[vsnet-grb-info 15652] GRB 141022A: Swift-XRT refined Analysis
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Wed Oct 22 22:48:11 JST 2014
TITLE: GCN CIRCULAR
NUMBER: 16941
SUBJECT: GRB 141022A: Swift-XRT refined Analysis
DATE: 14/10/22 13:48:04 GMT
FROM: Phil Evans at U of Leicester <pae9 at leicester.ac.uk>
P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC), M. de Pasquale (INAF-IASFPA),
M.C. Stroh (PSU), D.N. Burrows (PSU), J.A. Kennea (PSU), A.P. Beardmore
(U. Leicester), P.A. Evans (U. Leicester), B.P. Gompertz (U. Leicester)
and A. Vargas report on behalf of the Swift-XRT team:
We have analysed 10 ks of XRT data for GRB 141022A (Vargas et al. GCN
Circ. 16938), from 144 s to 25.5 ks after the BAT trigger. The data
are entirely in Photon Counting (PC) mode. The best available XRT
position (using the promptly downlinked event data, the XRT-UVOT
alignment and matching UVOT field sources to the USNO-B1 catalogue) is
RA, Dec = 241.8696, -72.1254 which is equivalent to:
RA (J2000): 16 07 28.70
Dec(J2000): -72 07 31.4
with an uncertainty of 2.1 arcsec (radius, 90% confidence).
The light curve can be modelled with a power-law decay with a decay
index of alpha=1.21 (+/-0.08).
A spectrum formed from the PC mode data can be fitted with an absorbed
power-law with a photon spectral index of 2.5 (+0.5, -0.4). The
best-fitting absorption column is 1.1 (+0.5, -0.4) x 10^22 cm^-2, in
excess of the Galactic value of 1.0 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 3.9 x 10^-11 (1.2 x 10^-10) erg
cm^-2 count^-1.
A summary of the PC-mode spectrum is thus:
Total column: 1.1 (+0.5, -0.4) x 10^22 cm^-2
Galactic foreground: 1.0 x 10^21 cm^-2
Excess significance: 4.5 sigma
Photon index: 2.5 (+0.5, -0.4)
If the light curve continues to decay with a power-law decay index of
1.21, the count rate at T+24 hours will be 2.7 x 10^-4 count s^-1,
corresponding to an observed (unabsorbed) 0.3-10 keV flux of 1.0 x
10^-14 (3.3 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/00616061.
This circular is an official product of the Swift-XRT team.
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