TITLE: GCN CIRCULAR NUMBER: 20316 SUBJECT: GRB 161220A: Swift-XRT refined Analysis DATE: 16/12/21 08:56:04 GMT FROM: Phil Evans at U of Leicester A.P. Beardmore (U. Leicester), P.A. Evans (U. Leicester), P. D'Avanzo (INAF-OAB), A. D'Ai (INAF-IASFPA), J.A. Kennea (PSU), B. Sbarufatti (INAF-OAB/PSU), D.N. Burrows (PSU), S.L. Gibson (U. Leicester) and V. D'Elia report on behalf of the Swift-XRT team: We have analysed 3.4 ks of XRT data for GRB 161220A (D'Elia et al. GCN Circ. 20302), from 60 s to 58.3 ks after the BAT trigger. The data comprise 85 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 refined XRT position is RA, Dec = 350.8479, -47.4978 which is equivalent to: RA (J2000): 23 23 23.49 Dec(J2000): -47 29 52.2 with an uncertainty of 3.6 arcsec (radius, 90% confidence). The light curve can be modelled with a series of power-law decays. The light curve initially rises, with an index alpha=-1.5 (+0.0, -2.0). At T+71.0 s it breaks to an alpha of 4.75 (+0.51, -0.29) before breaking again at T+217 s to a final decay with index alpha=0.82 (+0.13, -0.11). A spectrum formed from the WT mode data can be fitted with an absorbed power-law with a photon spectral index of 3.57 (+0.20, -0.19). The best-fitting absorption column is 3.2 (+/-0.4) x 10^21 cm^-2, in excess of the Galactic value of 1.2 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 2.1 x 10^-11 (9.9 x 10^-11) erg cm^-2 count^-1. A summary of the WT-mode spectrum is thus: Total column: 3.2 (+/-0.4) x 10^21 cm^-2 Galactic foreground: 1.2 x 10^20 cm^-2 Excess significance: 12.4 sigma Photon index: 3.57 (+0.20, -0.19) If the light curve continues to decay with a power-law decay index of 0.82, 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 5.7 x 10^-14 (2.6 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/00727610. This circular is an official product of the Swift-XRT team.