Notes. Data are from Walter et al. (2008) and Leroy et al. (2008) unless otherwise noted. Columns: (1) galaxy name; (2) inclination angle; (3) optical diameter measured at the 25 mag arcsec⁻² isophote in B-band; (4) distance; (5) absolute B-band magnitude; (6) galaxy morphological classification; (7) optical classification of the nuclear spectrum, from Ho et al. (1997) where Sy = Seyfert and T = transition object between HII nuclei and LINERs; (8) SFR based on the hybrid FUV+24 μm conversion that has an uncertainty of 0.3 dex; (9) radius of the actively star forming disc (within the last ≈100 Myr), estimated from the radial extent of the RC emission; (10) SFR surface density is with an uncertainty of 0.3 dex; (11) total mass , where r₂₅ is the radius of the galaxy estimated from d₂₅ using the distance D, and v₁₀₀ is the rotation speed in units of 100 km s⁻¹, with an uncertainty of 0.1 dex; (12) maximum rotation speeds in the flat part of the rotation curve with typical uncertainties of ±3 km s⁻¹.