GCN Circular 13583
Subject
GRB 120803B: Swift-XRT refined Analysis
Event
Date
2012-08-04T23:08:34Z (13 years ago)
From
Claudio Pagani at U of Leicester <cp232@star.le.ac.uk>
C. Pagani (U. Leicester) and J. L. Racusin (NASA/GSFC) report on behalf
of the Swift-XRT team:
We have analysed 4.4 ks of XRT data for GRB 120803B (Racusin et al.
GCN Circ. 13566), from 79 s to 17.5 ks after the BAT trigger. The data
comprise 31 s in Windowed Timing (WT) mode with the remainder in Photon
Counting (PC) mode. The enhanced XRT position for this burst was given
by Goad et al. (GCN. Circ 13571).
The light curve can be modelled with a power-law decay with a decay
index of alpha=1.25 (+0.07, -0.06).
A spectrum formed from the PC mode data can be fitted with an absorbed
power-law with a photon spectral index of 1.2 (+/-0.4). The
best-fitting absorption column is 8.5 (+4.7, -2.8) x 10^21 cm^-2,
consistent with the Galactic value of 5.7 x 10^21 cm^-2 (Kalberla et
al. 2005). The counts to observed (unabsorbed) 0.3-10 keV flux
conversion factor deduced from this spectrum is 8.4 x 10^-11 (1.1 x
10^-10) erg cm^-2 count^-1.
A summary of the PC-mode spectrum is thus:
Total column: 8.5 (+4.7, -2.8) x 10^21 cm^-2
Galactic foreground: 5.7 x 10^21 cm^-2
Excess significance: <1.6 sigma
Photon index: 1.2 (+/-0.4)
The results of the XRT-team automatic analysis are available at
http://www.swift.ac.uk/xrt_products/00529606.
This circular is an official product of the Swift-XRT team.