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GCN Circular 14831

Subject

GRB 130609A: RATIR Optical and NIR Observations

Date

2013-06-09T06:33:31Z (12 years ago)

Edited On

2024-11-07T18:50:05Z (3 months ago)

From

Nat Butler at Az State U <natbutler@asu.edu>

Edited By

Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov> on behalf of Leo P. Singer at NASA/GSFC <leo.p.singer@nasa.gov>

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), Antonino Cucchiara (UCSC),
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 130609A (Cummings, et al., GCN 14828Loading...
 
 ) 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 2013/06 9.15 to 2013/06 9.23 UTC (0.56 to 2.52
hours after the BAT trigger), obtaining a total of 1.24 hours exposure in
the r' and i' bands and 0.60 hours exposure in the Z, Y, J, and H bands.

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

  r'    > 23.34
  i'    > 23.27
  Z     > 22.39
  Y     > 21.91
  J     > 21.72
  H     > 21.06

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

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