Summary of results for the astrometric reduction of the data for the night on 5 January 2017 for the Pino Torinese station (N_* = 8300). For azimuth (left column) and zenith distance (right column), we show (a–b) bi- and mono-dimensional residuals histograms (2D histograms are log-stretched); (c–d) distorsion maps from the linear projection; and (e–f) random projection error maps.