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20242026
most citedMilky Way Mapper decoded abundances -- I. Shared disc enrichment patterns

2 citations · 2 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2026

Milky Way Mapper decoded abundances -- II: From patterns to paths

Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15

The element abundances of Milky Way disc stars encode entangled imprints of multiple enrichment processes, making it difficult to uncover the underlying chemical evolution. Here we…

astro-ph.GA20262 cited

Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns

Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15

Elemental abundances in the Milky Way disc trace its star-formation and enrichment history, but predicting these abundances from theory is limited by uncertain nucleosynthetic yiel…

astro-ph.GA2025

Hydrostatic and explosive -element chemical abundances of Milky Way globular clusters, halo substructures, and satellite galaxies

Danny Horta, Melissa K. Ness

Stellar atmospheric element abundance ratios of stars retain information about their birth conditions, helping elucidate their origin and nature. In this letter, we analyse and con…

astro-ph.GA2025

Four Elements to Rule Them All: Abundances are Rigidly Coupled in the Milky Way Disk

Jennifer Mead, Rebeca De La Garza, Melissa Ness

Chemical tagging is a central pursuit of galactic archaeology, but requires sufficiently discriminative abundances to uniquely identify sites of star formation. This task is compli…

astro-ph.IM2025

: A generative, multi-output, latent-variable model for astronomical data with noisy labels

Danny Horta, Adrian M. Price-Whelan, David W. Hogg +2

The large volume of spectroscopic data available now and from near-future surveys will enable high-dimensional measurements of stellar parameters and properties. Current methods fo…

astro-ph.EP2025

Exoplanet Occurrence Rate with Age for FGK Stars in Kepler

Maryum Sayeed, Ruth Angus, Travis Berger +5

We measure exoplanet occurrence rate as a function of isochrone and gyrochronology ages using confirmed and candidate planets identified in Q1-17 DR25 Kepler data. We employ Kepler…