[vsnet-grb-info 15828] GRB 141121A: Continued RATIR Optical Observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Sun Nov 30 01:15:29 JST 2014
TITLE: GCN CIRCULAR
NUMBER: 17116
SUBJECT: GRB 141121A: Continued RATIR Optical Observations
DATE: 14/11/29 16:15:21 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), Chris Klein (UCB), Ori Fox (UCB), J.
Xavier Prochaska (UCSC), Josh Bloom (UCB), Antonino Cucchiara (ORAU/GSFC),
Eleonora Troja (GSFC), 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 141121A (Lien et al., GCN 17075) 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 2014/11 29.29 to 2014/11 29.53 UTC (195.13 to 200.87 hours
after the BAT trigger), obtaining a total of 4.62 hours exposure in the r, i and
z bands.
For a source within the Swift-XRT error circle, in comparison with the SDSS DR9,
we obtain the following detections and upper limits (3-sigma):
r = 22.15 +/- 0.06
i = 21.97 +/- 0.06
z > 21.04
These magnitudes are in the AB system and are not corrected for Galactic
extinction in the direction of the GRB.
The afterglow continues to fade with a steepening temporal index.
We thank the staff of the Observatorio Astronómico Nacional in San Pedro Mártir.
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