GCN Circular 656

A. Henden (USRA/USNO) reports on behalf of the USNO GRB team:

We have acquired preliminary UBVRcIc all-sky photometry for
the field of GRB000418 with the USNOFS 1.0-m telescope on one
marginally photometric night.  This 11x11arcmin field includes
the proposed counterpart and extends a little fainter than V=20.
All stars brighter than V=14 are saturated and should be used
with care.  We have placed the photometric data on our
anonymous ftp site:
ftp://ftp.nofs.navy.mil/pub/outgoing/aah/grb/grb000418.dat
The current photometry has a potential external zero-point
error of about three percent.  The astrometry in this file
is based on linear plate solutions with respect to USNO-A2.0.
The internal errors are less than 100mas.

We suggest the use of five comparison stars in the field
until further photometry is obtained:

ID   x    y     U       B       V       R       I
A   000  000  16.726  16.682  16.037  15.686  15.313
               0.009   0.004   0.002   0.003   0.004

B  -158 +050  19.695  18.530  17.480  16.834  16.329
               0.110   0.013   0.007   0.009   0.012

C  -060 +134  18.899  19.172  18.302  17.874  17.369
               0.063   0.024   0.014   0.021   0.029

D  -094 -006    -     20.489  19.663  19.168  18.046
                       0.091   0.046   0.065   0.150

E  -200 -042    -     19.874  18.982  18.549  18.046
                       0.044   0.025   0.036   0.050

Notes: star A is the Mirabal et. al. comparison star
located at RA 12:25:25.65, DEC +20:04:57.4 J2000;
x,y offsets are in arcsec with respect to this star,
positive east and north.