[vsnet-grb-info 14067] GRB 131024B: RATIR Optical and NIR Observations

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Sat Oct 26 00:45:23 JST 2013


TITLE:   GCN CIRCULAR
NUMBER:  15381
SUBJECT: GRB 131024B: RATIR Optical and NIR Observations
DATE:    13/10/25 15:45:15 GMT
FROM:    Antonino Cucchiara at UCSC/UCO Lick  <acucchia at ucolick.org>

Antonino Cucchiara (ORAU/GSFC), Nat Butler (ASU), Alan M. Watson (UNAM), 
Alexander Kutyrev (GSFC), William H. Lee (UNAM), Michael G. Richer (UNAM), 
Chris Klein (UCB), Ori Fox (UCB), J. Xavier Prochaska (UCSC), Josh Bloom (UCB), 
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 131024B (Krimm, et al., GCN 15371) 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 25.41 to 2013/10 25.52 UTC (12.28
to 14.87 hours after the BAT trigger), obtaining a total of 1.78 hours
exposure in the r and i bands and 0.74 hours exposure in the Z,
Y, J, and H bands.

For a source within the Swift-XRT error circle, in comparison with the SDSS DR9 
and 2MASS, we obtain the following upper limits (3-sigma):

  r	> 23.68
  i	> 23.35
  Z	> 22.44
  Y	> 22.01
  J	> 21.75
  H	> 21.49

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.


More information about the vsnet-grb-info mailing list