activity
20172026
most citedMilky Way Satellite Census. III. Constraints on Dark Matter Properties from Observations of Milky Way Satellite Galaxies

331 citations · 2.8k across the 96 of their papers we have counts for

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Showing 2026Show all

11 papers · 1 filter

astro-ph.GA2026

Linking orbital history to the quenching of isolated dwarf galaxies

Sophia Um, Devontae C. Baxter, Ethan O. Nadler

Recent discoveries of isolated dwarf galaxies () with no signs of ongoing star formation have challenged the prevailing notion that these…

astro-ph.GA2026

Detectable subhalo impacts in Milky Way streams

Junyang Lu, Elias Bernreuther, Tongyan Lin +3

Dark matter subhalos leave gravitational imprints in the stellar streams of the Milky Way. Observing individual strong impacts of subhalos offers a compelling way to constrain and…

astro-ph.CO2026

Dark Matter Constraints from Small-Scale Cosmic Structure

Ethan O. Nadler, Keir K. Rogers, Alex Drlica-Wagner

Small-scale cosmic structure provides a powerful test of the fundamental nature of dark matter (DM). A wide range of DM models impact matter clustering on small scales, including w…

astro-ph.GA2026

What becomes of JWST/NIRCam-selected high-redshift massive galaxies?

Devontae C. Baxter, Alison L. Coil, Ethan O Nadler +2

Early JWST/NIRCam surveys revealed a puzzling population of high-redshift massive galaxy candidates largely absent from previous rest-frame UV surveys. Spectroscopic follow-up has…

astro-ph.CO2026

A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations

Andrew J. Benson, Ethan O. Nadler, Xiaolong Du +1

We measure the dark matter halo mass function, with backsplash halos removed, from a wide range of cosmological-box and zoom-in simulations. These include the MultiDark Planck boxe…

astro-ph.CO2026

Mixed Dark Matter: Limits from the Milky Way Satellite Galaxies

Wendy Crumrine, Dominic Pang, Ethan O. Nadler +2

The Standard Model of particle physics contains a diverse set of particle species, motivating the possibility of a similarly complex dark sector. Here we study two-component dark m…