GCN Circular 2508
Subject
XMM-Newton observation of GRB040106
Date
2004-01-07T10:27:31Z (20 years ago)
From
Norbert Schartel at XMM-Newton/ESA <nscharte@xmm.vilspa.esa.es>
M. Ehle, R. Gonzalez-Riestra and B. Gonzalez-Garcia, from the
XMM-Newton SOC report:
Quick-Look-Analysis of the first 30 ksec of the XMM-Newton
observation of the GRB040106 field (Mereghetti et al.,
GCN 2505) shows the presence of a bright source in the
EPIC-pn and MOS cameras within the INTEGRAL error circle,
XMMU J115213.1-464713:
R.A. (J2000) = 11h 52m 13.1s
Dec. (J2000) = -46deg 47' 13"
The EPIC-pn count rate decreased from 0.7 to 0.2 counts/sec
during the first 30 ksec of the observation.
At this stage of reduction the position error is expected
to be less than 10 arcsec.