All Tables

• Table 1: Template radio sources; Col. 1: source index; Col. 2: source name; Col. 3: reference for flux measurement; Col. 4: reference flux at 1380 MHz; Col. 5: reference flux at 1420 MHz; Col. 6: object type from Veron et al. (1972) or Kuhr et al. (1981).
• Table 2: Astrophysical HI-parameters (excerpt). Column 1: PGC or LEDA galaxy name; Col. 2: most usual galaxy name; Col. 3: J2000 equatorial coordinates; Col. 4: systemic heliocentric radial velocity (km s^-1); Col. 5: rms error (km s^-1); Col. 6: total line width at 20% of the maximum intensity (km s^-1); Col. 7: total corrected line width at 20% (km s^-1); Col. 8: rms error (km s^-1); Col. 9: total line width at 50% of the maximum intensity (km s^-1); Col. 10: total corrected line width at 50% (km s^-1); Col. 11: rms error (km s^-1); Col. 12: observed HI-flux (Jy km s^-1); Col. 13: beam-filling corrected HI-flux (Jy km s^-1); Col. 14: rms error (Jy km s^-1); Col. 15: signal to noise ratio; Col. 16: quality code (see Sect. 4) Col. 17: flag ("*'' marks a second independent measurement of lower quality, the 21-cm profile is not plotted in Fig. 4).
• Table 3: Notes on HI-observations (excerpt). Column 1: PGC or LEDA galaxy name; Col. 2: morphological type as known in HYPERLEDA; Col. 3: isophotal diameter D₂₅ in arcmin; Col. 4: position angle counted from the North () toward East between 0 and 180; Col. 5: quality code (see Sect. 2); Col. 6: comments; conf = "HI confusion'', comp = "companion'', cf = "comparison field'', poss = "possible'', w = "with''.
• Table 4: Template galaxies: Col. 1: PGC or HYPERLEDA galaxy name; Col. 2: right ascension (2000); Col. 3: declination (2000); Col. 4: morphological type; Col. 5: log D₂₅ isophotal diameter; Col. 6: log R₂₅ axis ratio; Col. 7: total B magnitude; Col. 8: total line width at 20% of the maximum intensity (km s^-1) (HYPERLEDA); Col. 9: 21-cm magnitude (HYPERLEDA); Col. 10: HI-flux in Jy km s^-1; (Theureau et al. 1998); Col. 11: systemic heliocentric radial velocity (km s^-1) (Theureau et al. 1998).