All Tables

Table 1: List of telescopes. Column 1: number of published 21-cm line widths; Col. 2: code number of the telescope in LEDA; Col. 3: Name of the telescope.
Table 2: Definition of the method of measurement of 21-cm line width. The columns are arranged as follows: Col. 1: number of published 21-cm line widths; Col. 2: code number of the method in LEDA; Col. 3: description of the method.
Table 3: List of the richest references (n>300). The columns are arranged as follows: Col. 1: number of measurements of 21-cm line width or $\log 2V_{\rm M}^{\sin i}$ ; Col. 2: code number of the reference in LEDA; Col. 3: Full reference. The full table is available in electronic form at the CDS.
Table 4: Correction of $\log W(r,l)$ to $\log 2V_{\rm M}^{\sin i}$ . This table gives the conversion coefficients and the mean error for the 26 subsamples (level and resolution). l is the level code (see Table 2). r is the mean velocity resolution in km s^-1. The full table is available in the electronic version of the journal.
Table 5: Correction of $\log 2V_{\rm M}^{\sin i}$ to the adopted standard (ref. 23286). This table gives the conversion coefficients and the mean error for the 65 references requiring an additional correction. The full table is available in the electronic version of the journal.
Table 6: Correction of m₂₁ to the scale of Nançay. This table gives the the zero-point shift and the mean error for the different radiotelescope (Col. 1). By its adoption as a standard, the Nançay radiotelescope (t=1) has b=0 and its standard deviation is $\sigma =0.24$ . The full table is available in the electronic version of the journal.
Table 7: Correction of m₂₁ to the standard (ref. 23289). This table gives the zero-point shift and its mean error for the 46 references requiring an additional correction. The full table is available in the electronic version of the journal.
Table 8: The final catalog of homogenized HI data. The catalog gives these data for 16 781 galaxies. The full catalog is available in electronic form at the CDS. Col. 1: PGC number from LEDA; Col. 2: Alternate name from LEDA; Col. 3: Right Ascension and Declination for the equinox 2000, in hours, minutes, seconds and tenths, and degrees, arcminutes and arcseconds; Col. 4: Mean homogenized decimal logarithm of twice the maximum rotation velocity uncorrected for inclination ( $V_{\rm M}^{\sin i}$ in km s^-1); Col. 5: Mean homogenized 21-cm magnitude (see Eq. (3)); Col. 6: Mean homogenized HI heliocentric radial velocity (in km s^-1); Each parameter is given with a flag f telling if it is uncertain (f=1).
Table A.1: New observations. (The full table is available in electronic form at the CDS). Col. 1: PGC number from LEDA; Col. 2: Alternate name from LEDA; Col. 3: Right Ascension and Declination for the equinox 2000, in hours, minutes, seconds and tenths, and degrees, arcminutes and arcseconds; Col. 4: 21-cm line width at 20% of the maximum (in km s^-1); Col. 5: 21-cm line width at 50% of the maximum (in km s^-1); Col. 6: HI heliocentric radial velocity (in km.s^-1); Col. 7: HI flux (area of the 21-cm line) (in mJy km s^-1); Col. 8: Signal to Noise ration; Col. 9: Quality of the line (see text) and notes (see Table A.3).
Table A.2: Periods of gain stability and correction factors ( $=F_0/F_{\rm HI}$ ).
Table A.3: Comments on some galaxies. The full table is available in electronic form at the CDS. The references concerning these comments are given at the end of the table.

Full Version
Table 4: Correction of $\log W(r,l)$ to $\log 2V_{M}^{\sin i}$ . This table gives the conversion coefficients and the mean error for the 26 subsamples (level and resolution). l is the level code (see Table 2). r is the mean velocity resolution in km s^-1.
Table 5: Correction of $\log 2V_{M}^{\sin i}$ to the adopted standard (ref. 23286). This table gives the conversion coefficients and the mean error for the 65 references requiring an additional correction.
Table 6: Correction of m₂₁ to the scale of Nançay. This table gives the the zero-point shift and the mean error for the different radiotelescope (Col. 1). By its adoption as a standard, the Nançay radiotelescope (t=1) has b=0 and its standard deviation is $\sigma =0.24$ .
Table 7: Correction of m₂₁ to the standard (ref. 23289). This table gives the zero-point shift and its mean error for the 46 references requiring an additional correction.