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SFI++ I: A New I‐Band Tully‐Fisher Template, the Cluster Peculiar Velocity Dispersion, and H0

  • Authors: Karen L. Masters, Christopher M. Springob, Martha P. Haynes, and Riccardo Giovanelli

Masters et al. 2006 The Astrophysical Journal 653 861.

  • Provider: AAS Journals

Caption: Fig. 6.

TF relations for individual clusters (not corrected for cluster peculiar velocities). Overlaid is the bivariate fit to the In sample from § 5 of ﹩M-5\mathrm{log}\,h=-20.849-7.845( \mathrm{log}\,W-2.5) ﹩. Solid circles are In sample galaxies, open circles In+. These data have been corrected for the incompleteness bias and other biases discussed in § 3.

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