GCN Circular 26346
B. Sbarufatti (PSU) ), J. D. Gropp (PSU) and P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Swift/BAT-detected burst GRB 191130A (Palmer et al. GCN Circ. 26327), collecting 5.0 ks of Photon Counting (PC) mode data between T0+310.0 ks and T0+343.5 ks. Three uncatalogued sources were detected, all of them too far from the GRB position to be likely afterglow candidates. The 3-sigma upper limit at the BAT position is 1.19e-3 ct s^-1, corresponding to a 0.3-10 keV observed flux of 6.0e-14 erg cm^-2 s^-1 (assuming a typical GRB spectrum). The results of the XRT-team automatic analysis of the XRT observations, including a position-specific upper limit calculator, are available at https://www.swift.ac.uk/ToO_GRBs/00020950. This circular is an official product of the Swift-XRT team.