TITLE: GCN CIRCULAR NUMBER: 17754 SUBJECT: GRB 150423A: Continued RATIR optical afterglow monitoring DATE: 15/04/24 19:01:43 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 (ORAU/GSFC), 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 again observed the field of GRB 150423A (Pagani, et al., GCN 17728) 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 2015/04 24.18 to 2015/04 24.48 UTC (21.74 to 28.97 hours after the BAT trigger), obtaining a total of 5.69 hours exposure in the r, i and z bands. For a source within the Swift-XRT error circle (Evans, et al., GCN 17735), in comparison with the SDSS DR9, we obtain the following upper limits (3-sigma): r > 24.82 i > 24.79 z > 22.07 These magnitudes are in the AB system and are not corrected for Galactic extinction in the direction of the GRB. In comparison to the earlier epoch of RATIR observations (Littlejohns, et al., GCN 17736), these upper limits indicate fading of at least 1 magnitude in the r and i bands. This implies a continuing power-law decay temporal power-law index of t^-0.5 or steeper, which is consistent with the comparison between the first epoch of RATIR observations and the earlier GROND measurements (Varela, et al., GCN 17732). The magnitude of source 2, as reported in the GROND observations, is consistent with being constant in both epochs of RATIR data. We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir.