GCN Circular 4525

K.L. Page, M.R. Goad, A.P. Beardmore (U. Leicester), D.N. Burrows (PSU),
A. Smale (NASA HQ) and L.  Cominsky (Sonoma State U.) report on behalf of
the Swift-XRT Team:

Swift performed a Target of Opportunity observation of GRB 060110 once it 
came out of the Moon constraint, approximately 2.4e5 seconds (2.8 days) 
after the BAT trigger (Zane et al., GCN 4463
Not found
 
 
).

A faint, fading, uncatalogued X-ray source was identified at a position 
of:

RA(J2000)  =  04h 50m 57.85s
Dec(J2000) = +28d 25' 53.88"

with an uncertainty of 4.1 arcsec (90% containment, including the latest
XRT boresight correction). This is 0.7" from the position given by Torii
in GCN 4468
Not found
 
 
 for a potential, low signal-to-noise source and 6.9"  from the
IR position in GCN 4467
Not found
 
 
 (Bloom & Li). The XRT position is also 21 arcsec
from the refined BAT position (Parsons et al., GCN 4477
Not found
 
 
)

Using 41.7 ks of data, the source is fading with a decay slope of alpha =
2.0 +/- 1.2. The spectrum can be modelled with a power-law of Gamma = 2.27
+/- 0.58, with absorption consistent with the Galactic value in this
direction (2.4e21 cm^-2). The time averaged 0.3-10 keV observed
(unabsorbed) flux between 2.4e5 and 4.8e5 seconds is 6.45e-14 (1.13e-13)
erg cm^-2 s^-1.