TITLE: GCN CIRCULAR NUMBER: 39997 SUBJECT: GRB 250331C: Swift-XRT refined Analysis DATE: 25/04/01 07:45:44 GMT FROM: Phil Evans at U of Leicester pae9@star.le.ac.uk
M. A. Williams (PSU), S. Dichiara (PSU), J.A. Kennea (PSU), J.P. Osborne (U. Leicester), K.L. Page (U. Leicester), A.P. Beardmore (U. Leicester), M.G. Bernardini (INAF-OAB), E. Ambrosi (INAF-IASFPA) , M. Capalbi (INAF-IASFPA) and P.A. Evans report on behalf of the Swift-XRT team:
We have analysed 3.9 ks of XRT data for GRB 250331C, from 137 s to 62.7 ks after the BAT trigger. The data comprise 95 s in Windowed Timing (WT) mode with the remainder in Photon Counting (PC) mode.
The light curve can be modelled with a power-law decay with a decay index of alpha=2.81 (+0.11, -0.10).
A spectrum formed from the WT mode data can be fitted with an absorbed power-law with a photon spectral index of 2.11 (+0.11, -0.08). The best-fitting absorption column is consistent with the Galactic value of 6.5 x 10^21 cm^-2 (Willingale et al. 2013). The PC mode spectrum has a photon index of 1.65 (+0.32, -0.30) and a best-fitting absorption column of 9.0 (+3.4, -2.5) x 10^21 cm^-2. The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor deduced from this spectrum is 5.9 x 10^-11 (8.6 x 10^-11) erg cm^-2 count^-1.
A summary of the PC-mode spectrum is thus: Total column: 9.0 (+3.4, -2.5) x 10^21 cm^-2 Galactic foreground: 6.5 x 10^21 cm^-2 Excess significance: <1.6 sigma Photon index: 1.65 (+0.32, -0.30)
If the light curve continues to decay with a power-law decay index of 2.81, the count rate at T+24 hours will be 3.2 x 10^-7 count s^-1, corresponding to an observed (unabsorbed) 0.3-10 keV flux of 1.9 x 10^-17 (2.8 x 10^-17) erg cm^-2 s^-1.
The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/01299967.
This circular is an official product of the Swift-XRT team.
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