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20112026
most citedFour-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances

120 citations · 946 across the 56 of their papers we have counts for

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astro-ph.SR2026

Long-term high-resolution spectroscopic monitoring of the evolved metal-poor binary PS Gem

V. G. Klochkova, V. E. Panchuk, J. K. Zhao +3

We present results of long-term high-resolution spectroscopic monitoring of the extremely low-metallicity star PS Gem (=HD 52961), associated with IRAS 07008+1050. The spectra were…

astro-ph.SR2026

Probabilistic Stellar Age Estimation for Gaia XP Stars with NGBoost

Xiaokun Hou, Wenbo Wu, Gang Zhao +2

Stellar age is a fundamental quantity for Galactic archaeology, but reliable age estimation for large stellar samples remains challenging. In this work, we develop an uncertainty a…

astro-ph.SR2026

A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to dex. II. Lithium Abundance and New Insight to the Lithium Plateau

Hong-Liang Yan, Jinxiao Qin, Shuai Liu +12

Metal-poor stars are crucially important for understanding the early Galaxy, first stars, and the Universe. In this series of papers, we present a homogeneous non-local thermodynam…

astro-ph.SR2026

The Stellar Abundances and Galactic Evolution Survey (SAGES). V. The First Data Release of the DDO51 Band

Qiqian Zhang, Zhou Fan, Gang Zhao +20

We present the first public data release of DDO51 band from the Stellar Abundances and Galactic Evolution Survey (SAGES), based on Nanshan One-meter Wide-field Telescope (NOWT) obs…

astro-ph.SR2026

Revisiting Ca II Activity Indices in FGK Stars: Systematic Biases in Infrared Triplet Measurements

Xiaozhen Yang, Xiaoting Fu, Mingjie Jian +10

Synthetic-template subtraction is widely used to measure chromospheric activity in large spectroscopic surveys. However, many solar-like FGK stars show systematically negative Ca I…

astro-ph.SR2026

A Highly Magnetic Ultra Massive White Dwarf with a 23-minute Rotation Period

Jincheng Guo, Xiaofeng Wang, Qichun Liu +17

We present a physical characterization of TMTS J00063798+3104160 (J0006), a rapidly rotating,ultra-massive white dwarf (WD) identified in high-cadence light curves from the Tsinghu…

astro-ph.SR2025

Looking for Signs of Unresolved Binarity in the Continuum of LAMOST Stellar Spectra

Mikhail Prokhorov, Kefeng Tan, Nikolay Samus +10

We describe an attempt to derive the binarity rate of samples of 166 A-, F-, G-, and K-type stars from LAMOST DR5 and 1000 randomly selected presumably single stars from Gaia DR3 c…

astro-ph.SR2024

Variable white dwarfs in TMTS: Asteroseismological analysis of a ZZ Ceti star, TMTS J17184064+2524314

Jincheng Guo, Yanhui Chen, Yonghui Yang +24

The Tsinghua University-Ma Huateng Telescope for Survey (TMTS) has been constantly monitoring the northern sky since 2020 in search of rapidly variable stars. To find variable whit…

astro-ph.SR2023★ 13 cited

Mass distribution for single-lined hot subdwarf stars in LAMOST

Zhenxin Lei, Ruijie He, Peter Nemeth +4

Masses for 664 single-lined hot subdwarf stars identified in LAMOST were calculated by comparing synthetic fluxes from spectral energy distribution (SED) with observed fluxes from…

astro-ph.SR2023★ 8 cited

Properties and Asteroseismological analysis of a new ZZ ceti discovered by TMTS

Jincheng Guo, Yanhui Chen, Xiaofeng Wang +24

Tsinghua university-Ma Huateng Telescope for Survey (TMTS) aims to discover rapidly evolving transients by monitoring the northern sky. The TMTS catalog is cross-matched with the w…

astro-ph.SR2022★ 30 cited

Hot subdwarf stars identified in LAMOST DR8 with single-lined and composite spectra

Zhenxin Lei, Ruijie He, Peter Nemeth +6

222 hot subdwarf stars were identified with LAMOST DR8 spectra, among which 131 stars show composite spectra and have been decomposed, while 91 stars present single-lined spectra.…

astro-ph.SR2022★ 120 cited

Four-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances

Haining Li, Wako Aoki, Tadafumi Matsuno +9

We present homogeneous abundance analysis of over 20 elements for 385 very metal-poor (VMP) stars based on the LAMOST survey and follow-up observations with the Subaru Telescope. I…

astro-ph.SR2022★ 29 cited

Four-hundred Very Metal-poor Stars studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency

