GCN Circular 1924

Kristian Pedersen (U. of Copenhagen), Johan Fynbo (U. of Aarhus),
Jens Hjorth (U. of Copenhagen), Darach Watson (U. of Copenhagen)
report on behalf of the GRACE collaboration:

"Chandra X-ray Observatory observed the field of the GRB 030226 
(Suzuki et al., GCN 1888
Not found
 
 
) with the ACIS-S3 detector for a total of 
11.9 hours, starting Feb 27, 16:49 UT, 37.1 hours after the GRB trigger. 
Based on a preliminary analysis we identify a previously unknown, fading 
X-ray source at the position

RA (J2000.0) = 11 33 04.93, Dec (J2000.0) =  +25 53 55.3

consistent with the position of the optical transient (Price et al.,
GCN 1880
Not found
 
 
). The positional accuracy is better than one arcsec. Hence 
we identify the source as the X-ray afterglow of GRB 030226.

The 0.3-10 keV count rate averaged over the observation is 9.7e-03 counts/s, 
and the average 2-10 keV flux is 3.2e-14 erg/cm^2/s. The spectrum is well 
fitted by an absorbed power law with spectral index 1.0 +/-0.2, absorption 
fixed at the Galactic value (1.6e20 cm^2), and an absorbing column density 
of 1e22 +/- 0.5e22 cm^-2 at a redshift of 1.98. A power law with Galactic
absorption only is not an acceptable fit to the soft part of the Chandra 
spectrum. No other obvious spectral features are detected.

We thank Harvey Tananbaum for rapidly approving Director's Discretionary
Time for this observation, and the staff at the Chandra Science Center
for smoothly implementing and processing the observation."