GCN Circular 6003
Subject
GRB070107: Swift/XRT refined analysis
Event
Date
2007-01-08T22:12:04Z (19 years ago)
From
Teresa Mineo at INAF-IASFA <teresa.mineo@ifc.inaf.it>
T. Mineo, B. Sbarufatti, V. Mangano, G. Cusumano (INAF-IASF Pa)
report on behalf of the Swift XRT team:
We have analyzed the first ten orbits of Swift-XRT data on GRB 070107
(Stamatikos et al. GCN 5999), with a total exposure of 420 s seconds
in Window Timing (WT) mode and 15.8 ks seconds in Photon Counting (PC)
mode.
This provides a refined XRT position at RA,Dec=159.4016,-53.2131
which is:
RA (J2000) = 10h 37m 36.4s
Dec(J2000) = -53d 12m 47.3s
with an estimated error radius of 3.7 arcseconds (90% confidence). This
position is 59.4 arcseconds from the BAT refined position (Barthelmy et
al. GCN 6001), 2.6 arcseconds from the initial XRT position
(Kennea & Stamatikos, GCN 6000), and 0.4 arcseconds from the UVOT
optical candidate (Boyd et al., GCN 6002