Notes. The columns are as follows: Colums 1–6: HRS (Boselli et al. 2010), CGCG (Zwicky et al. 1961), VCC (Binggeli et al. 1985), UGC (Nilson 1973), NGC (Dreyer 1888) and IC (Dreyer 1895) names. Columns 7–8: the J.2000 right ascension and declination. Column 9: morphological type:  −2 = dE/dS0, 0 = E-E/S0, 1 = S0, 2 = S0a-S0/Sa, 3 = Sa, 4 = Sab, 5 = Sb, 6 = Sbc, 7 = Sc, 8 = Scd, 9 = Sd, 10 = Sdm-Sd/Sm, 11 = Sm, 12 = Im, 13 = Pec, 14 = S/BCD, 15 = Sm/BCD, 16 = Im/BCD, 17 = BCD. Column 10: optical diameter (D₂₅) in arcminutes as given in Boselli et al. (2010). Note that for HRS295 we adopted the RC3 value instead of that given by Boselli et al. (2010), since it is much more representative of the “real” optical extent of the galaxy. Column 11: E(B − V) based on the maps of Schlegel et al. (1998). Column 12: distance in Mpc. As discussed in Boselli et al. (2010), we fixed the distances for galaxies belonging to the Virgo cluster (i.e., 23 Mpc for the Virgo B cloud and 17 Mpc for all the other clouds; Gavazzi et al. 1999), while for the rest of the sample distances have been estimated from their recessional velocities assuming a Hubble constant H₀ = 70 km s^-1 Mpc^-1. Columns 13–14: name of the NUV tile and exposure time in seconds. Columns 15–16: name of the FUV tile and exposure time in seconds. Column 17: note indicating whether a galaxy has been excluded because GALEX observations were not possible due to bright stars (S), the target was too close to the edge of the field (E), the frame was too shallow to be used for reliable photometry (F) or simply the galaxy was not observed (N).