Large-Scale Structure in the NIR-Selected MUNICS Survey

Details Large-Scale Structure in the NIR-Selected MUNICS Survey Large-Scale Structure in the NIR-Selected MUNICS Survey

2002-10-15

arxiv.org/abs/astro-ph/0210329v1

Astrophys.Space Sci. 284 (2003) 393-396

Astronomy and Astrophysics

Astrophysics

4 pages, to appear in "The Evolution of Galaxies III. From Simple Approaches to Self-Consistent Models", proceedings of the 3r

Scientific paper

10.1023/A:1024058917022

The Munich Near-IR Cluster Survey (MUNICS) is a wide-area, medium-deep, photometric survey selected in the K' band. The project's main scientific aims are the identification of galaxy clusters up to redshifts of unity and the selection of a large sample of field early-type galaxies up to z < 1.5 for evolutionary studies. We created a Large Scale Structure catalog, using a new structure finding technique specialized for photometric datasets, that we developed on the basis of a friends-of-friends algorithm. We tested the plausibility of the resulting galaxy group and cluster catalog with the help of Color-Magnitude Diagrams (CMD), as well as a likelihood- and Voronoi-approach.

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