Fig. 3 from SFI++ I: A New I‐Band Tully‐Fisher Template, the Cluster Peculiar Velocity Dispersion, and H0

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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. 3.

Absolute magnitude completeness histograms for each of the In+ cluster sample. The dashed lines show the smooth fits to the histograms used in our Monte Carlo simulations. The template clusters are ordered by right ascension and separated into Northern Hemisphere (top) and Southern Hemisphere (bottom) objects.

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