TITLE: GCN CIRCULAR NUMBER: 17087 SUBJECT: GRB 141121A: Continued RATIR Optical Observations DATE: 14/11/23 07:05:41 GMT FROM: Alan M. Watson at Instituto de Astronomia UNAM 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 (ORAU/GSFC), 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 141121A (Lien et al., GCN 17075) 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 2014/11 22.28 to 2014/11 22.53 UTC (26.79 to 32.94 hours after the BAT trigger), obtaining a total of 4.93 hours exposure in the r, i and z bands. For a source within the Swift-XRT error circle, in comparison with the SDSS DR9, we obtain the following detections and upper limits (3-sigma): r 20.84 +/- 0.03 i 20.68 +/- 0.03 z > 20.02 These magnitudes are in the AB system and are not corrected for Galactic extinction in the direction of the GRB. The source has faded in r and i by 1.2 magnitudes or roughly t^-0.73 since our observations on the first night (Watson et al., GCN 17084), confirming that it is the afterglow. This fading is steeper than the t^-0.15 fading seeing during our observations on the first night. We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir.