Abstract
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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References
Bahcall, N.A.: 1977, Clusters of galaxies, ARAA 15, 505–540.
Bahcall, N.A., Fan, X. and Cen, R.: 1997, Constraining Omega with cluster evolution, ApJ 485, L53+.
Bender, R., Appenzeller, I., Böhm, A., Drory, N., Fricke, K.J., Gabasch, A., Heidt, J., Hopp, U., Jäger, K., Kummel, M., Mehlert, D., Möllenhoff, C., Moorwood, A., Nicklas, H., Noll, S., Saglia, R.P., Seifert, W., Seitz, S., Stahl, O., Sutoriaus, E., Szeifert, T., Wagner, S.J. and Ziegler, B.L.: 2001, The FORS deep field: Photometric data and photometric redshifts, in: S. Christiani (ed.): ESO/ECF/STScI Workshop on Deep Fields, Springer, Berlin, pp. 327+.
Drory, N., Bender, R., Snigula, J., Feulner, G., Hopp, U., Maraston, C., Hill, G.J. and de Oliveira, C.M.: 2001a, The Munich near-infrared cluster survey: Number density evolution of massive field galaxies to z —1.2 as derived from the K-band-selected survey, ApJ 562, L111—LL114.
Drory, N., Feulner, G., Bender, R., Botzler, C.S., Hopp, U., Maraston, C., Mendes de Oliveira, C. and Snigula, J.: 200 lb, The Munich near-infrared cluster survey — I. Field selection, object extraction, and photometry, MNRAS 325, 550–562.
Feulner, G., Bender, R., Drory, N., Hopp, U., Snigula, J. and Hill, G.J.: 2003, The Munich near-infrared cluster survey (MUNICS) — V. The evolution of the rest-frame K-band and J-band galaxy luminosity functions to z — 0.7. MNRAS accepted.
Huchra, J.P. and Geller, M.J.: 1982, Groups of galaxies. I — Nearby groups, ApJ 257, 423–437.
Maraston, C.: 1998, Evolutionary synthesis of stellar populations: a modular tool, MNRAS 300, 872–892.
Nolthenius, R. and White, S.D.M.: 1987, Groups of galaxies in the CfA survey and in cold dark matter universes, MNRAS 225, 505–530.
Ramella, M., Boschin, W., Fadda, D. and Nonino, M.: 2001, Finding galaxy clusters using Voronoi tessellations, AA 368, 776–786.
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Botzler, C.S. et al. (2003). Large-Scale Structure in the NIR-Selected Munics Survey. In: Hensler, G., Stasińska, G., Harfst, S., Kroupa, P., Theis, C. (eds) The Evolution of Galaxies. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-3315-1_17
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DOI: https://doi.org/10.1007/978-94-017-3315-1_17
Publisher Name: Springer, Dordrecht
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