Notes. 1: Late-type galaxies with an HI-deficiency  ≤ 0.4. 2: Detected in the three SPIRE bands. 3: Detected by IRAS at 60 and 100 μm. 4: Determined from Hα data accurately corrected for [NII] contamination and dust extinction as described in Boselli et al. (2009). Galaxies hosting an AGN are not included. 5: With a metallicity measured using the same calibration (Hughes et al., in prep.). 6: With a direct measure of the Balmer decrement from integrated spectra (Boselli et al., in prep.). 7: With A(FUV) directly measured from the far infrared to FUV flux ratio as described in Cortese et al. (2008).