[vsnet-grb-info 19711] GRB 170813A: RATIR Optical and NIR Observations

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Mon Aug 14 05:13:38 JST 2017


TITLE:   GCN CIRCULAR
NUMBER:  21472
SUBJECT: GRB 170813A: RATIR Optical and NIR Observations
DATE:    17/08/13 20:13:16 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 (ASU), and Vicki Toy (UMD) report:

We observed the field of GRB 170813A (Page, et al., GCN 21468) 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 2017/08 13.15 to 2017/08 13.18 UTC (2.48 to
3.06 hours after the BAT trigger), obtaining a total of 0.36 hours exposure
in the r and i bands and 0.15 hours exposure in the Z, Y, J, and H bands.

For a source within the Swift-XRT error circle (Osborne, et al., GCN
21469), in comparison with the USNO-B1 and 2MASS catalogs, we obtain the
following upper limits (3-sigma):

  r > 22.46
  i > 22.08
  Z > 20.23
  Y > 19.82
  J > 19.38
  H > 19.13

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.



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