The GALAH Survey

second data release

Sven Buder, Martin Asplund, Ly Duong, Janez Kos, Karin Lind, Melissa K. Ness, Sanjib Sharma, Joss Bland-Hawthorn, Andrew R. Casey, Gayandhi M. De Silva, Valentina D'Orazi, Ken C. Freeman, Geraint F. Lewis, Jane Lin, Sarah L. Martell, Katharine J. Schlesinger, Jeffrey D. Simpson, Daniel B. Zucker, Tomaž Zwitter, Anish M. Amarsi & 24 others Borja Anguiano Jimenez, Daniela Carollo, Luca Casagrande, Klemen Čotar, Peter L. Cottrell, Gary Da Costa, Xudong D. Gao, Michael R. Hayden, Jonathan Horner, Michael Ireland, Prajwal R. Kafle, Ulisse Munari, David M. Nataf, Thomas Nordlander, Dennis Stello, Yuan-Sen Ting, Gregor Traven, Fred Watson, Robert A. Wittenmyer, Rosemary F. G. Wyse, David Yong, Joel C. Zinn, Maruša Žerjal, GALAH collaboration

Research output: Contribution to journalArticle

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Abstract

The Galactic Archaeology with HERMES (GALAH) survey is a large-scale stellar spectroscopic survey of the Milky Way, designed to deliver complementary chemical information to a large number of stars covered by the Gaia mission. We present the GALAH second public data release (GALAH DR2) containing 342 682 stars. For these stars, the GALAH collaboration provides stellar parameters and abundances for up to 23 elements to the community. Here we present the target selection, observation, data reduction, and detailed explanation of how the spectra were analysed to estimate stellar parameters and element abundances. For the stellar analysis, we have used a multistep approach. We use the physics-driven spectrum synthesis of Spectroscopy Made Easy (SME) to derive stellar labels (Teff, log g, [Fe/H], [X/Fe], vmic, vsin i, Aks) for a representative training set of stars. This information is then propagated to the whole sample with the data-driven method of The Cannon. Special care has been exercised in the spectral synthesis to only consider spectral lines that have reliable atomic input data and are little affected by blending lines. Departures from local thermodynamic equilibrium (LTE) are considered for several key elements, including Li, O, Na, Mg, Al, Si, and Fe, using 1D MARCS stellar atmosphere models. Validation tests including repeat observations, Gaia benchmark stars, open and globular clusters, and K2 asteroseismic targets lend confidence to our methods and results. Combining the GALAH DR2 catalogue with the kinematic information from Gaia will enable a wide range of Galactic Archaeology studies, with unprecedented detail, dimensionality, and scope.
Original languageEnglish
Pages (from-to)4513-4552
Number of pages40
JournalMonthly Notices of the Royal Astronomical Society
Volume478
Issue number4
DOIs
Publication statusPublished - 21 Aug 2018

Bibliographical note

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, Volume 478, Issue 4, 21 August 2018, Pages 4513–4552, https://doi.org/10.1093/mnras/sty1281. Copyright 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Keywords

  • Surveys
  • the Galaxy
  • methods: observational
  • methods: data analysis
  • stars: fundamental parameters
  • stars: abundances

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