The Munich Near-IR Cluster Survey (MUNICS)

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dc.creatorDrory, N.
dc.creatorHopp, U.
dc.creatorBender, R.
dc.creatorFeulner, G.
dc.creatorSnigula, J.
dc.creatorde Oliveira, C. Mendes
dc.creatorHill, G.
dc.date1999-10-14
dc.date.accessioned2026-07-07T02:33:51Z
dc.date.available2026-07-07T02:33:51Z
dc.descriptionThe 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.
dc.description5 pages, 5 eps figures; uses newpasp.sty; to appear in the proceedings of the IGRAP 99 conference "Clustering at High Redshift"
dc.identifierhttps://arxiv.org/abs/astro-ph/9910268
dc.identifierhttp://arxiv.org/abs/astro-ph/9910268
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15014
dc.subjectAstrophysics
dc.titleThe Munich Near-IR Cluster Survey (MUNICS)
dc.typetext

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