[vsnet-grb-info 16828] GRB 150801B: Swift-XRT refined Analysis

[GCN Circulars]

TITLE:   GCN CIRCULAR
NUMBER:  18109
SUBJECT: GRB 150801B: Swift-XRT refined Analysis
DATE:    15/08/02 18:14:27 GMT
FROM:    Boris Sbarufatti at INAF-OAB/IASFPA  <boris.sbarufatti at brera.inaf.it>

P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC), T.G.R. Roegiers (PSU), L.M.
McCauley (PSU), J.A. Kennea (PSU), B.P. Gompertz (U. Leicester), J.P.
Osborne (U. Leicester), A. D'ai (INAF-IASFPA) and B. Sbarufatti
(INAF-OAB/PSU) report on behalf of the Swift-XRT team:

We have analysed 12 ks of XRT data for GRB 150801B (Sbarufatti et al.
GCN Circ. 18104), from 64 s to 40.0 ks after the BAT trigger. We have
analysed 12 ks of XRT data for GRB 150801B (Sbarufatti et al. GCN Circ.
18104), from 64 s to 40.0 ks after the	BAT trigger. The data comprise
8 s in Windowed Timing (WT) mode while Swift was slewing to the burst,
270 s in PC mode, a further 185 s in WT mode during a bright flare
starting at T0+366 s (also seen in the BAT), with the remainder 11.5 ks
in Photon Counting (PC) mode. The enhanced XRT position for this burst
was given by Evans et al. (GCN Circ. 18108).

The late-time light curve (from T0+4.9 ks) can be modelled with a
power-law decay with a decay index of alpha=1.74 (+0.18, -0.17).

A spectrum formed from the PC mode data can be fitted with an absorbed
power-law with a photon spectral index of 1.79 (+0.21, -0.19). The
best-fitting absorption column is  3.0 (+/-0.4) x 10^22 cm^-2, in
excess of the Galactic value of 2.7 x 10^21 cm^-2 (Willingale et al.
2013). The counts to observed (unabsorbed) 0.3-10 keV flux conversion
factor deduced from this spectrum  is 7.6 x 10^-11 (1.5 x 10^-10) erg
cm^-2 count^-1. 

A summary of the PC-mode spectrum is thus:
Total column:	     3.0 (+/-0.4) x 10^22 cm^-2
Galactic foreground: 2.7 x 10^21 cm^-2
Excess significance: 10.8 sigma
Photon index:	     1.79 (+0.21, -0.19)

If the light curve continues to decay with a power-law decay index of
1.74, the count rate at T+24 hours will be 1.4 x 10^-3 count s^-1,
corresponding to an observed (unabsorbed) 0.3-10 keV flux of 1.1 x
10^-13 (2.2 x 10^-13) erg cm^-2 s^-1.

The results of the XRT-team automatic analysis are available at
http://www.swift.ac.uk/xrt_products/00650977.

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