TITLE: GCN CIRCULAR NUMBER: 8854 SUBJECT: GRB 090126A: Swift-XRT Refined Analysis DATE: 09/01/27 01:23:41 GMT FROM: Michael Stroh at PSU/Swift M. C. Stroh (PSU) reports on behalf of the Swift-XRT team: We have analyzed the first 3.1 ks of XRT data for GRB 090126A (Evangelista et al., GCN Circ. 8852), from T+48 ks to T+60 ks after the trigger. The data is all taken in Photon Counting (PC) mode. Using 1435 s of XRT Photon Counting mode data and 2 UVOT images, we find an astrometrically corrected X-ray position (using the XRT-UVOT alignment and matching to the USNO-B1 catalogue): RA, Dec = 3.6577, 81.3733 which is equivalent to: RA (J2000): 00 14 37.85 Dec (J2000): +81 22 24.0 with an uncertainty of 2.2 arcsec (90% confidence). This position may be improved as more data are received. The latest position can be viewed at http://www.swift.ac.uk/xrt_positions. Position enhancement is described by Goad et al. (2007, A&A, 476, 1401 http://www.swift.ac.uk/xrt_positions/Goad.pdf) , the current algorithm is an extension of this method. A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 1.8 (+0.6, -0.4). The best- fitting absorption column is 1.8 (+/- 1.8) x 10^21 cm^-2, which is consistent with the Galactic value of 1.4 x 10^21 cm^-2 (Kalberla et al. 2005). The observed (unabsorbed) flux in the 0.3-10.0 keV band is 1.49 (1.9) x 10^-12 erg cm^-2 s^-1. The light curve shows a potentially decaying source which can be fit using a single power-law decay with a slope, alpha = 1.2 (+/- 1.1). Assuming the light curve decays at the current rate, we predict count rates at T+24 and T+48 hours to be 1.6 x 10^-2 and 7.0 x 10^-3 respectively. This is an official product of the Swift-XRT team.