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Groups of galaxies. III. the CfA survey

Journal Article · · Astrophys. J., Suppl. Ser.; (United States)
DOI:https://doi.org/10.1086/190859· OSTI ID:6049291
We present a statistically homogeneous group catalog (CfA) based on the CfA redshift survey (Huchra et al.). Groups in the catalog are all density enhancements in redshift space of a factor greater than 20. Group members are identified according to the procedure described in our previous study (Huchra and Geller) of a shallower whole-sky sample. All groups contain at least three members. Of the 176 groups in the CfA catalog, 102 have been identified in one or more previous studies. Because our algorithm searches for volume rather than surface density enhancements, the groups in a given region generally change only through the addition of fainter members when the magnitude limit of the galaxy catalog increases. In the region of overlap, agreement between our shallow catalog and the CfA catalog is excellent.
Research Organization:
Harvard-Smithsonian Center for Astrophysics
OSTI ID:
6049291
Journal Information:
Astrophys. J., Suppl. Ser.; (United States), Journal Name: Astrophys. J., Suppl. Ser.; (United States) Vol. 52:2; ISSN APJSA
Country of Publication:
United States
Language:
English

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