TITLE: GCN CIRCULAR NUMBER: 35421 SUBJECT: GRB 231222B: Swift-XRT afterglow detection DATE: 23/12/23 12:50:08 GMT FROM: Phil Evans at U of Leicester <pae9@star.le.ac.uk> M. Ferro (INAF-OAB), J.A. Kennea (PSU), A. Tohuvavohu (U. Toronto), D.N. Burrows (PSU), J.P. Osborne (U. Leicester), K.L. Page (U. Leicester), A.P. Beardmore (U. Leicester), R. Brivio (INAF-OAB), A. D'Ai (INAF-IASFPA) and P.A. Evans (U. Leicester) reports on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Fermi/LAT-detected burst GRB 231222B in a series of observations tiled on the sky. We point out that the burst was improperly named GRB 231222A in GCN Circ 35415, where the tiling was announced. The total exposure time is 4.1 ks, distributed over 4 tiles; the maximum exposure at a single sky location was 2.3 ks. The data were collected between T0+43.2 ks and T0+54.8 ks, and are entirely in Photon Counting (PC) mode. Three uncatalogued X-ray sources are detected, of which one ("Source 1") is believed to be the afterglow. Using 1211 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 = 251.24744, +19.62084 which is equivalent to: RA (J2000): 16h 44m 59.39s Dec(J2000): +19d 37' 15.0" with an uncertainty of 3.3 arcsec (radius, 90% confidence). This position is 9.3 arcmin from the Fermi/LAT position. The source has a mean count rate of 6.0e-02 ct/sec; we cannot determine at the present time whether it is fading. A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 1.65 (+0.49, -0.29). The best-fitting absorption column is consistent with the Galactic value of 7.1 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 3.4 x 10^-11 (3.8 x 10^-11) erg cm^-2 count^-1. A summary of the PC-mode spectrum is thus: Total column: 7 (+/-14) x 10^20 cm^-2 Galactic foreground: 7.1 x 10^20 cm^-2 Excess significance: <1.6 sigma Photon index: 1.65 (+0.49, -0.29) The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00021639. The results of the full analysis of the tiled XRT observations are available at https://www.swift.ac.uk/xrt_products/TILED_GRB00118. This circular is an official product of the Swift-XRT team. View this GCN Circular online at https://gcn.nasa.gov/circulars/35421. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...