[vsnet-grb-info 20403] GRB 180314B: RATIR Optical Observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Fri Mar 16 08:02:29 JST 2018
TITLE: GCN CIRCULAR
NUMBER: 22499
SUBJECT: GRB 180314B: RATIR Optical Observations
DATE: 18/03/15 23:01:36 GMT
FROM: Alan M. Watson at Instituto de Astronomia UNAM <alan at astro.unam.mx>
Alan M. Watson (UNAM), Nat Butler (ASU), 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 180314B (D'Avanzo et al., GCN 22491) 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 2018/03 15.46 to 2018/03 15.52
UTC (12.55 to 13.99 hours after the BAT trigger), obtaining a total of
1.07 hours exposure in the r and i bands.
For a source within the Swift-XRT error circle, in comparison with the
USNO-B1 and 2MASS catalogs, we obtain the following 3-sigma upper
limits:
r > 23.29
i > 22.90
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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