GCN Circular 15963
Subject
GRB 140311B: Swift-XRT refined Analysis
Event
Date
2014-03-12T13:20:17Z (12 years ago)
From
Valerio D'Elia at ASDC <delia@asdc.asi.it>
V. D'Elia (ASDC), L. Izzo (URoma/ICRA) and J. L. Racusin (NASA/GSFC)
report on behalf of the Swift-XRT team:
We have analysed 7.8 ks of XRT data for GRB 140311B (Racusin et al.
GCN Circ. 15945), from 3.4 ks to 46.3 ks after the BAT trigger. The
data are entirely in Photon Counting (PC) mode. The enhanced XRT
position for this burst was given by Evans et al. (GCN Circ. 15958).
The light curve can be modelled with a power-law decay with a decay
index of alpha=1.66 (+0.18, -0.15).
A spectrum formed from the PC mode data can be fitted with an absorbed
power-law with a photon spectral index of 1.68 (+0.25, -0.23). The
best-fitting absorption column is 1.6 (+0.9, -0.8) x 10^21 cm^-2, in
excess of the Galactic value of 3.6 x 10^20 cm^-2 (Kalberla et al.
2005). The counts to observed (unabsorbed) 0.3-10 keV flux conversion
factor deduced from this spectrum is 4.1 x 10^-11 (4.9 x 10^-11) erg
cm^-2 count^-1.
A summary of the PC-mode spectrum is thus:
Total column: 1.6 (+0.9, -0.8) x 10^21 cm^-2
Galactic foreground: 3.6 x 10^20 cm^-2
Excess significance: 2.7 sigma
Photon index: 1.68 (+0.25, -0.23)
If the light curve continues to decay with a power-law decay index of
1.66, the count rate at T+24 hours will be 9.6 x 10^-4 count s^-1,
corresponding to an observed (unabsorbed) 0.3-10 keV flux of 4.0 x
10^-14 (4.8 x 10^-14) erg cm^-2 s^-1.
The results of the XRT-team automatic analysis are available at
http://www.swift.ac.uk/xrt_products/00591392.
This circular is an official product of the Swift-XRT team.