1999/10/14 by N. Drory, Niv Drory, U. Hopp +14
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9910268
5 pages, 5 eps figures; uses newpasp.sty; to appear in the proceedings of the IGRAP 99 conference "Clustering at High Redshift"
arxiv created 1999/10/14 · openalex publication_date 1999/10/14 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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