499 citations · 751 across the 6 of their papers we have counts for
4 papers · 1 filter
When Does the Intergalactic Medium Become Enriched?
Benjamin D. Oppenheimer, Romeel Davé, Kristian Finlator
We use cosmological hydrodynamic simulations including galactic feedback based on observations of local starbursts to find a self-consistent evolutionary model capable of fitting t…
The Mass-Metallicity Relation in Cosmological Hydrodynamic Simulations
Romeel Daveé, Kristian Finlator, Benjamin D. Oppenheimer
We use cosmological hydrodynamic simulations with enriched galactic outflows to compare predictions for the galaxy mass-metallicity (M*-Z) relation versus observations at z~2 from…
Constraints on Physical Properties of z~6 Galaxies Using Cosmological Hydrodynamic Simulations
K. Finlator, R. Dave', B. Oppenheimer
We conduct a detailed comparison of broad-band spectral energy distributions of six z >= 5.5 galaxies against galaxies drawn from cosmological hydrodynamic simulations. We employ a…
Measuring the Average Evolution of Luminous Galaxies at z<3: The Rest-frame Optical Luminosity Density, Spectral Energy Distribution, and Stellar Mass Density
Gregory Rudnick, Ivo Labbe, Natascha M. Foerster Schreiber +11
(Abridged) We present the evolution of the volume averaged properties of the rest-frame optically luminous galaxy population to z~3, determined from four disjoint deep fields with…