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20182026
most citedCompleteness of the Gaia-verse III: using hidden states to infer gaps, detection efficiencies and the scanning law from the DR2 light curves

19 citations · 22 across the 5 of their papers we have counts for

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5 papers · 1 filter

astro-ph.GA2026

From observing strategies to velocity dispersion bias: forward modeling unresolved binaries in ultra-faint dwarf galaxies

Xiaowei Ou, Andrew B. Pace, Nitya Kallivayalil +9

Ultra-faint dwarf galaxies (UFDs) in the Milky Way are ideal probes of low-mass galaxy formation and dark matter because they are highly dark-matter dominated. In the lowest-mass s…

astro-ph.GA2025★ 3 cited

Stellar velocity distributions in binary-rich ultrafaint dwarf galaxies

Amery Gration, David D. Hendriks, Payel Das +2

Ultrafaint dwarf (UFD) galaxies are dominated by dark matter, the distribution of which may be inferred from the kinematics of that galaxy's stellar population. Star-by-star observ…

astro-ph.GA2024

Mapping dust in the giant molecular cloud Orion A

Amery Gration, John Magorrian

The Sun is located close to the Galactic mid-plane, meaning that we observe the Galaxy through significant quantities of dust. Moreover, the vast majority of the Galaxy's stars als…

astro-ph.GA2020★ 19 cited

Completeness of the Gaia-verse III: using hidden states to infer gaps, detection efficiencies and the scanning law from the DR2 light curves

Douglas Boubert, Andrew Everall, Jack Fraser +2

The completeness of the Gaia catalogues heavily depends on the status of that space telescope through time. Stars are only published with each of the astrometric, photometric and s…

astro-ph.GA2018

Dynamical modelling of dwarf-spheroidal galaxies using Gaussian-process emulation

Amery Gration, Mark I. Wilkinson

We present a novel and efficient method for fitting dynamical models of stellar kinematic data in dwarf spheroidal galaxies (dSph). Our approach is based on Gaussian-process emulat…