[vsnet-grb-info 15536] GRB 140916A: Swift-XRT refined Analysis
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Wed Sep 17 08:00:20 JST 2014
TITLE: GCN CIRCULAR
NUMBER: 16825
SUBJECT: GRB 140916A: Swift-XRT refined Analysis
DATE: 14/09/16 22:58:06 GMT
FROM: Phil Evans at U of Leicester <pae9 at leicester.ac.uk>
B. Sbarufatti (INAF-OAB/PSU), D.N. Burrows (PSU), J.A. Kennea (PSU), V.
Mangano (PSU), C. Pagani (U. Leicester), A.P. Beardmore (U. Leicester),
P.A. Evans (U. Leicester), P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC) and
J.L. Racusin report on behalf of the Swift-XRT team:
We have analysed 13 ks of XRT data for GRB 140916A (Racusin et al. GCN
Circ. 16819), from 141 s to 30.7 ks after the BAT trigger. The data
comprise 218 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. 16820). The late-time light curve (from T0+5.3 ks) is
consistent with a constant source of mean count rate 5.4e-01 ct/sec. A
power-law fit gives an index of -0.04 (+/-0.08).
A spectrum formed from the WT mode data can be fitted with an absorbed
power-law with a photon spectral index of 2.70 (+/-0.11). The
best-fitting absorption column is 1.51 (+0.24, -0.23) x 10^21 cm^-2,
in excess of the Galactic value of 1.7 x 10^20 cm^-2 (Willingale et al.
2013). The PC mode spectrum has a photon index of 2.05 (+/-0.09) and a
best-fitting absorption column of 1.34 (+0.26, -0.25) x 10^21 cm^-2.
The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor
deduced from this spectrum is 3.3 x 10^-11 (4.3 x 10^-11) erg cm^-2
count^-1.
A summary of the PC-mode spectrum is thus:
Total column: 1.34 (+0.26, -0.25) x 10^21 cm^-2
Galactic foreground: 1.7 x 10^20 cm^-2
Excess significance: 7.8 sigma
Photon index: 2.05 (+/-0.09)
If the light curve continues to decay with a power-law decay index of
-0.04, the count rate at T+24 hours will be 0.23 count s^-1,
corresponding to an observed (unabsorbed) 0.3-10 keV flux of 7.6 x
10^-12 (9.9 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/00612804.
This circular is an official product of the Swift-XRT team.
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