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The I-Band Tully-Fisher Relation for Cluster Galaxies: Data Presentation

R. Giovanelli·M. Haynes·T. Herter·N. Vogt·L. da Costa·W. Freudling·J. Salzer·G. Wegner
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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. The construction of a TF template, bias corrections and cluster motions are discussed in an accompanying paper.

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R. Giovanelli, M. Haynes, T. Herter, N. Vogt, L. da Costa, W. Freudling, J. Salzer, G. Wegner. 1996-10-15. The I-Band Tully-Fisher Relation for Cluster Galaxies: Data Presentation. https://doi.org/10.1086/118233

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