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pro vyhledávání: '"K. G. Noeske"'
Autor:
S. M. Faber, C. N. A. Willmer, C. Wolf, D. C. Koo, B. J. Weiner, J. A. Newman, M. Im, A. L. Coil, C. Conroy, M. C. Cooper, M. Davis, D. P. Finkbeiner, B. F. Gerke, K. Gebhardt, E. J. Groth, P. Guhathakurta, J. Harker, N. Kaiser, S. Kassin, M. Kleinheinrich, N. P. Konidaris, R. G. Kron, L. Lin, G. Luppino, D. S. Madgwick, K. Meisenheimer, K. G. Noeske, A. C. Phillips, V. L. Sarajedini, R. P. Schiavon, L. Simard, A. S. Szalay, N. P. Vogt, R. Yan
The DEEP2 and COMBO-17 surveys are used to study the evolution of the luminosity function of red and blue galaxies to $z \sim 1$. Schechter function fits show that, since $z = 1$, $M^*_B$ dims by $\sim$ 1.3 mag per unit redshift for both color classe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::87183f06718aa7e5d3383a82ba28447a
https://doi.org/10.1086/519294
https://doi.org/10.1086/519294
