activity
20172024
most citedLithium-rich Giants in LAMOST Survey. I. The Catalog

61 citations · 368 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2024

Stellar atmospheric parameters of 11,000 RR Lyrae stars from LAMOST Spectra

Jiangtao Wang, Jianrong Shi, Jianning Fu +2

Accurate determination of the stellar atmospheric parameters of RR Lyrae stars (RRLs) requires short individual exposures of the spectra to mitigate pulsation effects. We present i…

astro-ph.HE2022★ 21 cited

An X-Ray-dim "Isolated'' Neutron Star in a Binary?

Jie Lin, Chunqian Li, Weiyang Wang +13

We report the discovery of a dark companion to 2MASS J15274848+3536572 with an orbital period of 6.14 hr. Combining the radial velocity from LAMOST observations and modelling of th…

astro-ph.HE2022★ 20 cited

The Nearest Neutron Star Candidate in a Binary Revealed by Optical Time-domain Surveys

Ling-Lin Zheng, Mouyuan Sun, Wei-Min Gu +19

The near-Earth (within pc) supernova explosions in the past several million years can cause the global deposition of radioactive elements (e.g., Fe) on Earth. The…

astro-ph.SR2022★ 12 cited

A White Dwarf-Main Sequence Binary Unveiled by Time-Domain Observations from LAMOST and TESS

Ling-Lin Zheng, Wei-Min Gu, Mouyuan Sun +16

We report a single-lined white dwarf-main sequence binary system, LAMOST J172900.17+652952.8, which is discovered by LAMOST's medium resolution time-domain surveys. The radial velo…

astro-ph.SR2022★ 13 cited

A long-period pre-ELM system discovered from LAMOST medium-resolution survey

Zhi-Xiang Zhang, Ling-Lin Zheng, Wei-Min Gu +16

We present LAMOST~J041920.07+072545.4 (hereafter J0419), a close binary consisting of a bloated extremely low mass pre-white dwarf (pre-ELM WD) and a compact object with an orbital…

astro-ph.SR2022★ 31 cited

A dynamically discovered and characterized non-accreting neutron star -- M dwarf binary candidate

Tuan Yi, Wei-Min Gu, Zhi-Xiang Zhang +26

Optical time-domain surveys can unveil and characterize exciting but less-explored non-accreting and/or non-beaming neutron stars (NS) in binaries. Here we report the discovery of…

astro-ph.SR2022★ 12 cited

Mass-Ratio Distribution of Binaries From the LAMOST-MRS Survey

Jiangdan Li, Jiao Li, Chao Liu +7

Binary evolution leads to the formation of important objects crucial to the development of astrophysics, but the statistical properties of binary populations are still poorly under…

astro-ph.SR2022★ 25 cited

Stellar Atmospheric Parameters of M-type Stars from LAMOST DR8

Ming-Yi Ding, Jian-Rong Shi, Yue Wu +9

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Low Resolution Spectroscopic Survey (LRS) provides massive spectroscopic data of M-type stars, and the derive…

astro-ph.SR2021★ 5 cited

Spot and Facula Activity Variations of the Eccentric Detached Eclipsing Binary KIC 8098300 Based on the Time-series Orbital Solutions

Hubiao Niu, Jianning Fu, Jiaxin Wang +1

The LAMOST spectra and light curves are combined to investigate the detached eclipsing binary KIC 8098300, which shows the O'Connell effect caused by spot/facula modu…

astro-ph.SR2021★ 31 cited

LAMOST Time-Domain Survey: First Results of four 2 plates

Song Wang, Haotong Zhang, Zhongrui Bai +23

From Oct. 2019 to Apr. 2020, LAMOST performs a time-domain spectroscopic survey of four 2 plates with both low- and med-resolution observations. The low-resolution spectroscopic…

astro-ph.SR2021★ 50 cited

Double-, triple-line spectroscopic candidates in the LAMOST Medium-Resolution Spectroscopic Survey

Chun-qian Li, Jian-rong Shi, Hong-liang Yan +3

The LAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS) provides an unprecedented opportunity for detecting multi-line spectroscopic systems. Based on the method of Cross-Co…

astro-ph.SR2021★ 18 cited

Lithium Evolution of Giant Stars Observed by LAMOST and Kepler

Jinghua Zhang, Jian-Rong Shi, Hong-Liang Yan +8

Mapping lithium evolution for evolved stars will provide restrictions and constraints on the fundamental stellar interior physical processes, which further shed light on our unders…

astro-ph.SR2021★ 19 cited

The Lithium Abundances from the Large Sky Area Multi-object Fiber Spectroscopic Telescope Medium-resolution Survey. I. The Method

Qi Gao, Jian-Rong Shi, Hong-Liang Yan +9

Standard stellar evolution model predicts a severe depletion of lithium (Li) abundance during the first dredge-up process (FDU). Yet a small fraction of giant stars are still found…

astro-ph.SR2020★ 11 cited

Searching for r-process-enhanced stars in the LAMOST Survey I: The Method

Tian-Yi Chen, Jian-Rong Shi, Timothy C. Beers +5

The abundance patterns of -process-enhanced stars contain key information required to constrain the astrophysical site(s) of -process nucleosynthesis, and to deepen our under…

astro-ph.SR2019★ 61 cited

Lithium-rich Giants in LAMOST Survey. I. The Catalog

Qi Gao, Jian-Rong Shi, Hong-Liang Yan +5

Standard stellar evolution model predicts a severe depletion of lithium (Li) abundance during the first dredge up process (FDU). Yet a small fraction of giant stars are still found…

astro-ph.SR2019★ 31 cited

Exploring the spectral \textit{information content} in the LAMOST medium-resolution survey (MRS)

Bo Zhang, Chao Liu, Chun-Qian Li +3

Low-resolution spectra are proved competitive to high-resolution spectra in determining many stellar labels at comparable precision. It is useful to consider the spectral informati…

astro-ph.SR2017★ 8 cited

New ZZ Ceti stars from the LAMOST survey

Jie Su, Jianning Fu, Guifang Lin +3

The spectroscopic sky survey carried out by the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) provides the largest stellar spectra library in the world until n…