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S., Wechsler, R

21 Pith papers cite this work, alongside 548 external citations. Polarity classification is still indexing.

21 Pith papers citing it
548 external citations · Pith
abstract

We present a new algorithm for generating merger trees and halo catalogs which explicitly ensures consistency of halo properties (mass, position, and velocity) across timesteps. Our algorithm has demonstrated the ability to improve both the completeness (through detecting and inserting otherwise missing halos) and purity (through detecting and removing spurious objects) of both merger trees and halo catalogs. In addition, our method is able to robustly measure the self-consistency of halo finders; it is the first to directly measure the uncertainties in halo positions, halo velocities, and the halo mass function for a given halo finder based on consistency between snapshots in cosmological simulations. We use this algorithm to generate merger trees for two large simulations (Bolshoi and Consuelo) and evaluate two halo finders (ROCKSTAR and BDM). We find that both the ROCKSTAR and BDM halo finders track halos extremely well; in both, the number of halos which do not have physically consistent progenitors is at the 1-2% level across all halo masses. Our code is publicly available at http://code.google.com/p/consistent-trees . Our trees and catalogs are publicly available at http://hipacc.ucsc.edu/Bolshoi/ .

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representative citing papers

Galactic Amnesia: The Information Washout of the Milky Way Merger History

astro-ph.GA · 2026-05-05 · unverdicted · novelty 6.0

Mutual information analysis of TNG50 simulations shows gravitational potential and total energy retain merger mass and infall time information longest, while radial velocity loses it within ~5 Gyr, with washout depending on radius, merger age, and mass.

Resolving galaxy formation in the early Universe with BonFIRE and CampFIRE

astro-ph.GA · 2026-05-22 · unverdicted · novelty 5.0

BonFIRE and CampFIRE simulations show bursty clustered star formation in early galaxies and predict UV luminosity functions matching observations at faint magnitudes with a turnover at M_UV approx -14 but overpredicting brighter galaxies.

Correlation between baryonic process and galaxy assembly bias

astro-ph.GA · 2026-05-19 · unverdicted · novelty 5.0

Simulations show gas cooling and stellar feedback dominate assembly bias for stellar-mass selected galaxies while star formation gives way to gas cooling for SFR-selected galaxies as number density rises.

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Showing 11 of 11 citing papers after filters.