[vsnet-grb-info 19880] GRB 171001A: RATIR Optical and NIR Observations

[GCN Circulars]

TITLE:   GCN CIRCULAR
NUMBER:  21959
SUBJECT: GRB 171001A: RATIR Optical and NIR Observations
DATE:    17/10/02 15:46:07 GMT
FROM:    Nat Butler at Az State U  <natbutler at asu.edu>

Nat Butler (ASU), Alan M. Watson (UNAM), Alexander Kutyrev (GSFC), William
H. Lee (UNAM), Michael G. Richer (UNAM), Ori Fox (STScI), J. Xavier
Prochaska (UCSC), Josh Bloom (UCB), Antonino Cucchiara (UVI), Eleonora
Troja (GSFC), Owen Littlejohns (ASU), Enrico Ramirez-Ruiz (UCSC), Jesús
González (UNAM), Carlos Román-Zúñiga (UNAM), Harvey Moseley (GSFC), John
Capone (UMD), V. Zach Golkhou (U. Wash.), and Vicki Toy (UMD) report:

We observed the field of GRB 171001A (Lien, et al., GCN 21946) 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 2017/10 2.17 to 2017/10 2.51 UTC (9.63 to
17.69 hours after the BAT trigger), obtaining a total of 5.31 hours
exposure in the r and i bands and 2.24 hours exposure in the Z, Y, J, and H
bands.

We do not detect a source within the XRT error region (Evans, et al., GCN
21952) or at the position of the Nanshan optical transient (Tan, et al.,
GCN 21957).  In comparison with the USNO-B1 and 2MASS catalogs, we obtain
the following upper limits (3-sigma):

 r > 24.15
 i > 23.98
 Z > 22.96
 Y > 22.77
 J > 22.43
 H > 22.03

These magnitudes are in the AB system and are not corrected for Galactic
extinction in the direction of the GRB.

We thank the staff of the Observatorio Astronómico Nacional in San Pedro
Mártir.