activity
20192026
most citedIdentical or fraternal twins? : The chemical homogeneity of wide binaries from Gaia DR2

94 citations · 346 across the 22 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

15 papers · 1 filter

astro-ph.GA2026

The Twentieth Data Release of the Sloan Digital Sky Survey: First All-Sky BOSS Spectra, eROSITA-SDSS-V Mapper Coordinated Observations, and a Preview of the Local Volume Mapper

SDSS Collaboration, Mojgan Aghakhanloo, David Aguilar +273

This paper presents the twentieth data release (DR20) from the Sloan Digital Sky Survey, the third data release of its fifth generation (SDSS-V). SDSS-V is a panoptic spectroscopy…

astro-ph.GA2026

The Milky Way's Missing In-Situ Halo

Madeline Lucey, Robyn E. Sanderson, Alexander H. Riley +3

The Milky Way's stellar halo preserves a record of its mass assembly history, encoding accretion events in its structural properties. Among the most prominent of these features is…

astro-ph.GA2026

The Dynamics of Old Inner Galaxy Stars in Milky Way-mass Galaxies Using FIRE-2 Simulations

Emma Tasso, Madeline Lucey, Robyn Sanderson +2

Understanding how galaxies like the Milky Way assembled over cosmic time remains a central question in astrophysics. Understanding the processes that shaped their formation and evo…

astro-ph.GA2026

Self-consistent dynamical modelling of the Milky Way bar with orbital frequency analysis

Zachary Langford, Robyn Sanderson, Madeline Lucey +1

We present an update to the frequency analysis method for measuring the properties of a galactic bar. The method involves computing the fundamental frequencies of orbits in rotatin…

astro-ph.GA2026

Discovery of the First Five Carbon-Enhanced Metal-Poor Stars in the LMC

Madeline Lucey, Vedant Chandra, Alexander Ji +7

A substantial fraction of metal-poor stars in the local Milky Way halo exhibit large overabundances of carbon. These stars, dubbed Carbon-Enhanced Metal-Poor (CEMP) stars, provide…

astro-ph.GA2025

Inferring Stellar Densities with Flexible Models I: The Distribution of RR Lyrae in the Milky Way with DR3

Madeline Lucey, Cecilia Mateu, Adrian Price-Whelan +3

Understanding the formation and evolutionary history of the Milky Way requires detailed mapping of its stellar components, which preserve fossil records of the Galaxy's assembly th…

astro-ph.GA2025★ 6 cited

Mapping the Distant and Metal-Poor Milky Way with SDSS-V

Vedant Chandra, Phillip A. Cargile, Alexander P. Ji +28

The fifth-generation Sloan Digital Sky Survey (SDSS-V) is conducting the first all-sky low-resolution spectroscopic survey of the Milky Way's stellar halo. We describe the stellar…

astro-ph.GA2025★ 8 cited

The Nineteenth Data Release of the Sloan Digital Sky Survey

SDSS Collaboration, Gautham Adamane Pallathadka, Mojgan Aghakhanloo +210

Mapping the local and distant Universe is key to our understanding of it. For decades, the Sloan Digital Sky Survey (SDSS) has made a concerted effort to map millions of celestial…

astro-ph.GA2025

Counterculture Stars: Slow and Retrograde Stars with Low-Alpha Disk Abundances

Carrie Filion, Michael S. Petersen, Danny Horta +3

The Milky Way is home to a thin disk that can be defined via kinematics and/or elemental abundances. The elemental abundance-defined thin disk, also called the low-alpha disk, is g…

astro-ph.GA2024

Cosmological predictions for minor axis stellar density profiles in the inner regions of Milky Way-mass galaxies

Madeline Lucey, Robyn Sanderson, Danny Horta +5

CDM cosmology predicts the hierarchical formation of galaxies which build up mass by merger events and accreting smaller systems. The stellar halo of the Milky Way has proven to…

astro-ph.GA2022★ 28 cited

Carbon-Enhanced Metal-Poor star candidates from BP/RP Spectra in DR3

Madeline Lucey, Nariman Al Kharusi, Keith Hawkins +6

Carbon-enhanced metal-poor (CEMP) stars comprise almost a third of stars with [Fe/H] < --2, although their origins are still poorly understood. It is highly likely that one sub-cla…

astro-ph.GA2022★ 44 cited

Dynamically constraining the length of the Milky Way bar

Madeline Lucey, Sarah Pearson, Jason A. S. Hunt +5

We present a novel method for constraining the length of the Galactic bar using 6D phase space information to directly integrate orbits. We define a pseudo-length for the Galactic…

astro-ph.GA2021

The COMBS Survey -- III. The Chemodynamical Origins of Metal-Poor Bulge Stars

Madeline Lucey, Keith Hawkins, Melissa Ness +6

The characteristics of the stellar populations in the Galactic Bulge inform and constrain the Milky Way's formation and evolution. The metal-poor population is particularly importa…

astro-ph.GA2020★ 44 cited

The COMBS Survey -- II. Distinguishing the Metal-Poor Bulge from the Halo Interlopers

Madeline Lucey, Keith Hawkins, Melissa Ness +9

The metal-poor stars in the bulge are important relics of the Milky Way's formation history, as simulations predict that they are some of the oldest stars in the Galaxy. In order t…

astro-ph.GA2020★ 22 cited

The Chemical Nature of the Young 120-Myr-old Nearby Pisces-Eridanus Stellar Stream Flowing through the Galactic Disk

Keith Hawkins, Madeline Lucey, Jason Curtis

Recently, a new cylindrical-shaped stream of stars up to 700 pc long was discovered hiding in the Galactic disk using kinematic data enabled by the Gaia mission. This stream of sta…