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J. D. Cohn

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ORCID 0000-0002-6365-4170

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collaborators

4 papers

astro-ph2008★ 150 cited

Reconstructing Baryon Oscillations: A Lagrangian Theory Perspective

Nikhil Padmanabhan, Martin White, J. D. Cohn

Recently Eisenstein and collaborators introduced a method to `reconstruct' the linear power spectrum from a non-linearly evolved galaxy distribution in order to improve precision i…

astro-ph2008★ 35 cited

The Clustering and Host Halos of Galaxy Mergers at High Redshift

Andrew R. Wetzel, J. D. Cohn, Martin White

High-resolution simulations of cosmological structure formation indicate that dark matter substructure in dense environments, like groups and clusters, may survive for a long time.…

astro-ph2008★ 84 cited

Simulating Subhalos at High Redshift: Merger Rates, Counts, and Types

Andrew R. Wetzel, J. D. Cohn, Martin White

Galaxies are believed to be in one-to-one correspondence with simulated dark matter subhalos. We use high-resolution N-body simulations of cosmological volumes to calculate the sta…

astro-ph2007★ 75 cited

Constraints on the correlation between QSO luminosity and host halo mass from high-redshift quasar clustering

Martin White, Paul Martini, J. D. Cohn

Recent measurements of high-redshift QSO clustering from the Sloan Digital Sky Survey indicate that QSOs at z~4 have a bias b~14. We find that this extremely high clustering amplit…

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