zeiss-1000/Koshka (CrAO) telescope between May 31 (UT) 22:32:32 and June 01 (UT) 00:58:11. We took several unfiltered images with exposure of 180 s. The afterglow (Lipunov et al. GCN 21173; Pozanenko et al. GCN 21174) is clearly visible in each image in first initial images, and detected later in combined images. The finding chart of the combined image can be found at http://grb.rssi.ru/GRB170531B/GRB170531B_Koshka_170531_sources.png The coordinates of the afterglow (source A in the finding chart) are (J2000) 19:07:32.10 -16:25:06.0 with uncertainty of 0.5 arcsec in both coordinates. The coordinates are consistent with the position reported by de Ugarte Postigo et al., GCN 21177, Tyurina et al., GCN 21179, and Siegel et al., GCN 21188. Preliminary photometry of the afterglow can be found in the light curve at http://grb.rssi.ru/GRB170531B/GRB170531B_light_curve_v2.png The photometry is based on nearby USNO-B1.0 stars, calibrated against to R2 magnitudes USNO-B.1_id R2 0736-0718845 16.77 0735-0729622 16.96 0735-0729439 16.59 0735-0729327 17.22 Due to presence of sources in near vicinity to the afterglow the photometry of wide FOV telescopes might be affected by the sources. In particular our photometry reported in GCN 21189 is apparently biased by the two sources C and D (see the finding chart). We report coordinates and brightness of the nearby sources. Source coordinates(J2000) AG distance filter mag. err. C 19:07:32.34 -16:25:09.1 4.6" CR 20.46 0.04 D 19:07:31.83 -16:25:05.6 3.9" CR 20.47 0.04