TITLE: GCN CIRCULAR NUMBER: 14824 SUBJECT: GRB 130606A: Continued RATIR Optical and NIR Monitoring DATE: 13/06/08 13:54:51 GMT FROM: Nat Butler at UC berkeley 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), 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), and Harvey Moseley (GSFC) report: We observed the field of GRB 130606A (Ukwatta, et al., GCN 14781) 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 2013/06 8.18 to 2013/06 8.46 UTC (31.14 to 37.86 hours after the BAT trigger), obtaining a total of 4.96 hours exposure in the r' and i' bands and 2.07 hours exposure in the Z, Y, J, and H bands. The optical/NIR afterglow (Jelinek, et al., GCN 14782; Xu et al., GCN 14783) is well detected. In comparison with SDSS DR9 and 2MASS, we obtain the following detections and 3-sigma upper limit: r' >24.06 i' 24.06 +/- 0.27 Z 21.50 +/- 0.09 Y 21.41 +/- 0.12 J 21.16 +/- 0.12 H 20.78 +/- 0.12 These magnitudes are in the AB system and not corrected for Galactic extinction in the direction of the GRB. In comparison to our observations on the previous night (2013/06/07; Butler, et al., GCN 14799), the afterglow has faded by about 3 magnitudes in all bands. We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir.