GCN Circular 30751

J.A. Kennea (PSU), P.A. Evans (U. Leicester), J.P. Osborne (U.
Leicester), K.L. Page (U. Leicester), P. D'Avanzo (INAF-OAB), M.G.
Bernardini (INAF-OAB), E. Ambrosi  (INAF-IASFPA) , A. Tohuvavohu (U.
Toronto), B. Sbarufatti (PSU) and S. Laha report on behalf of the
Swift-XRT team:

We have analysed 2.5 ks of XRT data for GRB 210901A (Laha et al. GCN
Circ. 30746
Not found
 
 
), from 139 s to 79.9 ks after the  BAT trigger. The data
comprise 126 s in Windowed Timing (WT) mode (the first 7 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. 30749
Not found
 
 
).

The light curve can be modelled with a series of power-law decays. The
initial decay index is alpha=2.8 (+0.3, -0.4). At T+207 s  the decay
steepens to an alpha of 5.1 (+/-0.4) before breaking again at T+517 s
to a final decay with index alpha=0.60 (+/-0.09).

A spectrum formed from the WT mode data can be fitted with an absorbed
power-law with a photon spectral index	of 2.55 (+0.14, -0.13). The
best-fitting absorption column is  2.8 (+/-0.4) x 10^21 cm^-2, in
excess of the Galactic value of 1.0 x 10^21 cm^-2 (Willingale et al.
2013). The PC mode spectrum has a photon index of 2.0 (+0.4, -0.3) and
a best-fitting absorption column of 1.7 (+1.2, -0.6) x 10^21 cm^-2. The
counts to observed (unabsorbed) 0.3-10 keV flux conversion factor
deduced from this spectrum  is 3.5 x 10^-11 (4.6 x 10^-11) erg cm^-2
count^-1. 

A summary of the PC-mode spectrum is thus:
Total column:	     1.7 (+1.2, -0.6) x 10^21 cm^-2
Galactic foreground: 1.0 x 10^21 cm^-2
Excess significance: <1.6 sigma
Photon index:	     2.0 (+0.4, -0.3)

The results of the XRT-team automatic analysis are available at
http://www.swift.ac.uk/xrt_products/01071488.

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