TITLE: GCN CIRCULAR NUMBER: 20176 SUBJECT: GRB 161113A: Swift-XRT refined Analysis DATE: 16/11/15 08:12:35 GMT FROM: Paolo D'Avanzo at INAF-OAB J.P. Osborne (U. Leicester), K.L. Page (U. Leicester), A. Melandri (INAF-OAB), P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC), B. Sbarufatti (INAF-OAB/PSU), D.N. Burrows (PSU), T.G.R. Roegiers (PSU), B. Mingo (U. Leicester) report on behalf of the Swift-XRT team: We have analysed 23 ks of XRT data for GRB 161113A (D'Avanzo et al. GCN Circ. 20172), from 42 s to 74.9 ks after the BAT trigger. The data comprise 118 s in Windowed Timing (WT) mode (the first 8 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 Evans et al. (GCN Circ. 20174). The light curve can be modelled with a series of power-law decays. The initial decay index is alpha=2.52 (+0.25, -0.28). At T+109 s the decay steepens to an alpha of 6.0 (+0.5, -0.4) before breaking again at T+272 s to a final decay with index alpha=0.45 (+0.04, -0.05). A spectrum formed from the WT mode data can be fitted with an absorbed power-law with a photon spectral index of 2.82 (+/-0.09). The best-fitting absorption column is 3.63 (+0.29, -0.27) x 10^21 cm^-2, in excess of the Galactic value of 2.1 x 10^20 cm^-2 (Willingale et al. 2013). The PC mode spectrum has a photon index of 2.03 (+0.22, -0.21) and a best-fitting absorption column of 1.2 (+0.6, -0.5) x 10^21 cm^-2. The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor deduced from this spectrum is 3.3 x 10^-11 (4.1 x 10^-11) erg cm^-2 count^-1. A summary of the PC-mode spectrum is thus: Total column: 1.2 (+0.6, -0.5) x 10^21 cm^-2 Galactic foreground: 2.1 x 10^20 cm^-2 Excess significance: 3.0 sigma Photon index: 2.03 (+0.22, -0.21) The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00722063. This circular is an official product of the Swift-XRT team.