TITLE: GCN CIRCULAR NUMBER: 29843 SUBJECT: GRB 210419C: RATIR Optical and NIR Upper Limits DATE: 21/04/20 16:34:17 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 210419C (Moss, et al., GCN 29834) with the Reionization and Transients Infrared Camera (RATIR) on the 1.5m Harold Johnson Telescope at the Observatorio Astronómico Nacional on Sierra San Pedro Mártir from 2021/04 20.14 to 2021/04 20.50 UTC (2.58 to 11.15 hours after the BAT trigger), obtaining a total of 4.53 hours exposure in the r and i bands and 1.89 hours exposure in the Z, Y, J, and H bands. We do not detect any sources within the enhanced XRT error region (Beardmore, et al. GCN 29839). In comparison with the SDSS DR9 and 2MASS catalogs, we obtain the following upper limits (3-sigma): r > 23.60 i > 23.53 Z > 22.31 Y > 20.10 J > 22.21 H > 21.87 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.