TITLE: GCN CIRCULAR NUMBER: 15067 SUBJECT: GRB 130803A: RATIR Optical and NIR Observations DATE: 13/08/04 07:00:59 GMT FROM: Owen Littlejohns at Az State U Owen Littlejohns (ASU), Nat Butler (ASU), Alan M. Watson (UNAM), Alexander Kutyrev (GSFC), William H. Lee (UNAM), Michael G. Richer (UNAM), Chris Klein (UCB), Ori Fox (UCB), J. Xavier Prochaska (UCSC), Josh Bloom (UCB), Antonino Cucchiara (UCSC), Eleonora Troja (GSFC), Enrico Ramirez-Ruiz (UCSC), José A. de Diego (UNAM), Leonid Georgiev (UNAM), Jesús González (UNAM), Carlos Román-Zúñiga (UNAM), Neil Gehrels (GSFC), and Harvey Moseley (GSFC) report: We observed the field of GRB 130803A (Page, et al., GCN 15059) 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 2013/08 4.15 to 2013/08 4.25 UTC (17.51 to 19.98 hours after the BAT trigger), obtaining a total of 1.53 hours exposure in the r' and i' bands and 0.63 hours exposure in the Z, Y, J, and H bands. For a source within the Swift-XRT error circle, in comparison with SDSS DR9 and 2MASS, we obtain the following upper limits (3-sigma): r' > 23.29 i' > 23.24 Z > 22.27 Y > 21.70 J > 20.90 H > 20.24 These magnitudes are in the AB system and not corrected for Galactic extinction in the direction of the GRB. Our upper limits are consistent with the detections and upper limits reported by Varela, et al. (GCN 15066). We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir.