TITLE: GCN CIRCULAR NUMBER: 12696 SUBJECT: GRB 111215A: WHT, LT and NOT imaging DATE: 11/12/16 17:24:54 GMT FROM: Nial Tanvir at U.Leicester N. R. Tanvir, K. Wiersema (U. Leicester), A. Melandri (INAF-OAB), T. Kruehler, J. Fynbo (DARK), A. J. Levan (U. Warwick), C. G. Mundell, R. J. Smith (LJMU), C. Guidorzi (U. Ferrara), D. Xu (WIS) and I. Skillen (ING) report: We imaged the field of GRB111215A (Oates et al. GCN12681) using the WHT, the LT and the NOT, all on La Palma, on the night of 2011-Dec-15 (UT). Seeing conditions were rather poor (FWHM~2"), and no counterpart was located to the following 3-sigma limits at the given mid-times post-burst: WHT/LIRIS (calibrated against 2MASS) K>19.3 at 4hr 55m J>19.4 at 5hr 15m LT/RATCam (calibrated against SDSS) z'>21.7 at 6hr 50m NOT/StanCam (calibrated against SDSS) z'>22.5 at 6hr 50m The K-band limit is consistent with that provided by D'Avanzo et al. (GCN12695) from the TNG, and confirms this source to be dark even in the infrared. We are grateful to Ilia Ilyin for assistance in obtaining the NOT observations.