THE ASTRONOMICAL JOURNAL    VOLUME 113, IN PRESS                   JANUARY 1997

    THE I BAND TULLY-FISHER RELATION FOR CLUSTER GALAXIES: DATA PRESENTATION

    RICCARDO GIOVANELLI, MARTHA P. HAYNES, TERRY HERTER, AND NICOLE P. VOGT

     Center for Radiophysics and Space Research and National Astronomy and
         Ionosphere Center, Cornell University, Ithaca, New York 14853

                                  GARY WEGNER

            Department of Physics and Astronomy, Dartmouth College,
                         Hanover, New Hampshire 03755

                                JOHN J. SALZER

  Department of Astronomy, Wesleyan University, Middletown, Connecticut 06459

                               LUIZ N. Da COSTA

         European Southern Observatory, Karl Schwarzschild Strasse 2,
                     D-85748 Garching b. Muenchen, Germany

                               WOLFRAM FREUDLING

 Space Telescope-European Coordinating Facility, Karl Schwarzschild Strasse 2,
                     D-85748 Garching b. Muenchen, Germany


                                   ABSTRACT

    Observational parameters which can be used for redshift-independent
    distance determination using the Tully-Fisher (TF) technique are given
    for 782 spiral galaxies in the fields of 24 clusters or groups.  I band
    photometry for the full sample was either obtained by us or compiled
    from published literature.  Rotational velocities are derived either
    from 21 cm spectra or optical emission line long-slit spectra, and
    converted to a homogeneous scale.  In addition to presenting the data,
    a discussion of the various sources of error on TF parameters is
    introduced, and the criteria for the assignment of membership to each
    cluster are given.