TITLE: GCN CIRCULAR NUMBER: 22182 SUBJECT: GRB 171205A: RATIR Optical and NIR Observations DATE: 17/12/05 15:10:17 GMT FROM: Nat Butler at Az State U 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), Jesús González (UNAM), Carlos Román-Zúñiga (UNAM), Harvey Moseley (GSFC), John Capone (UMD), V. Zach Golkhou (U. Wash.), and Vicki Toy (UMD) report: We observed the field of GRB 171205A (D'Elia, et al., GCN 22177) 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 2017/12 5.40 to 2017/12 5.53 UTC (2.15 to 5.36 hours after the BAT trigger), obtaining a total of 1.44 hours exposure in the r and i bands and 0.71 hours exposure in the Z and Y bands. In comparison with the USNO-B1 and 2MASS catalogs, we detect and obtain the following photometry for the source reported by Izzo et al. (GCN 22180): r = 18.30 +/- 0.05 i = 18.13 +/- 0.02 Z = 18.35 +/- 0.05 Y = 18.13 +/- 0.05 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.