activity
20092025
most citedThe GALAH Survey: Scientific Motivation

839 citations · 12.5k across the 128 of their papers we have counts for

collaborators

126 papers

astro-ph.GA2025★ 5 cited

The GALAH survey: Improving chemical abundances using star clusters

Janez Kos, Sven Buder, Kevin L. Beeson +18

Large spectroscopic surveys aim to consistently compute stellar parameters of very diverse stars while minimizing systematic errors. We explore the use of stellar clusters as bench…

astro-ph.GA2024★ 20 cited

The GALAH survey: Tracing the Milky Way's formation and evolution through RR Lyrae stars

Valentina D'Orazi, Nicholas Storm, Andrew R. Casey +39

Stellar mergers and accretion events have been crucial in shaping the evolution of the Milky Way (MW). These events have been dynamically identified and chemically characterised us…

astro-ph.GA2023★ 10 cited

Tidal debris from Omega Centauri discovered with unsupervised machine learning

Kris Youakim, Karin Lind, Iryna Kushniruk

The gravitational interactions between the Milky Way and in-falling satellites offer a wealth of information about the formation and evolution of our Galaxy. In this paper, we expl…

astro-ph.SR2023★ 50 cited

The Gaia-ESO Survey: homogenisation of stellar parameters and elemental abundances

A. Hourihane, P. Francois, C. C. Worley +59

The Gaia-ESO Survey is a public spectroscopic survey that has targeted stars covering all major components of the Milky Way from the end of 2011 to 2018, delivering i…

astro-ph.SR2023★ 18 cited

Raising the observed metallicity floor with a 3D non-LTE analysis of SDSS J102915.14+172927.9

C. Lagae, A. M. Amarsi, L. F. Rodríguez Díaz +4

Context: The first stars produced the first heavy elements and set the stage for the formation of the first galaxies. Accurate chemical abundances of ultra metal-poor stars ([Fe/H]…

astro-ph.IM2023★ 6 cited

Automatic line selection for abundance determination in large stellar spectroscopic surveys

Georges Kordopatis, Vanessa Hill, Karin Lind

*Context: The optimisation of new multiplex spectrographs (resolution, wavelength range,...), their associated surveys (choice of setup), or their parameterisation pipelines requir…