633 citations · 1.5k across the 7 of their papers we have counts for
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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…
Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
Benjamin D. Oppenheimer, Romeel Davé
We investigate models of self-consistent chemical enrichment of the intergalactic medium (IGM) from z=6 to 1.5, based on hydrodynamic simulations of structure formation that incorp…