activity
20182026
most citedThe GALAH Survey: Non-LTE departure coefficients for large spectroscopic surveys

105 citations · 298 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2026★ 5 cited

Magnesium isotope ratios in Milky Way and dwarf galaxy stars

M. McKenzie, S. Monty, D. Yong +8

Under the assumption of hierarchical galaxy formation, dwarf galaxies are the closest existing analogues to the high-redshift protogalaxies that merged to form the Milky Way. These…

astro-ph.GA2026★ 3 cited

The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios

M. McKenzie, D. Yong, A. I. Karakas +8

The complex star cluster M 22 (NGC 6656) provides a unique opportunity for studying slow neutron-capture (s-process) nucleosynthesis at low metallicity due to its two stellar group…

astro-ph.GA2026★ 30 cited

The complex stellar system M 22: confirming abundance variations with high precision differential measurements

M. McKenzie, D. Yong, A. F. Marino +8

M 22 (NGC 6656) is a chemically complex globular cluster-like system reported to harbour heavy element abundance variations. However, the extent of these variations and the origin…

astro-ph.IM2026

PySME v1.0: improved modelling of stellar spectra for survey-scale applications

Mingjie Jian, Nikolai Piskunov, Jeff Valenti +4

Stellar abundance analysis relies on flexible, high-performance spectral synthesis. To meet these needs, we present PySME v1.0, an updated Python implementation of Spectroscopy Mad…

astro-ph.SR2026

3D NLTE Sodium abundances in late-type stars. Abundance corrections and synthetic spectra

G. Canocchi, E. X. Wang, A. M. Amarsi +2

Neutral sodium is an important tracer of the Galactic chemical evolution, a powerful diagnostic of different stellar populations, and the subject of detailed studies of exoplanet a…

astro-ph.SR2025

Optical spectroscopic signatures of the red giant evolutionary state

Ella Xi Wang, Melissa Ness, Thomas Nordlander +17

Modern spectroscopic surveys output large data volumes. Theoretical models provide a means to transform the information encoded in these data to measurements of physical stellar pr…