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20152025
most citedThe GALAH Survey: Scientific Motivation

839 citations · 3k across the 34 of their papers we have counts for

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astro-ph.SR201591 cited

Nucleosynthesis in a Primordial Supernova: Carbon and Oxygen Abundances in SMSS J031300.36-670839.31

Michael Bessell, Remo Collett, Stefan Keller +15

SMSS J031300.36-670839.3 (hereafter SM0313-6708) is a sub-giant halo star, with no detectable Fe lines and large overabundances of C and Mg relative to Ca. We obtained VLT-UVES spe…

astro-ph.SR2015110 cited

Mg line formation in late-type stellar atmospheres: I. The model atom

Y. Osorio, P. S. Barklem, K. Lind +4

Mg is often traced in late-type stars using lines of neutral magnesium, which is expected to be subject to departures from LTE. The astrophysical importance of Mg as well as its re…

astro-ph.GA201566 cited

The Gaia-ESO Survey: a quiescent Milky Way with no significant dark/stellar accreted disc

G. R. Ruchti, J. I. Read, S. Feltzing +26

According to our current cosmological model, galaxies like the Milky Way are expected to experience many mergers over their lifetimes. The most massive of the merging galaxies will…

astro-ph.SR2015132 cited

High-Resolution Spectroscopic Study of Extremely Metal-Poor Star Candidates from the SkyMapper Survey

Heather. R. Jacobson, Stefan Keller, Anna Frebel +13

The SkyMapper Southern Sky Survey is carrying out a search for the most metal-poor stars in the Galaxy. It identifies candidates by way of its unique filter set that allows for est…

astro-ph.GA2015839 cited

The GALAH Survey: Scientific Motivation

G. M. De Silva, K. C. Freeman, J. Bland-Hawthorn +44

The GALAH survey is a large high-resolution spectroscopic survey using the newly commissioned HERMES spectrograph on the Anglo-Australian Telescope. The HERMES spectrograph provide…

astro-ph.SR201556 cited

The Gaia-ESO Survey: A globular cluster escapee in the Galactic halo

K. Lind, S. E. Koposov, C. Battistini +37

A small fraction of the halo field is made up of stars that share the light element (Z<=13) anomalies characteristic of second generation globular cluster (GC) stars. The ejected s…