TITLE: GCN CIRCULAR NUMBER: 18156 SUBJECT: GRB 150817A: Continued RATIR Optical Observations - Afterglow Confirmation DATE: 15/08/18 16:29:47 GMT FROM: Alan M. Watson at Instituto de Astronomia UNAM Alan M. Watson (UNAM), Nat Butler (ASU), Alexander Kutyrev (GSFC), William H. Lee (UNAM), Michael G. Richer (UNAM), Ori Fox (UCB), J. Xavier Prochaska (UCSC), Josh Bloom (UCB), Antonino Cucchiara (ORAU/GSFC), Eleonora Troja (GSFC), Owen Littlejohns (ASU), Enrico Ramirez-Ruiz (UCSC), José A. de Diego (UNAM), Leonid Georgiev (UNAM), Jesús González (UNAM), Carlos Román-Zúñiga (UNAM), Neil Gehrels (GSFC), Harvey Moseley (GSFC), John Capone (UMD), V. Zach Golkhou (ASU), and Vicki Toy (UMD) report: We observed the field of GRB 150817A (D'Elia, et al., GCN 18143) with the Reionization and Transients Infrared Camera (RATIR; www.ratir.org) on the 1.5m Harold Johnson Telescope at the Observatorio Astronómico Nacional on Sierra San Pedro Mártir from 2015/08 18.16 to 2015/08 18.27 UTC (25.78 to 28.42 hours after the BAT trigger), obtaining a total of 1.77 hours exposure in the r, i, and z bands. The first source reported by Butler et al. (GCN 18144) has not faded since our first epoch of observations. The second source, reported by Butler et al. (GCN 18145), has continued to fade and is now only marginally detected. In comparison with the USNO-B1 and 2MASS catalogs, we obtain the following marginal detections and upper limit (3-sigma): r = 23.8 ± 0.4 i = 23.8 ± 0.3 z > 20.2 These magnitudes are in the AB system and are not corrected for Galactic extinction in the direction of the GRB. We note that the second source is consistent with the enhanced Swift-XRT error circle (Osborne et al. GCN 18146). This coincidence and the clear fading suggest that it is the afterglow of the GRB. We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir.