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

105 citations · 172 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020105 cited

The GALAH Survey: Non-LTE departure coefficients for large spectroscopic surveys

A. M. Amarsi, K. Lind, Y. Osorio +23

Massive sets of stellar spectroscopic observations are rapidly becoming available and these can be used to determine the chemical composition and evolution of the Galaxy with unpre…

astro-ph.EP202010 cited

K2-HERMES II. Planet-candidate properties from K2 Campaigns 1-13

Robert A. Wittenmyer, Jake T. Clark, Sanjib Sharma +22

Accurate and precise radius estimates of transiting exoplanets are critical for understanding their compositions and formation mechanisms. To know the planet, we must know the host…

astro-ph.SR201924 cited

The GALAH Survey: Temporal Chemical Enrichment of the Galactic Disk

Jane Lin, Martin Asplund, Yuan-Sen Ting +22

We present isochrone ages and initial bulk metallicities (, by accounting for diffusion) of 163,722 stars from the GALAH Data Release 2, mainly composed of main…

astro-ph.GA201926 cited

The GALAH Survey: Chemically tagging the Fimbulthul stream to the globular cluster Centauri

Jeffrey D. Simpson, Sarah L. Martell, Gary Da Costa +17

Using kinematics from Gaia and the large elemental abundance space of the second data release of the GALAH survey, we identify two new members of the Fimbulthul stellar stream, and…

astro-ph.SR2019

The 2018 eruption and long term evolution of the new high-mass Herbig Ae/Be object Gaia-18azl = VES 263

U. Munari, V. Joshi, D. P. K. Banerjee +9

We have been monitoring, at high cadence, the photometric and spectroscopic evolution of VES 263 following the discovery in 2018 of a brightening labeled as event Gaia-18azl. VES 2…

astro-ph.SR20197 cited

The GALAH survey: unresolved triple Sun-like stars discovered by the Gaia mission

Klemen Čotar, Tomaž Zwitter, Gregor Traven +16

The latest Gaia data release enables us to accurately identify stars that are more luminous than would be expected on the basis of their spectral type and distance. During an inves…