Combined APOGEE-GALAH stellar catalogues using the Cannon

Govind Nandakumar*, Michael R. Hayden, Sanjib Sharma, Sven Buder, Martin Asplund, Joss Bland-Hawthorn, Gayandhi M. De Silva, Valentina D'orazi, Ken C. Freeman, Janez Kos, Geraint F. Lewis, Sarah L. Martell, Katharine J. Schlesinger, Jane Lin, Jeffrey D. Simpson, Daniel B. Zucker, Tomaž Zwitter, Thomas Nordlander, Luca Casagrande, Karin LindKlemen Côtar, Dennis Stello, Robert A. Wittenmyer, Thor Tepper-Garcia

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

10 Citations (Scopus)
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Abstract

APOGEE and GALAH are two high resolution multi-object spectroscopic surveys that provide fundamental stellar parameters and multiple elemental abundance estimates for about half a million stars in the Milky Way. Both surveys observe in different wavelength regimes and use different data reduction pipelines leading to significant offsets and trends in stellar parameters and abundances for the common stars observed in both surveys. Such systematic differences/offsets in stellar parameters and abundances make it difficult to effectively utilize them to investigate Galactic abundance trends in spite of the unique advantage provided by their complementary sky coverage and different Milky Way components they observe. Hence, we use the Cannon data-driven method selecting a training set of 4418 common stars observed by both surveys. This enables the construction of two catalogues, one with the APOGEE-scaled and the other with the GALAH-scaled stellar parameters. Using repeat observations in APOGEE and GALAH, we find high precision in metallicity (∼0.02-0.4 dex) and alpha abundances (∼0.02-0.03 dex) for spectra with good signal-to-noise ratio (SNR > 80 for APOGEE and SNR > 40 for GALAH). We use open and globular clusters to validate our parameter estimates and find small scatter in metallicity (0.06 dex) and alpha abundances (0.03 dex) in APOGEE-scaled case. The final catalogues have been cross-matched with the Gaia EDR3 catalogue to enable their use to carry out detailed chemo-dynamic studies of the Milky Way from perspectives of APOGEE and GALAH.

Original languageEnglish
Pages (from-to)232-255
Number of pages24
JournalMonthly Notices of the Royal Astronomical Society
Volume513
Issue number1
DOIs
Publication statusPublished - Jun 2022

Bibliographical note

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2022 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Keywords

  • surveys
  • stars: abundances
  • Galaxy: disc
  • Galaxy: evolution
  • Galaxy: formation
  • Galaxy: structure

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