activity
20192025
most citedA dark matter profile to model diverse feedback-induced core sizes of CDM haloes

160 citations · 466 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2025★ 5 cited

Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter

Maria C. Straight, Michael Boylan-Kolchin, James S. Bullock +6

We investigate the central density structure of dark matter halos in cold dark matter (CDM) and self-interacting dark matter (SIDM) models using simulations that are part of the Fe…

astro-ph.CO2024★ 36 cited

Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Robert Feldmann, Michael Boylan-Kolchin, James S. Bullock +11

Recent observations with the James Webb Space Telescope (JWST) have uncovered unexpectedly high cosmic star formation activity in the early Universe, mere hundreds of millions of y…

astro-ph.CO2023

An analytic surface density profile for CDM halos and gravitational lensing studies

Alexandres Lazar, James S. Bullock, Anna Nierenberg +2

We introduce an analytic surface density profile for dark matter halos that accurately reproduces the structure of simulated halos of mass , makin…

astro-ph.GA2022★ 70 cited

Galaxies lacking dark matter produced by close encounters in a cosmological simulation

Jorge Moreno, Shany Danieli, James S. Bullock +18

The standard cold dark matter plus cosmological constant model predicts that galaxies form within dark-matter haloes, and that low-mass galaxies are more dark-matter dominated than…

astro-ph.CO2020★ 17 cited

Out of sight, out of mind? The impact of correlated clustering in substructure lensing

Alexandres Lazar, James S. Bullock, Michael Boylan-Kolchin +3

A promising route for revealing the existence of dark matter structures on mass scales smaller than the faintest galaxies is through their effect on strong gravitational lenses. We…

astro-ph.GA2020★ 114 cited

The time-scales probed by star formation rate indicators for realistic, bursty star formation histories from the FIRE simulations

José A. Flores Velázquez, Alexander B. Gurvich, Claude-André Faucher-Giguère +10

Understanding the rate at which stars form is central to studies of galaxy formation. Observationally, the star formation rates (SFRs) of galaxies are measured using the luminosity…

astro-ph.GA2020★ 160 cited

A dark matter profile to model diverse feedback-induced core sizes of CDM haloes

Alexandres Lazar, James S. Bullock, Michael Boylan-Kolchin +11

We analyze the cold dark matter density profiles of 54 galaxy halos simulated with FIRE-2 galaxy formation physics, each resolved within of the halo virial radius. These ha…

astro-ph.GA2019★ 51 cited

Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations

Ethan D. Jahn, Laura V. Sales, Andrew Wetzel +5

Within CDM, dwarf galaxies like the Large Magellanic Cloud (LMC) are expected to host numerous dark matter subhalos, several of which should host faint dwarf companions. Recent…

astro-ph.GA2019★ 13 cited

Accurate mass estimates from the proper motions of dispersion-supported galaxies

Alexandres Lazar, James S. Bullock

Starting with the spherical Jeans equation, we show that there exists a radius where the mass enclosed depends only on the projected tangential velocity dispersion, assuming that t…