The Munich Near-Infrared Cluster Survey (MUNICS) - IX. Galaxy Evolution to z ~ 2 From Optically Selected Catalogues

Simple item page
dc.creatorFeulner, Georg
dc.creatorGoranova, Yuliana
dc.creatorHopp, Ulrich
dc.creatorGabasch, Armin
dc.creatorBender, Ralf
dc.creatorBotzler, Christine S.
dc.creatorDrory, Niv
dc.date2007-03-30
dc.date.accessioned2026-07-07T11:01:19Z
dc.date.available2026-07-07T11:01:19Z
dc.description(Abridged) We present B, R, and I-band selected galaxy catalogues based on the Munich Near-Infrared Cluster Survey (MUNICS) which, together with the K-selected sample, serve as an important probe of galaxy evolution in the redshift range 0 < z < 2. Furthermore, used in comparison they are ideally suited to study selection effects. The construction of the B, R, and I-selected photometric catalogues, containing ~9000, ~9000, and ~6000 galaxies, respectively, is described in detail. The catalogues reach 50% completeness limits for point sources of B ~ 24.5mag, R ~ 23.5mag, and I ~ 22.5mag and cover an area of about 0.3 square degrees. Photometric redshifts are derived for all galaxies with an accuracy of dz/(1+z) ~ 0.057. We investigate the influence of selection band and environment on the specific star formation rate (SSFR). We find that K-band selection indeed comes close to selection in stellar mass, while B-band selection purely selects galaxies in star formation rate. We use a galaxy group catalogue constructed on the K-band selected MUNICS sample to study possible differences of the SSFR between the field and the group environment, finding a marginally lower average SSFR in groups as compared to the field, especially at lower redshifts. The field-galaxy luminosity function in the B and R band as derived from the R-selected sample evolves out to z ~ 2 in the sense that the characteristic luminosity increases but the number density decreases. This effect is smaller at longer rest-frame wavelengths and gets more pronounced at shorter wavelengths. Parametrising the redshift evolution of the Schechter parameters as M*(z) = M*(0) + a ln(1+z) and Phi*(z) = Phi*(0) (1+z)^b we find evolutionary parameters a ~ -2.1 and b ~ -2.5 for the B band, and a ~ -1.4 and b ~ -1.8 for the R band.
dc.description23 pages, 19 figures; accepted for publication in MNRAS; version with high-resolution figures will be made available at http://www.usm.uni-muenchen.de/people/feulner/munics9/preprint_munics9.pdf
dc.identifierhttps://arxiv.org/abs/astro-ph/0703792
dc.identifierhttp://arxiv.org/abs/astro-ph/0703792
dc.identifierMon.Not.Roy.Astron.Soc.378:429-448,2007
dc.identifierdoi:10.1111/j.1365-2966.2007.11802.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187918
dc.subjectAstrophysics
dc.titleThe Munich Near-Infrared Cluster Survey (MUNICS) - IX. Galaxy Evolution to z ~ 2 From Optically Selected Catalogues
dc.typetext

Files

Collections

arXiv