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20152024
most citedemcee v3: A Python ensemble sampling toolkit for affine-invariant MCMC

292 citations · 834 across the 17 of their papers we have counts for

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Showing astro-ph.COShow all

6 papers · 1 filter

astro-ph.CO2024

Reversing Arrested Development: A New Method to Address Halo Assembly Bias

William Smith, Andreas Berlind, Manodeep Sinha

Halo assembly bias is a phenomenon whereby the clustering of dark matter halos is dependent on halo properties, such as age, at fixed mass. Understanding the origin of assembly bia…

astro-ph.CO2019204 cited

Corrfunc --- A Suite of Blazing Fast Correlation Functions on the CPU

Manodeep Sinha, Lehman H. Garrison

The two-point correlation function (2PCF) is the most widely used tool for quantifying the spatial distribution of galaxies. Since the distribution of galaxies is determined by gal…

astro-ph.CO2019

The 21cm bispectrum during reionization: a tracer of the ionization topology

Anne Hutter, Catherine A. Watkinson, Jacob Seiler +3

We compute the bispectra of the 21cm signal during the Epoch of Reionization for three different reionization scenarios that are based on a dark matter N-body simulation combined w…

astro-ph.CO2018

The Secondary Spin Bias of Dark Matter Haloes

James W. Johnson, Ariyeh H. Maller, Andreas A. Berlind +2

We investigate the role of angular momentum in the clustering of dark matter haloes. We make use of data from two high-resolution N-body simulations spanning over four orders of ma…

astro-ph.CO2018

Likelihood Non-Gaussianity in Large-Scale Structure Analyses

ChangHoon Hahn, Florian Beutler, Manodeep Sinha +3

Standard present day large-scale structure (LSS) analyses make a major assumption in their Bayesian parameter inference --- that the likelihood has a Gaussian form. For summary sta…

astro-ph.CO201788 cited

Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties

Andrés N. Salcedo, Ariyeh H. Maller, Andreas A. Berlind +5

We explore the phenomenon commonly known as halo assembly bias, whereby dark matter halos of the same mass are found to be more or less clustered when a second halo property is con…