From observing strategies to velocity dispersion bias: forward modeling unresolved binaries in ultra-faint dwarf galaxies
astro-ph.GA, astro-ph.SR
Submitted: 2026-09-16
Updated: 2026-09-16
Comments: 15 pages + appendices, 6 figures, submitted to ApJ. Code available at https://github.com/xou-mit/binary-observation-simulator
Code: https://github.com/xou-mit/binary-observation-simulator
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The abundance and properties of the lowest luminosity dwarf galaxies around the Milky Way: Insights from Semi-Analytic Models
- A Chemodynamical Census of the Milky Way's Ultra-Faint Compact Satellites. I. A First Population-Level Look at the Internal Kinematics and Metallicities of 19 Extremely-Low-Mass Halo Stellar Systems
- A Unified Framework Connecting Chemical Enrichment to Resolved Star Formation Histories with Applications to Local Group Dwarf Irregulars
- The Local Volume Database: a library of the observed properties of nearby dwarf galaxies and star clusters
- The Via Project: Overview of the Science, Instrument, and Survey
Related papers
- Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
- Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
- Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
- Deriving volume density profiles of filaments from observed surface densities
- Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
- MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies