The I band Tully-Fisher relation for cluster galaxies: data presentation.

Observational parameters which can be used for redshift-independent distance determination using the Tully-Fisher (TF) technique are given for 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.