GCN Circular 5849
Subject
GRB 061122: Candidate Optical Afterglow
Date
2006-11-24T05:00:33Z (18 years ago)
From
Jules Halpern at Columbia U. <jules@astro.columbia.edu>
J. P. Halpern & E. Armstrong (Columbia U.) report on behalf of the
MDM Observatory GRB follow-up team:
"We obtained R-band observations of the field of INTEGRAL GRB 061122
(Mereghetti et al., GCN 5834) on two consecutive nights using the
MDM 2.4m telescope. Within 1" of the Swift XRT candidate X-ray
afterglow (Beardmore et al., GCN 5842), we find a fading object at
(J2000) R.A.=20h15m19.84s, Decl.=+15d31'02.5"
with positional uncertainty ~0.5", and the following magnitudes:
------------------------------------------------
Date(UT) Mid-time(UT) t-t0(hr) R(mag) +/-
------------------------------------------------
Nov. 23 01:52 17.9 22.61 0.05
Nov. 24 02:26 42.5 23.41 0.15
------------------------------------------------
We propose this as the optical afterglow of GRB 061122.
Magnitudes are referenced to the USNO B1.0 star at
(J2000) R.A.=20h15m18.48s, Decl.= +15d31'05.5" with R=17.61,
and are not corrected for Galactic extinction, A_R=0.49 mag
in this direction (Schlegel et al. 1998).
MDM images of the field are posted at
http://www.astro.columbia.edu/~jules/grb/061122/
This message may be cited."