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

Observational parameters which can be used for redshift-independent di stance determination using the Tully-Fisher (TF) technique are given f or 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 f rom published literature. Rotational velocities are derived either fro m 21 cm spectra or optical emission line long-slit spectra, and conver ted to a homogeneous scale. In addition to presenting the data, a disc ussion of the various sources of error on TF parameters is introduced, and the criteria for the assignment of membership to each cluster are given. (C) 1997 American Astronomical Society.