[vsnet-grb-info 28089] GRB 210610A: Swift-XRT refined Analysis

[GCN Circulars]

TITLE:   GCN CIRCULAR
NUMBER:  30192
SUBJECT: GRB 210610A: Swift-XRT refined Analysis
DATE:    21/06/11 06:21:16 GMT
FROM:    Phil Evans at U of Leicester  <pae9 at leicester.ac.uk>

D.N. Burrows (PSU), J. D. Gropp (PSU), A.P. Beardmore (U. Leicester),
P.A. Evans (U. Leicester), J.P. Osborne (U. Leicester), T. Sbarrato
(INAF-OAB), P. D'Avanzo (INAF-OAB), M.G. Bernardini (INAF-OAB), J.A.
Kennea (PSU) and K.L. Page report on behalf of the Swift-XRT team:

We have analysed 7.1 ks of XRT data for GRB 210610A (Page et al. GCN
Circ. 30160), from 97 s to 45.9 ks after the  BAT trigger. The data are
entirely in Photon Counting (PC) mode. The enhanced XRT position for
this burst was given by Goad et al. (GCN Circ. 30165).

The late-time light curve (from T0+4.1 ks) can be modelled with a
power-law decay with a decay index of alpha=1.05 (+/-0.10).

A spectrum formed from the PC mode data can be fitted with an absorbed
power-law with a photon spectral index of 1.84 (+0.12, -0.10). The
best-fitting absorption column is  2.6 (+9.0, -2.6) x 10^21 cm^-2, at a
redshift of 3.54, in addition to the Galactic value of 2.2 x 10^20
cm^-2 (Willingale et al. 2013). The counts to observed (unabsorbed)
0.3-10 keV flux conversion factor deduced from this spectrum  is 3.5 x
10^-11 (3.7 x 10^-11) erg cm^-2 count^-1. 

A summary of the PC-mode spectrum is thus:
Galactic foreground: 2.2 x 10^20 cm^-2
Intrinsic column:    2.6 (+9.0, -2.6) x 10^21 cm^-2 at z=3.54
Photon index:	     1.84 (+0.12, -0.10)

If the light curve continues to decay with a power-law decay index of
1.05, the count rate at T+24 hours will be 9.7 x 10^-3 count s^-1,
corresponding to an observed (unabsorbed) 0.3-10 keV flux of 3.4 x
10^-13 (3.6 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/01054627.

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