TY - JOUR
T1 - The GALAH plus survey
T2 - Third data release
AU - GALAH collaboration
AU - Buder, Sven
AU - Sharma, Sanjib
AU - Kos, Janez
AU - Amarsi, Anish M.
AU - Nordlander, Thomas
AU - Lind, Karin
AU - Martell, Sarah L.
AU - Asplund, Martin
AU - Bland-Hawthorn, Joss
AU - Casey, Andrew R.
AU - De Silva, Gayandhi M.
AU - D'Orazi, Valentina
AU - Freeman, Ken C.
AU - Hayden, Michael R.
AU - Lewis, Geraint F.
AU - Lin, Jane
AU - Schlesinger, Katharine J.
AU - Simpson, Jeffrey D.
AU - Stello, Dennis
AU - Zucker, Daniel B.
AU - Zwitter, Tomaž
AU - Beeson, Kevin L.
AU - Buck, Tobias
AU - Casagrande, Luca
AU - Clark, Jake T.
AU - Čotar, Klemen
AU - Da Costa, Gary S.
AU - de Grijs, Richard
AU - Feuillet, Diane
AU - Horner, Jonathan
AU - Kafle, Prajwal R.
AU - Khanna, Shourya
AU - Kobayashi, Chiaki
AU - Liu, Fan
AU - Montet, Benjamin T.
AU - Nandakumar, Govind
AU - Nataf, David M.
AU - Ness, Melissa K.
AU - Spina, Lorenzo
AU - Tepper-García, Thor
AU - Ting, Yuan-Sen
AU - Traven, Gregor
AU - Vogrinčič, Rok
AU - Wittenmyer, Robert A.
AU - Wyse, Rosemary F. G.
AU - Žerjal, Maruša
N1 - This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, Volume 506, Issue 1, September 2021, Pages 150–201, https://doi.org/10.1093/mnras/stab1242. Copyright 2021 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
PY - 2021/9
Y1 - 2021/9
N2 - The ensemble of chemical element abundance measurements for stars, along with precision distances and orbit properties,
provides high-dimensional data to study the evolution of the Milky Way. With this third data release of the Galactic Archaeology
with HERMES (GALAH) survey, we publish 678 423 spectra for 588 571 mostly nearby stars (81.2 per cent of stars are within
<2 kpc), observed with the HERMES spectrograph at the Anglo-Australian Telescope. This release (hereafter GALAH+ DR3)
includes all observations from GALAH Phase 1 (bright, main, and faint survey, 70 per cent), K2-HERMES (17 per cent),
TESS-HERMES (5 per cent), and a subset of ancillary observations (8 per cent) including the bulge and >75 stellar clusters.
We derive stellar parameters Teff, log g, [Fe/H], vmic, vbroad, and vrad using our modified version of the spectrum synthesis
code Spectroscopy Made Easy (SME) and 1D MARCS model atmospheres. We break spectroscopic degeneracies in our spectrum
analysis with astrometry from Gaia DR2 and photometry from 2MASS. We report abundance ratios [X/Fe] for 30 different
elements (11 of which are based on non-LTE computations) covering five nucleosynthetic pathways. We describe validations
for accuracy and precision, flagging of peculiar stars/measurements and recommendations for using our results. Our catalogue
comprises 65 per cent dwarfs, 34 per cent giants, and 1 per cent other/unclassified stars. Based on unflagged chemical composition
and age, we find 62 per cent young low-α, 9 per cent young high-α, 27 per cent old high-α, and 2 per cent stars with [Fe/H]
≤ −1. Based on kinematics, 4 per cent are halo stars. Several Value-Added-Catalogues, including stellar ages and dynamics,
updated after Gaia eDR3, accompany this release and allow chrono-chemodynamic analyses, as we showcase.
AB - The ensemble of chemical element abundance measurements for stars, along with precision distances and orbit properties,
provides high-dimensional data to study the evolution of the Milky Way. With this third data release of the Galactic Archaeology
with HERMES (GALAH) survey, we publish 678 423 spectra for 588 571 mostly nearby stars (81.2 per cent of stars are within
<2 kpc), observed with the HERMES spectrograph at the Anglo-Australian Telescope. This release (hereafter GALAH+ DR3)
includes all observations from GALAH Phase 1 (bright, main, and faint survey, 70 per cent), K2-HERMES (17 per cent),
TESS-HERMES (5 per cent), and a subset of ancillary observations (8 per cent) including the bulge and >75 stellar clusters.
We derive stellar parameters Teff, log g, [Fe/H], vmic, vbroad, and vrad using our modified version of the spectrum synthesis
code Spectroscopy Made Easy (SME) and 1D MARCS model atmospheres. We break spectroscopic degeneracies in our spectrum
analysis with astrometry from Gaia DR2 and photometry from 2MASS. We report abundance ratios [X/Fe] for 30 different
elements (11 of which are based on non-LTE computations) covering five nucleosynthetic pathways. We describe validations
for accuracy and precision, flagging of peculiar stars/measurements and recommendations for using our results. Our catalogue
comprises 65 per cent dwarfs, 34 per cent giants, and 1 per cent other/unclassified stars. Based on unflagged chemical composition
and age, we find 62 per cent young low-α, 9 per cent young high-α, 27 per cent old high-α, and 2 per cent stars with [Fe/H]
≤ −1. Based on kinematics, 4 per cent are halo stars. Several Value-Added-Catalogues, including stellar ages and dynamics,
updated after Gaia eDR3, accompany this release and allow chrono-chemodynamic analyses, as we showcase.
KW - methods: data analysis
KW - methods: observational
KW - surveys
KW - stars: abundances
KW - stars: fundamental parameters
U2 - 10.1093/mnras/stab1242
DO - 10.1093/mnras/stab1242
M3 - Article
VL - 506
SP - 150
EP - 201
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
SN - 1365-2966
IS - 1
ER -