TITLE: GCN CIRCULAR NUMBER: 15137 SUBJECT: GRB 130822A: optical upper limits DATE: 13/08/30 13:20:03 GMT FROM: Alexei Pozanenko at IKI, Moscow A. Volnova (IKI), R.Inasaridze (AAO), O. Kvaratskhelia (AAO), V. Ayvazian(AAO), Yu. Krugly (IA KhNU), I. Slyusarev (IA KhNU), I. Molotov (KIAM), V. Linkov (ISON), A. Pozanenko (IKI) report on behalf of larger GRB follow-up collaboration: We observed the field of Swift GRB 130822A (Kocevski et al., GCN 15112) on Aug., 22 with AS-32 (0.7m) telescope of Abastumani Observatory, SANTEL-400AN (0.4m) telescope of ISON-Kislovodsk observatory, and AZT-8 (0.7m) telescope of Institute of Astronomy, Kharkiv National University. We obtained several unfiltered frames with exposures of 120 s (AS-32), 100 s and 60 s (SANTEL-400AN), and several frames with filter R with exposure of 120 s (AZT-8). Within the enhanced XRT circle (Beardmore et al., GCN 15117) we did not detect any source on stacked images. The details of the photometry are the following: Telescope t_start, UT filter exptime,s t-t0, mid, days uplim AZT-8 21:39:21 R 55*120 0.28000 20.6 S-400 22:31:37 None 23*100 0.30332 19.3 AS-32 23:46:59 None 40*120 0.36513 21.9 The photometry is based on SDSS stars, R mag (R mag obtained via transformations ugriz in BVRI (Lupton, 2005): SDSS id R R_err J015202.75-031421.9 12.80 0.012 J015134.64-031348.8 13.95 0.013 J015148.69-030854.9 14.62 0.013