Galactic star formation and accretion histories from matching galaxies to dark matter haloes

We present a new statistical method to determine the relationship between the stellar masses of galaxies and the masses of their host dark matter haloes over the entire cosmic history from z ∼ 4 to the present. This multi-epoch abundance matching (MEAM) model self-consistently takes into account tha...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2013-02, Vol.428 (4), p.3121-3138
Hauptverfasser:	Moster, Benjamin P., Naab, Thorsten, White, Simon D. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Cosmic rays Dark matter Satellites Simulation Star & galaxy formation
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