THE ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 107:97-102, 1996 November

          PARAMETERS OF 2447 SOUTHERN SPIRAL GALAXIES FOR USE IN THE
                             TULLY-FISHER RELATION

                        D. D. MATHEWSON AND V. L. FORD
      Mount Stromlo and Siding Spring Observatories, Australian National
    University, Private Bag, Weston Creek Post Office, ACT 2611, Australia


                                   ABSTRACT

        I-band luminosities, rotational velocities, and redshifts of 1092
     spiral galaxies have been measured by CCD photometry and Halpha
     spectroscopy using the 1 m and 2.3 m telescopes at Siding Spring
     Observatory, respectively.  The results are tabulated.  Luminosity
     profiles and Halpha rotation curves are given for the galaxies.
        When these results are combined with similar data for 1355 spiral
     galaxies published previously (Mathewson, Ford, & Buchhorn, hereafter
     Paper I), it provides a large, uniform, and unique data set with which
     to measure, via the Tully-Fisher relation, the peculiar velocities of
     galaxies in the local universe to a distance of 11,000 km/s (Mathewson
     & Ford).
        Taking advantage of the opportunity for publishing this data in
     machine-readable form, in the CD-ROM, we have also published similar
     data for the 1355 galaxies in Paper I.

     Subject headings: galaxies: distances and redshifts -- galaxies:
                       kinematics and dynamics -- galaxies: photometry --
                       surveys