TITLE: GCN CIRCULAR NUMBER: 7014 SUBJECT: GRB 071028: Swift-XRT Team refined analysis DATE: 07/10/28 23:13:12 GMT FROM: Judith Racusin at PSU J. Racusin (PSU) reports on behalf of the Swift-XRT Team: We have analysed the first 2 orbits of Swift-XRT data obtained for GRB 071028 (Racusin et al. GCN Circ. 7012), totaling 61 s of Windowed Timing (WT) data and 2.9 ks of Photon Counting (PC) data. Using 399 s of overlapping XRT Photon Counting mode and UVOT V-band data, we find an astrometrically corrected X-ray position (using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue): RA, Dec = 119.81936, 21.48482 which is equivalent to: RA (J2000): 07 59 16.65 Dec (J2000): +21 29 05.4 with an uncertainty of 1.9 arcsec (radius, 90% confidence). This is 6.5 arcsec from the previous XRT position (GCN Circ. 7012), and 51 arcsec from the refined BAT position (Cummings et al., GCN Circ. 7013). The bright X-ray light-curve can be fit by a broken power-law, with an initial steep decay index of 3.3 +/- 0.4 followed by a flatter decay index of 1.1 +/- 0.3 after a break at 475 +/- 150 seconds. The WT data (124-182 seconds) can be modeled as an absorbed power-law, with photon index of 1.9 +/- 0.2 and a total absorbing column of NH = (5.9 +/- 5.6)e20 cm^-2, consistent with the Galactic value of 5.1e20 cm^-2. The 0.3-10 keV observed (unabsorbed) flux during this time is 3.1e-10 (3.6e-10) erg cm^-2 s^-1. Assuming the source continues to decay with the same decay index of 1.1, we predict an XRT count rate of 5.5e-4 counts/s at T+24 hours, which corresponds to an 0.3-10.0 keV observed flux of 2.3e-14 ergs cm^-2 s^-1. This circular is an official product of the Swift-XRT team.