Modeling Luminosity‐dependent Galaxy Clustering through Cosmic Time
نویسندگان
چکیده
منابع مشابه
Modeling Luminosity-dependent Galaxy Clustering through Cosmic Time
We employ high-resolution dissipationless simulations of the concordance ΛCDM cosmology (Ω0 = 1 − ΩΛ = 0.3, h = 0.7, σ8 = 0.9) to model the observed luminosity dependence and evolution of galaxy clustering through most of the age of the universe, from z ∼ 5 to z ∼ 0. We use a simple, nonparametric model which monotonically relates galaxy luminosities to the maximum circular velocity of dark mat...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2006
ISSN: 0004-637X,1538-4357
DOI: 10.1086/503602