TITLE: GCN CIRCULAR NUMBER: 23813 SUBJECT: GRB 190129B: Swift-XRT candidate afterglow detection DATE: 19/01/30 09:11:11 GMT FROM: Andrea Melandri at INAF-OAB S. J. LaPorte (PSU), J.A. Kennea (PSU), J.P. Osborne (U. Leicester), K.L. Page (U. Leicester), A.P. Beardmore (U. Leicester), P. D'Avanzo (INAF-OAB), V. D'Elia (ASDC), A. D'Ai (INAF-IASFPA), B. Sbarufatti (INAF-OAB/PSU) and P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the IPN-detected burst GRB 190129B in a series of observations tiled on the sky. The total exposure time is 6.3 ks, distributed over 14 tiles; the maximum exposure at a single sky location was 1.1 ks. The data were collected between T0+45.0 ks and T0+60.4 ks, and are entirely in Photon Counting (PC) mode. An uncatalogued X-ray source is detected and is above the RASS limit, and is therefore likely the GRB afterglow. Using 42 s of PC mode data and 1 UVOT image, we find an enhanced XRT position (using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue): RA, Dec = 117.46104, +0.93484 which is equivalent to: RA (J2000): 07h 49m 50.65s Dec(J2000): +00d 56' 05.4" with an uncertainty of 3.0 arcsec (radius, 90% confidence). This position is about 7 arcmin from the edge of the IPN 3 sigma error box (Hurley et al., GCN Circ 23808). The light curve is consistent with a constant source of mean count rate 4.4e-01 ct/sec. A power-law fit gives an index of 1.2 (+1.6, -2.1). A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 1.8 (+/-0.4). The best-fitting absorption column is 4.7 (+2.8, -2.1) x 10^21 cm^-2, in excess of the Galactic value of 7.3 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 4.4 x 10^-11 (6.3 x 10^-11) erg cm^-2 count^-1. A summary of the PC-mode spectrum is thus: Total column: 4.7 (+2.8, -2.1) x 10^21 cm^-2 Galactic foreground: 7.3 x 10^20 cm^-2 Excess significance: 3.1 sigma Photon index: 1.8 (+/-0.4) The results of the XRT-team automatic analysis of the likely afterglow are at http://www.swift.ac.uk/xrt_products/TILED_GRB00076/Source1.php. The results of the full analysis of the tiled XRT observations are available at http://www.swift.ac.uk/xrt_products/TILED_GRB00076. This circular is an official product of the Swift-XRT team.