activity
19962021
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 7.4k across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.CO2021★ 128 cited

The Cosmological -body Code

Lehman H. Garrison, Daniel J. Eisenstein, Douglas Ferrer +2

We present , a fast and accurate cosmological -body code based on a new method for calculating the gravitational potential from a static multipole mesh. The met…

astro-ph.CO2019★ 35 cited

Cosmology with Stacked Cluster Weak Lensing and Cluster-Galaxy Cross-Correlations

Andrés N. Salcedo, Benjamin D. Wibking, David H. Weinberg +4

Cluster weak lensing is a sensitive probe of cosmology, particularly the amplitude of matter clustering and matter density parameter . The main nuisance parameter in a c…

astro-ph.CO2018★ 103 cited

A High-Fidelity Realization of the Euclid Code Comparison -body Simulation with Abacus

Lehman H. Garrison, Daniel J. Eisenstein, Philip A. Pinto

We present a high-fidelity realization of the cosmological -body simulation from the Schneider et al. (2016) code comparison project. The simulation was performed with our Abacu…

astro-ph.CO2017★ 105 cited

The Abacus Cosmos: A Suite of Cosmological N-body Simulations

Lehman H. Garrison, Daniel J. Eisenstein, Douglas Ferrer +3

We present a public data release of halo catalogs from a suite of 125 cosmological -body simulations from the Abacus project. The simulations span 40 CDM cosmologies centered…

astro-ph.CO2017★ 59 cited

Emulating galaxy clustering and galaxy-galaxy lensing into the deeply nonlinear regime: methodology, information, and forecasts

Benjamin D. Wibking, Andrés N. Salcedo, David H. Weinberg +6

The combination of galaxy-galaxy lensing (GGL) with galaxy clustering is one of the most promising routes to determining the amplitude of matter clustering at low redshifts. We sho…

astro-ph.CO2016★ 74 cited

Improving Initial Conditions for Cosmological -Body Simulations

Lehman H. Garrison, Daniel J. Eisenstein, Douglas Ferrer +2

In cosmological -body simulations, the representation of dark matter as discrete "macroparticles" suppresses the growth of structure, such that simulations no longer reproduce l…