The Munich Near-IR Cluster Survey (MUNICS)

N. Drory; U. Hopp; R. Bender; G. Feulner; J. Snigula; C. Mendes de Oliveira; G. Hill

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The Munich Near-IR Cluster Survey (MUNICS)

N. Drory·U. Hopp·R. Bender·G. Feulner·J. Snigula·C. Mendes de Oliveira·G. Hill

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Abstract

The Munich Near-IR Cluster Survey (MUNICS) is a K' selected survey covering 1 square degree in the K' and J NIR bands with complementary optical photometry in the V, R, and I bands covering a subarea of 0.35 square degrees. The 3-sigma limiting magnitude is 19.5 in K'. The main goals of the project are the identification of clusters of galaxies at redshifts 0.6<z<1.0 and the study of the evolution of the early-type field population at similar redshifts. Here we present first results regarding color distributions and the surface densities of EROs as well as photometric redshifts and a first clustering analysis of the sample.

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N. Drory, U. Hopp, R. Bender, G. Feulner, J. Snigula, C. Mendes de Oliveira, G. Hill. 1999-10-14. The Munich Near-IR Cluster Survey (MUNICS). https://arxiv.org/abs/astro-ph/9910268

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