TITLE: GCN CIRCULAR NUMBER: 22376 SUBJECT: GRB 180204A: Swift-XRT refined Analysis DATE: 18/02/04 10:26:23 GMT FROM: Phil Evans at U of Leicester J.P. Osborne (U. Leicester), A.P. Beardmore (U. Leicester), A. Melandri (INAF-OAB), P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC), D.N. Burrows (PSU), A. Tohuvavohu (PSU), S. J. LaPorte (PSU) and K.L. Page report on behalf of the Swift-XRT team: We have analysed 8.0 ks of XRT data for GRB 180204A (Page et al. GCN Circ. 22375), from 90 s to 21.2 ks after the BAT trigger. The data comprise 32 s in Windowed Timing (WT) mode with the remainder 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 = 330.1333, 30.8381 which is equivalent to: RA (J2000): 22 00 32.00 Dec(J2000): +30 50 17.1 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=1.15 (+/-0.03). A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 2.02 (+0.23, -0.22). The best-fitting absorption column is 6.9 (+1.7, -1.5) x 10^21 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 4.3 x 10^-11 (7.6 x 10^-11) erg cm^-2 count^-1. A summary of the PC-mode spectrum is thus: Total column: 6.9 (+1.7, -1.5) x 10^21 cm^-2 Galactic foreground: 1.0 x 10^21 cm^-2 Excess significance: 6.5 sigma Photon index: 2.02 (+0.23, -0.22) If the light curve continues to decay with a power-law decay index of 1.15, the count rate at T+24 hours will be 2.7 x 10^-3 count s^-1, corresponding to an observed (unabsorbed) 0.3-10 keV flux of 1.2 x 10^-13 (2.0 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/00808483. This circular is an official product of the Swift-XRT team.