GCN Circular 13790

A.P. Beardmore (U. Leicester) and S.R. Oates (MSSL-UCL) report on
behalf of the Swift-XRT team:

We have analysed 4.7 ks of XRT data for the GBM and IPN-detected burst
GRB 120919A (Rau et al. GCN Circ. 13785
Not found
 
 
, Hurley et al.	GCN Circ.
13786
Not found
 
 
), from 133.7 ks to 157.6 ks after the IPN trigger. The data are
entirely in Photon Counting (PC) mode.	Two uncatalogued X-ray sources
are detected within the IPN error box with the following refined XRT
positions :

Source 1 :

RA, Dec = 214.83981, -45.56220 which is equivalent to:

RA (J2000): 14h 19m 21.56s
Dec(J2000): -45d 33m 43.9s

with an uncertainty of 3.1 arcsec (radius, 90% confidence). This
position is 181 arcsec from the centre of the IPN error box. The
source is detected with a 0.3-10 keV count rate of 0.0067 +/- 0.0014
count/s, which corresponds to an observed flux of 2.7e-13 erg cm^-2
s^-1 for a typical GRB-like spectrum.

Source 2 :

RA, Dec =  214.79040, -45.56518 which is equivalent to:

RA (J2000): 14h 19m 09.70s
Dec(J2000): -45d 33m 54.66s

with an uncertainty of 5.5 arcsec (radius, 90% confidence). This
position is 57 arcsec from centre of the IPN error box. The source is
detected with a 0.3-10 keV count rate of 0.0037 +/- 0.0011 count/s,
which corrsponds to an observed flux of 1.5e-13 erg cm^-2 s^-1 for a
typical GRB-like spectrum.

We cannot determine whether either of the sources are fading at the
present time.

This circular is an official product of the Swift-XRT team.