GCN Circular 7208
Subject
GRB 080123: Swift-XRT refined analysis
Event
Date
2008-01-23T17:24:42Z (18 years ago)
From
Boris Sbarufatti at INAF-IASF-Pa <sbarufatti@ifc.inaf.it>
V. Mangano, B. Sbarufatti (INAF-IASF PA), T. N. Ukwatta (GSFC/GWU),
and D. N. Burrows (PSU) report on behalf of the Swift XRT team:
We have analyzed the XRT data collected during the first three
orbits of observation of GRB 080123 (Ukwatta et al., GCN Circ. 7203).
We have 124 s of exposure in WT mode (from T+108 to T+224 s)
and 7.1 ks in PC mode.
The initial XRT on-board position was centered on a cosmic ray hit.
This position was retracted. The XRT position reported in GCN Circ.
7203 was obtained from the first downlinked data, but we note that the
error circle given in this circular erroneously ignored the systematic
component and was therefore much too small. The new, refined position
of the XRT afterglow is
22h 35m 46.6s, -64d 54' 03.8" (J2000)
with an error circle radius of 3.9" (90% confidence).
As reported by Osborne et al. (GCN Circ. 7204