Wako Aoki, Haining Li, Tadafumi Matsuno +11

The chemical abundances of very metal-poor stars provide important constraints on the nucleosynthesis of the first generation of stars and early chemical evolution of the Galaxy. W…

astro-ph.SR2021★ 16 cited

White dwarfs identified in LAMOST Data Release 5

Jincheng Guo, Jingkun Zhao, Huawei Zhang +5

In this paper, we report white dwarfs identified in the 5th Data Release of the Large Area Multi-Object fibre Spectroscopic Telescope, including spectral types of DA, DB, DC, DZ, a…

astro-ph.SR2020★ 24 cited

Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances

Tadafumi Matsuno, Wako Aoki, Luca Casagrande +9

We combine asteroseismology, optical high-resolution spectroscopy, and kinematic analysis for 26 halo red giant branch stars in the \textit{Kepler} field in the range of $-2.5<[\ma…

astro-ph.SR2016★ 67 cited

Stellar activity with LAMOST. I. Spot configuration in Pleiades

Xiang-Song Fang, Gang Zhao, Jing-Kun Zhao +2

We use the spectra of Pleiades and field stars from LAMOST DR2 archive to study how spottedness and activity vary as a function of mass at young ages. We obtained standard TiO band…

astro-ph.SR2014★ 17 cited

Three Moving Groups Detected in the LAMOST DR1 Archive

Jingkun Zhao, Gang Zhao, Yuqin Chen +3

We analyze the kinematics of thick disk and halo stars observed by the Large sky Area Multi-Object Fiber Spectroscopic Telescope. We have constructed a sample of 7,993 F, G and K n…

astro-ph.SR2013★ 23 cited

White dwarf-main sequence binaries identified from the LAMOST pilot survey

Juanjuan Ren, Ali Luo, Yinbi Li +5

We present a set of white dwarf-main sequence (WDMS) binaries identified spectroscopically from the Large sky Area Multi-Object fiber Spectroscopic Telescope (LAMOST, also called t…

astro-ph.SR2013★ 49 cited

M dwarf catalog of LAMOST pilot survey

Z. P. Yi, A. L. Luo, Y. H. Song +17

We present a spectroscopic catalog of 67082 M dwarfs from the LAMOST pilot survey. For each spectrum of the catalog, spectral subtype, radial velocity, equivalent width of H, a…

astro-ph.SR2013★ 33 cited

72 DA White Dwarfs Identified in LAMOST Pilot Survey

J. K. Zhao, A. L. Luo, T. D. Oswalt +1

We present a spectroscopically identified catalogue of 72 DA white dwarfs from the LAMOST pilot survey. 35 are found to be new identifications after cross-correlation with the Eise…

astro-ph.SR2013★ 21 cited

Tracers of chromospheric structure. I. CaII HK emission distribution of 13000 F, G and K stars in SDSS DR7 spectroscopic sample

J. K. Zhao, T. D. Oswalt, G. Zhao +3

We present chromospheric activity index measurements for over 13,000 F, G and K disk stars with high signal-to-noise ratio ( 60) spectra in the Sloan Digital Sky Sur…

astro-ph.SR2011★ 58 cited

The Initial-Final Mass Relation among White Dwarfs in Wide Binaries

Jingkun Zhao, Terry D. Oswalt, Lee Anne Willson +2

We present the initial-final mass relation derived from 10 white dwarfs in wide binaries that consist of a main sequence star and a white dwarf. The temperature and gravity of each…

astro-ph.SR2011★ 4 cited

Fragile Binary Candidates in the SDSS DR8 spectroscopic archive

Jingkun Zhao, Terry D. Oswalt, Gang Zhao

We present a catalog of 80 very wide fragile binary candidates (projected separations > 10000 AU) from the SDSS DR8 spectral archive. The pairs were selected based on proper motion…

astro-ph.SR2011★ 10 cited

Metallicity and Kinematic distributions of Red Horizontal-Branch Stars from the SDSS Survey

Y. Q. Chen, G. Zhao, J. K. Zhao +2

On the basis of a recently derived color-metallicity relation and stellar parameters from the Sloan Digtal Sky Survey Data Release 7 spectroscopic survey, a large sample of red hor…