Skip to main content
Testing. You are viewing the public testing version of GCN. For the production version, go to
New Announcement Feature, Code of Conduct, Circular Revisions. See news and announcements

GCN Circular 17170

GRB 141212A: extended object within the XRT error circle
2014-12-12T22:18:17Z (9 years ago)
Daniele Malesani at Dark Cosmology Centre, Niels Bohr Inst <>
D. Malesani (DARK/NBI), P. D'Avanzo (INAF/OABr), V. D'Elia (INAF/OAR and 
ASI/ASDC), S. D. Vergani (CNRS/GEPI), G. Andreuzzi (INAF/TNG), A. Garcia 
de Gurtubai Escudero (INAF/TNG), A. Bonomo (INAF/OATo), report on behalf 
of the CIBO collaboration:

We observed the field of GRB 141212A (Ukwatta et al., GCN 17158) using 
the TNG optical telescope located in La Palma. Observations started on 
2014 Dec 12.832 UT (7.73 hr after the GRB) and consisted of 10x240 s in 
the R band. The PSF in our image was around 1.5".

Within the XRT error circle (Osborne et al., GCN 17164; see also, we detect a single, extended 
object (A), with coordinates (J2000):

RA = 02:36:29.95
Dec = +18:08:47.2

Its Vega magnitude is R = 22.66 +- 0.23, assuming R = 16.83 for the USNO 
star at RA = 02:36:35.95, Dec = +18:09:16.8.

We cannot yet make any claim about variability, so the connection of 
this object with GRB 141212A is unclear. This may be the GRB host, 
though some contribution from an afterglow cannot be excluded.

We also note the presence of two extended objects just outside the XRT 
error circle.

(B): RA = 02:36:30.25, Dec = +18:08:50.1, R = 22.29 +- 0.16;
(C): RA = 02:36:29.64, Dec = +18:08:50.2, R ~ 24.0

Object (C) is barely detected. No other sources are visibile in the 
proximity of the XRT error circle down to a limiting magnitude of R = 24.

A finding chart can be seen at the following URL:
Looking for U.S. government information and services? Visit