A Metallicity Catalog of Very Metal-poor Main-sequence Turn-off and Red Giant Stars from LAMOST DR10

We present a catalog of 8440 candidate very metal-poor (VMP; [Fe/H] ≤ −2.0) main-sequence turn-off (MSTO) and red giant stars in the Milky Way, identified from low-resolution spectra in LAMOST DR10. More than 7000 of these candidates are brighter than G  ∼ 16, making them excellent targets for high-...

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Main Authors: Xiangyu Li, Huiling Chen, Yang Huang, Huawei Zhang, Timothy C. Beers, Linxuan Zhu, Jifeng Liu
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Supplement Series
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Online Access:https://doi.org/10.3847/1538-4365/ade3ca
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author Xiangyu Li
Huiling Chen
Yang Huang
Huawei Zhang
Timothy C. Beers
Linxuan Zhu
Jifeng Liu
author_facet Xiangyu Li
Huiling Chen
Yang Huang
Huawei Zhang
Timothy C. Beers
Linxuan Zhu
Jifeng Liu
author_sort Xiangyu Li
collection DOAJ
description We present a catalog of 8440 candidate very metal-poor (VMP; [Fe/H] ≤ −2.0) main-sequence turn-off (MSTO) and red giant stars in the Milky Way, identified from low-resolution spectra in LAMOST DR10. More than 7000 of these candidates are brighter than G  ∼ 16, making them excellent targets for high-resolution spectroscopic follow-up with 4–10 m class telescopes. Unlike most previous studies, we employed an empirical calibration to estimate metallicities from the equivalent widths of the calcium triplet lines, taking advantage of the high signal-to-noise ratio in the red arm of LAMOST spectra. We further refined this calibration to improve its reliability for more distant stars. This method enables robust identification of VMP candidates with metallicities as low as [Fe/H] = −4.0 among both MSTO and red giant stars. Comparisons with metal-poor samples from other spectroscopic surveys and high-resolution follow-up observations confirm the accuracy of our estimates, showing a typical median offset of ∼0.1 dex and a standard deviation of ∼0.2 dex.
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institution Kabale University
issn 0067-0049
language English
publishDate 2025-01-01
publisher IOP Publishing
record_format Article
series The Astrophysical Journal Supplement Series
spelling doaj-art-15a327aad5e14efc8a9ae08fcbed47b32025-08-20T03:43:58ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492025-01-0127925310.3847/1538-4365/ade3caA Metallicity Catalog of Very Metal-poor Main-sequence Turn-off and Red Giant Stars from LAMOST DR10Xiangyu Li0Huiling Chen1https://orcid.org/0009-0008-2988-2680Yang Huang2https://orcid.org/0000-0003-3250-2876Huawei Zhang3https://orcid.org/0000-0002-7727-1699Timothy C. Beers4https://orcid.org/0000-0003-4573-6233Linxuan Zhu5Jifeng Liu6National Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; huangyang@ucas.ac.cn; School of Astronomy and Space Science, University of Chinese Academy of Sciences , Beijing 100049, People’s Republic of ChinaDepartment of Astronomy, School of Physics, Peking University , Beijing 100871, People’s Republic of China ; zhanghw@pku.edu.cn; Kavli Institute for Astronomy and Astrophysics, Peking University , Beijing 100871, People’s Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; huangyang@ucas.ac.cn; School of Astronomy and Space Science, University of Chinese Academy of Sciences , Beijing 100049, People’s Republic of ChinaDepartment of Astronomy, School of Physics, Peking University , Beijing 100871, People’s Republic of China ; zhanghw@pku.edu.cn; Kavli Institute for Astronomy and Astrophysics, Peking University , Beijing 100871, People’s Republic of ChinaDepartment of Physics and Astronomy and JINA Center for the Evolution of the Elements (JINA-CEE), University of Notre Dame , Notre Dame, IN 46556, USADepartment of Astronomy, School of Physics, Peking University , Beijing 100871, People’s Republic of China ; zhanghw@pku.edu.cn; Kavli Institute for Astronomy and Astrophysics, Peking University , Beijing 100871, People’s Republic of ChinaNational Astronomical Observatories, Chinese Academy of Sciences , Beijing 100101, People’s Republic of China ; huangyang@ucas.ac.cn; School of Astronomy and Space Science, University of Chinese Academy of Sciences , Beijing 100049, People’s Republic of ChinaWe present a catalog of 8440 candidate very metal-poor (VMP; [Fe/H] ≤ −2.0) main-sequence turn-off (MSTO) and red giant stars in the Milky Way, identified from low-resolution spectra in LAMOST DR10. More than 7000 of these candidates are brighter than G  ∼ 16, making them excellent targets for high-resolution spectroscopic follow-up with 4–10 m class telescopes. Unlike most previous studies, we employed an empirical calibration to estimate metallicities from the equivalent widths of the calcium triplet lines, taking advantage of the high signal-to-noise ratio in the red arm of LAMOST spectra. We further refined this calibration to improve its reliability for more distant stars. This method enables robust identification of VMP candidates with metallicities as low as [Fe/H] = −4.0 among both MSTO and red giant stars. Comparisons with metal-poor samples from other spectroscopic surveys and high-resolution follow-up observations confirm the accuracy of our estimates, showing a typical median offset of ∼0.1 dex and a standard deviation of ∼0.2 dex.https://doi.org/10.3847/1538-4365/ade3caChemical abundancesGalaxy stellar contentHalo starsPopulation II stars
spellingShingle Xiangyu Li
Huiling Chen
Yang Huang
Huawei Zhang
Timothy C. Beers
Linxuan Zhu
Jifeng Liu
A Metallicity Catalog of Very Metal-poor Main-sequence Turn-off and Red Giant Stars from LAMOST DR10
The Astrophysical Journal Supplement Series
Chemical abundances
Galaxy stellar content
Halo stars
Population II stars
title A Metallicity Catalog of Very Metal-poor Main-sequence Turn-off and Red Giant Stars from LAMOST DR10
title_full A Metallicity Catalog of Very Metal-poor Main-sequence Turn-off and Red Giant Stars from LAMOST DR10
title_fullStr A Metallicity Catalog of Very Metal-poor Main-sequence Turn-off and Red Giant Stars from LAMOST DR10
title_full_unstemmed A Metallicity Catalog of Very Metal-poor Main-sequence Turn-off and Red Giant Stars from LAMOST DR10
title_short A Metallicity Catalog of Very Metal-poor Main-sequence Turn-off and Red Giant Stars from LAMOST DR10
title_sort metallicity catalog of very metal poor main sequence turn off and red giant stars from lamost dr10
topic Chemical abundances
Galaxy stellar content
Halo stars
Population II stars
url https://doi.org/10.3847/1538-4365/ade3ca
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