GCN Circular 17557

J.A. Kennea (PSU), B. Sbarufatti (INAF-OAB/PSU), K.L. Page (U.
Leicester), C. Pagani (U. Leicester), A.P. Beardmore (U. Leicester), P.
D'Avanzo (INAF-OAB), V. D'Elia (ASDC), M. de Pasquale (INAF-IASFPA),
D.N. Burrows (PSU) and J.R. Cummings report on behalf of the Swift-XRT
team:

We have analysed 6.9 ks of XRT data for GRB 150309A (Cummings et al.
GCN Circ. 17553
Not found
 
 
), from 122 s to 17.9 ks after the  BAT trigger. The
data comprise 273 s in Windowed Timing (WT) mode (the first 8 s were
taken while Swift was slewing) with the remainder in Photon Counting
(PC) mode. The enhanced XRT position for this burst was given by
Osborne et al. (GCN Circ. 17555
Not found
 
 
).

The light curve can be modelled with an initial power-law decay with an
index of alpha=2.11 (+0.09, -0.07), followed by a break at T+477 s to
an alpha of 0.98 (+/-0.04).

A spectrum formed from the WT mode data can be fitted with an absorbed
power-law with a photon spectral index	of 1.82 (+/-0.07). The
best-fitting absorption column is  2.03 (+0.28, -0.27) x 10^21 cm^-2,
in excess of the Galactic value of 9.1 x 10^20 cm^-2 (Willingale et al.
2013). The PC mode spectrum has a photon index of 1.91 (+0.12, -0.11)
and a best-fitting absorption column of 2.8 (+/-0.5) x 10^21 cm^-2. The
counts to observed (unabsorbed) 0.3-10 keV flux conversion factor
deduced from this spectrum  is 3.9 x 10^-11 (5.4 x 10^-11) erg cm^-2
count^-1. 

A summary of the PC-mode spectrum is thus:
Total column:	     2.8 (+/-0.5) x 10^21 cm^-2
Galactic foreground: 9.1 x 10^20 cm^-2
Excess significance: 6.6 sigma
Photon index:	     1.91 (+0.12, -0.11)

If the light curve continues to decay with a power-law decay index of
0.98, the count rate at T+24 hours will be 0.022 count s^-1,
corresponding to an observed (unabsorbed) 0.3-10 keV flux of 8.4 x
10^-13 (1.2 x 10^-12) erg cm^-2 s^-1.

The results of the XRT-team automatic analysis are available at
http://www.swift.ac.uk/xrt_products/00634200.

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