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Clustering of Loose Groups and Galaxies in the Perseus‐Pisces Survey

  • Authors: Roberto Trasarti-Battistoni, Gianluca Invernizzi, and Silvio A. Bonometto

Trasarti‐Battistoni, Invernizzi, & Bonometto 1997 The Astrophysical Journal 475 1.

  • Provider: AAS Journals

Caption: Fig. 2.

Ratio dNG/dNg between the number dNG of (identified) groups and the number dNg of (observed) galaxies in the galaxy sample PPS2. Three typical cases (with different search parameters D0, V0, and φ(L); see Table 1) are shown. Within the relevant distance range 2000 ≲ cz/km s−1 ≲ 10,000, the radial distribution of groups and galaxies are in good agreement, i.e., groups and galaxies share the same radial selection function (dNG/dNg ~ 1/15 independently of cz).

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