GCN Circular 10247

A. de Ugarte Postigo (INAF-OAB), A.J. Castro-Tirado, J. Gorosabel, M. 
Jel�nek, S. Guziy (IAA-CSIC), A. Cabrera-Lavers, D. Garc�a, G. G�mez 
(GTC/IAC), G. Bergond (CAHA), D. P�rez-Ram�rez (Univ. de Ja�n), R. 
Cuniffe (IAA-CSIC) and P. Kub�nek (IAA-CSIC, U. Valencia) report on 
behalf of a larger collaboration:

"We have observed the field of the INTEGRAL GRB 091202  (Mereghetti et 
al. GCN 10234
Not found
 
 
) using OSIRIS at the 10.4m Gran Telescopio Canarias (GTC) 
at the Observatorio del Roque de los Muchachos of the Instituto de 
Astrof�sica de Canarias, in the island of La Palma. Observations were 
carried out between 04:55 and 05:23 UT on 4 December 2009 (~1.25 days 
after the burst). The observation consisted of 5x30s exposures in r, i 
and z bands. Addtional near-IR observations were obtained in with 
Omega2000 at the 3.5m telescope at the German-Spanish Calar Alto 
Observatory in J, H and K' bands between 01:06 and 04:46 UT.

Within the XRT error circle (Vetere et al. GCN 10239
Not found
 
 
) we detect two 
sources, one point-like and one apparently extended in all three GTC 
frames. Only one source (point-like) shows up in the near-IR frame, 
which appears to be superimposed to the extended one seen in the 
optical. This will imply a strong red colour (r-H >= 4) typical of GRB 
afterglows (Gorosabel et al. 2002, A&A 384, 11). Hence, we identify this 
source as the likely afterglow to GRB 091202, at coordinates (J2000.0):

R.A.:  09 15 19.75
Dec.: +62 32 59.0

with a 0".5 astrometry error.

At a mean epoch of 1.25 days after the burst, we measure for it a 
magnitude of r = 23.7 � 0.1. From the nIR observations we measure H = 
19.7 � 0.2. at a mean epoch 1.21 days after the burst. For the optical 
photometry we used the SDSS star located at coordinates R.A.: 09 15 
21.23, Dec: +62 32 33.4 (J2000.0) for which we assume a magnitude of r = 
21.27. The nIR images were calibrated against a 2MASS star at 
coordinates R.A.: 09 15 14.41, Dec: +62:31:55.5 (J2000.0) with H = 13.94.

Based on the optical GTC image, at this moment we cannot rule out that 
the optical flux arises from an underlying somehow extended blue galaxy 
whereas the highly extincted afterglow is only observed in the nIR. A 
figure showing the optical & nIR images of the likely afterglow to GRB 
091202 can be found at:  http://www.iaa.es/~gss/GRB091202

This message may be quoted."