TITLE: GCN CIRCULAR NUMBER: 21959 SUBJECT: GRB 171001A: RATIR Optical and NIR Observations DATE: 17/10/02 15:46:07 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 171001A (Lien, et al., GCN 21946) 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 2017/10 2.17 to 2017/10 2.51 UTC (9.63 to 17.69 hours after the BAT trigger), obtaining a total of 5.31 hours exposure in the r and i bands and 2.24 hours exposure in the Z, Y, J, and H bands. We do not detect a source within the XRT error region (Evans, et al., GCN 21952) or at the position of the Nanshan optical transient (Tan, et al., GCN 21957). In comparison with the USNO-B1 and 2MASS catalogs, we obtain the following upper limits (3-sigma): r > 24.15 i > 23.98 Z > 22.96 Y > 22.77 J > 22.43 H > 22.03 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.