TITLE: GCN CIRCULAR NUMBER: 13361 SUBJECT: GRB 120612A: Swift-XRT refined Analysis DATE: 12/06/12 14:18:04 GMT FROM: Phil Evans at U of Leicester D.N. Burrows (PSU), O.M. Littlejohns (U. Leicester), J.P. Osborne (U. Leicester), K.L. Page (U. Leicester), V. Mangano (INAF-IASFPA), A. Melandri (INAF-OAB), B. Sbarufatti (INAF-OAB/PSU), J.A. Kennea (PSU), M.C. Stroh (PSU) and C. Pagani report on behalf of the Swift-XRT team: We have analysed 13 ks of XRT data for GRB 120612A (Pagani et al. GCN Circ. 13357), from 144 s to 30.4 ks after the BAT trigger. The data comprise 91 s in Windowed Timing (WT) mode with the remainder in Photon Counting (PC) mode. The enhanced XRT position for this burst was given by Evans et al. (GCN. Circ 13359). The light curve can be modelled with an initial power-law decay with an index of alpha=3.27 (+0.26, -0.22), followed by a break at T+485 s to an alpha of 0.90 (+0.11, -0.10). A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 2.20 (+0.23, -0.22). The best-fitting absorption column is 1.9 (+/-0.6) x 10^21 cm^-2, in excess of the Galactic value of 5.5 x 10^20 cm^-2 (Kalberla et al. 2005). The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor deduced from this spectrum is 3.5 x 10^-11 (5.5 x 10^-11) erg cm^-2 count^-1. A summary of the PC-mode spectrum is thus: Total column: 1.9 (+/-0.6) x 10^21 cm^-2 Galactic foreground: 5.5 x 10^20 cm^-2 Excess significance: 3.9 sigma Photon index: 2.20 (+0.23, -0.22) The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00524128. This circular is an official product of the Swift-XRT team.