V. D'Elia (SSDC & INAF-OAR), A. D'Ai (INAF-IASFPA), D.N. Burrows (PSU),
J. D. Gropp (PSU), J.A. Kennea (PSU), K.L. Page (U. Leicester), A.P.
Beardmore (U. Leicester), P.A. Evans (U. Leicester), A. Melandri
(INAF-OAB) and M.G. Bernardini report on behalf of the Swift-XRT team:
We have analysed 4.9 ks of XRT data for GRB 210725B (Bernardini et al.
GCN Circ. 30508), from 94 s to 107.1 ks after the BAT trigger. The
data comprise 68 s in Windowed Timing (WT) mode with the remainder in
Photon Counting (PC) mode. The enhanced XRT position for this burst was
given by Goad et al. (GCN Circ. 30510).
The light curve can be modelled with a power-law decay with a decay
index of alpha=3.43 (+0.20, -0.18).
A spectrum formed from the WT mode data can be fitted with an absorbed
power-law with a photon spectral index of 1.77 (+0.29, -0.27). The
best-fitting absorption column is 6.6 (+2.7, -2.1) x 10^21 cm^-2, in
excess of the Galactic value of 2.0 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 4.5 x 10^-11 (6.7 x 10^-11) erg
A summary of the WT-mode spectrum is thus:
Total column: 6.6 (+2.7, -2.1) x 10^21 cm^-2
Galactic foreground: 2.0 x 10^20 cm^-2
Excess significance: 5.2 sigma
Photon index: 1.77 (+0.29, -0.27)
The results of the XRT-team automatic analysis are available at
This circular is an official product of the Swift-XRT team.