TITLE: GCN CIRCULAR NUMBER: 15340 SUBJECT: GRB 131014A: RATIR Optical and NIR Observations DATE: 13/10/15 17:19:59 GMT FROM: Eleonora Troja at GSFC E. Troja (GSFC), Alan M. Watson (UNAM), Nat Butler (ASU), 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), 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 131014A (Fitzpatrick et al., GCN 15332, Desiante, et al., GCN 15333) 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 2013/10 15.36 to 2013/10 15.52 UTC (27.45 to 31.41 hours after the GBM trigger), obtaining a total of 2.84 hours exposure in the r and i bands, 1.19 hours exposure in the Z and Y bands, and 1.09 hours exposure in the J and H bands. For a source within the Swift-XRT error circle (Kennea et al. GCN 15335), in comparison with 2MASS, we obtain the following measurements: r 23.42 ± 0.21 i 22.76 ± 0.17 Z 23.1 ± 0.4 (2.7 sigma) Y 21.20 ± 0.27 J 21.9 ± 0.6 (1.8 sigma) H 21.8 ± 0.7 (1.6 sigma) These magnitudes are in the AB system and are not corrected for Galactic extinction in the direction of the GRB. The object is located 0.4 arcsec from the NOT afterglow candidate (Schulze et al., GCN 15337) and consistent with it. We cannot determine whether the source is fading. No other uncatalogued source is detected within the XRT error circle. Despite the large errors, our preliminary analysis indicates a blue continuum in YJH, suggestive of a possible z-band dropout, and implying a high-redshift (z ~ 6) for GRB 131014A. Further observations are planned. We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir.