GCN Circular 15892
Subject
GRB 140226A/iPTF14yb: RATIR Optical and NIR Observations
Date
2014-02-28T15:47:46Z (10 years ago)
From
Antonino Cucchiara at NASA/GSFC <antonino.cucchiara@nasa.gov>
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),
Jos� A. de Diego (UNAM), Leonid Georgiev (UNAM), Jes�s Gonz�lez (UNAM),
Carlos Rom�n-Z��iga (UNAM), Neil Gehrels (GSFC), and Harvey Moseley (GSFC) report:
We observed again the field of the GRB-like transient iPTF14yb (Cenko et al., GCN 15883,
Beardmore et al., GCN 15884, 15891) with the Reionization and Transients Infrared Camera
(RATIR; www.ratir.org) on the 1.5m Harold Johnson Telescope at the Observatorio Astron�mico
Nacional on Sierra San Pedro M�rtir from 2014/02 28.34 to 2014/02 28.53 UTC (roughly 46
to 50 hours after the reported time of discovery), obtaining a total of 2.63 hours exposure
in the r and i bands and 1.12 hours exposure in the Z and J bands.
For the source within the Cenko et al. (GCN 15883) error circle, in comparison with the
SDSS DR9 and 2MASS, we obtain the following detections and upper limits:
r 23.28 +/- 0.32
i 22.51 +/- 0.20
Z > 22.11
J > 21.73
The detections are at the 2-sigma level and the upper limits at the 3-sigma level.
These magnitudes are in the AB system and are not corrected for Galactic
extinction in the direction of the GRB.
Our photometry indicates that the transient is still fading in r band with a similar
decay index (within the systematic errors) as reported by Cucchiara et al. (GCN
15886).
We thank the staff of the Observatorio Astron�mico Nacional in San Pedro
M�rtir.
[GCN OPS NOTE(28feb14): Per author's reuqest, the Y & H bands were removed
from the last sentence in the first paragraph.]