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

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

1996-10-15

arxiv.org/abs/astro-ph/9610117v1

Astron.J.113:22-52,1997

Astronomy and Astrophysics

Astrophysics

38 pages, 3 tables, 18 figures, uses AAS LaTex; to appear in AJ Jan 97 Table 2 consists of 23 pages. Only the first page is in

Scientific paper

10.1086/118233

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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