TITLE: GCN CIRCULAR NUMBER: 20066 SUBJECT: GRB 161014A: Continued RATIR Optical and NIR Observations DATE: 16/10/17 23:23:29 GMT FROM: V. Zach Golkhou at ASU/RATIR V. Zach Golkhou (ASU), Nat Butler (ASU), Alan M. Watson (UNAM), Alexander Kutyrev (GSFC), William H. Lee (UNAM), Michael G. Richer (UNAM), Ori Fox (STScI), J. Xavier Prochaska (UCSC), Josh Bloom (UCB), Antonino Cucchiara (UVI), 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), and Vicki Toy (UMD) report: We observed the field of GRB 161014A (Racusin, et al., GCN 20035) 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 2016/10 16.16 to 2016/10 16.26 UTC (39.29 to 41.69 hours after the BAT trigger), obtaining a total of 1.78 hours exposure in the r and i bands and 0.75 hours exposure in the Z, Y, J, and H bands. For a source within the Swift-XRT error circle (Mingo, et al., GCN 20050) and reported in Golkhou, et al. (GCN 20052), in comparison with the SDSS DR9 and 2MASS catalogs, we obtain the following detection and upper limits (3-sigma): r > 23.79 i 23.57 +/- 0.32 Z > 22.72 Y > 22.57 J > 22.20 H > 21.91 These magnitudes are in the AB system and are not corrected for Galactic extinction in the direction of the GRB. We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir.