activity
19942023
most citedThe Optical and Near-Infrared Properties of Galaxies: I. Luminosity and Stellar Mass Functions

2.3k citations · 25.6k across the 160 of their papers we have counts for

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Showing 2001Show all

6 papers · 1 filter

astro-ph2001★ 218 cited

Bar-driven dark halo evolution: a resolution of the cusp--core controversy

Martin D. Weinberg, Neal Katz

Simulations predict that the dark matter halos of galaxies should have central cusps, while those inferred from observed galaxies do not have cusps. We demonstrate, using both line…

astro-ph2001★ 13 cited

Comparing Simulations and Observations of the Lyman-Alpha Forest I. Methodology

C. E. Petry, C. D. Impey, N. Katz +2

We describe techniques for comparing spectra extracted from cosmological simulations and observational data, using the same methodology to link Lyman-alpha properties derived from…

astro-ph2001★ 7 cited

The Infuence of Omega_baryon on High-Redshift Structure

Jeffrey P. Gardner, Neal Katz, Lars Hernquist +1

We analyze high-redshift structure in three hydrodynamic simulations that have identical initial conditions and cosmological parameters and differ only in the value of the baryon d…

astro-ph2001★ 6 cited

Sub-mm Galaxies in Cosmological Simulations

Mark A. Fardal, Neal Katz, David H. Weinberg +2

We study the predicted sub-mm emission from massive galaxies in a Lambda-CDM universe, using hydrodynamic cosmological simulations. Assuming that most of the emission from newly fo…

astro-ph2001★ 133 cited

The growth of galaxies in cosmological simulations of structure formation

Chigurupati Murali, Neal Katz, Lars Hernquist +2

We use hydrodynamic simulations to examine how the baryonic components of galaxies are assembled, focusing on the relative importance of mergers and smooth accretion in the formati…

astro-ph2001★ 226 cited

Metal Enrichment of the Intergalactic Medium in Cosmological Simulations

Anthony Aguirre, Lars Hernquist, Joop Schaye +3

Observations have established that the diffuse intergalactic medium (IGM) at z ~ 3 is enriched to ~0.1-1% solar metallicity and that the hot gas in large clusters of galaxies (ICM)…