Notes. Columns are (1): HRS name; (2): Reference to the integrated spectrum: 1: B15; 2: Kennicutt (1992). (3): (Integrated) Hα EW corrected for continuum absorption according to GANDALF; (4): (Integrated) [OIII]/Hβ; (5): (Integrated) [NII]/Hα; (6): (Integrated) [SII]/Hα; (7): (Integrated) classification using the BPT ([NII]/Hα and [SII]/Hα) diagrams; (8): (Integrated) classification using the WHAN diagram; (9): Reference to the nuclear spectroscopy: 3: this work or Gavazzi et al. (2013); 4: SDSS DR13 or DR12 (Albareti et al. 2017); 5: Ho et al. (1997); 6: Jones et al. (2009); 7: Veilleux et al. (1995); 8: Jansen et al. (2000); 9: Falco et al. (1999). (10): (Nuclear) Hα EW corrected for continuum absorption according to GANDALF or according to Table 1; (11): (Nuclear) [OIII]/Hβ; (12): (Nuclear) [NII]/Hα; (13): (Nuclear) [SII]/Hα; notice that the nuclear value of the [OI]/Hα ratio (available for only 101 galaxies) is not reported. (14): (Nuclear) classification using the BPT ([NII]/Hα and [SII]/Hα) diagrams; (15): (Nuclear) classification using the WHAN diagram. Columns marked "" were not observed, while columns marked - were not detected; positive EW means emission. A letter “a” marks galaxies with integrated spectra remeasured by us using the GANDALF code; letter “b” marks galaxies with Hβ SN < 3.0 instead letter “c” marks galaxies with Hα SN < 3.0 in the integrated spectrum; letter “d” marks galaxies with nuclear Hβ SN < 3.0. Cols. (2)-(8) refer to integrated spectra, Cols. (9)-(15) to nuclear spectra. In Cols. (6) and (12) the classification “(PAS)” is added to galaxies whose spectra do not contain Hα, [NII], [OIII], Hβ, [SII](6716Å), and [SII](6731Å) in emission. In Cols. (7) and (14), two BPT classifications are reported: the first spectral type is from the BPT with [NII]/Hα ratio, the second is from the BPT with [SII]/Hα ratio. The full catalog is available at the CDS in the electronic form.