activity
20092023
most citedThe First Data Release (DR1) of the LAMOST general survey

862 citations · 2.4k across the 56 of their papers we have counts for

collaborators

56 papers

astro-ph.SR2023★ 4 cited

A Study of Pulsation properties of 57 Non-Blazhko effect ab-type RR Lyrae stars with homogeneous metallicities from the LAMOST-Kepler/K2 survey

Peng Zong, Jian-Ning Fu, Jiaxin Wang +4

Homogeneous metallicities and continuous high-precision light curves play key roles in studying the pulsation properties of RR Lyrae stars. By cross-matching with LAMOST DR6, we ha…

astro-ph.SR2023★ 5 cited

Data Release of the AST3-2 Automatic Survey from Dome A, Antarctica

Xu Yang, Yi Hu, Zhaohui Shang +18

AST3-2 is the second of the three Antarctic Survey Telescopes, aimed at wide-field time-domain optical astronomy. It is located at Dome A, Antarctica, which is by many measures the…

astro-ph.SR2023

The cradle of nonlinear asteroseismology: observations of oscillation mode variability in compact pulsating stars

Weikai Zong, Stéphane Charpinet, Gérard Vauclair +2

We briefly review progress in developing a pathway to nonlinear astereoseismology, both from theoretical and observational aspects. As predicted by the theory of weak nonlinear int…

astro-ph.SR2022★ 11 cited

An Ap star catalog based on LAMOST DR9

Fangfei Shi, Huawei Zhang, Jianning Fu +2

We present a sample of 2700 Ap stars in LAMOST DR9. The candidates are first selected to be in a temperature range typical of Ap stars by using the - color index from Gaia…

astro-ph.SR2022★ 11 cited

Precise Evolutionary Asteroseismology of High-Amplitude δ Scuti Star AE Ursae Majoris

Hui-Fang Xue, Jia-Shu Niu, Jian-Ning Fu

Stellar structure and evolution theory is one of the basis in modern astronomy. Stellar inner structures and their evolutionary states can be precisely tested by asteroseismology,…

astro-ph.IM2022★ 18 cited

ET White Paper: To Find the First Earth 2.0

Jian Ge, Hui Zhang, Weicheng Zang +163

We propose to develop a wide-field and ultra-high-precision photometric survey mission, temporarily named "Earth 2.0 (ET)". This mission is designed to measure, for the first time,…

astro-ph.SR2022★ 12 cited

K2 photometry on oscillation mode variability: the new pulsating hot B subdwarf star EPIC 220422705

Xiao-Yu Ma, Weikai Zong, Jian-Ning Fu +4

We present an analysis of oscillation mode variability in the hot B subdwarf star EPIC~220422705, a new pulsator discovered from ~days of {\em K}2 photometry. The high-qual…

astro-ph.GA2022★ 93 cited

Overview of the LAMOST survey in the first decade

Hongliang Yan, Haining Li, Song Wang +24

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), also known as the Guoshoujing Telescope, is a major national scientific facility for astronomical research l…

astro-ph.SR2022★ 8 cited

The Properties and Evolutions of Starspots on Three Detached Eclipsing Binaries in the LAMOST-Kepler survey

Jiaxin Wang, Jianning Fu, Weikai Zong +4

The spotted detached eclipsing binary (DEB) offers insights into starspots on the binary. Three spotted DEBs, KIC 8097825, KIC 6859813, and KIC 5527172, which were observed by the…

astro-ph.SR2021★ 44 cited

The Spectroscopic Binaries from LAMOST Medium-Resolution Survey (MRS). I. Searching for Double-lined Spectroscopic Binaries (SB2s) with Convolutional Neural Network

Bo Zhang, Ying-Jie Jing, Fan Yang +13

We developed a convolutional neural network (CNN) model to distinguish the double-lined spectroscopic binaries (SB2s) from others based on single exposure medium-resolution spectra…

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★ 7 cited

LTD064402+245919: A Subgiant with a 1-3 M Undetected Companion Identified from LAMOST-TD Data

Fan Yang, Bo Zhang, Richard J. Long +11

Single-line spectroscopic binaries recently contribute to the stellar-mass black hole discovery, independently of the X-ray transient method. We report the identification of a sing…

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★ 5 cited

Discovery of multiple p-mode pulsation frequencies in the roAp star, HD 86181

Fangfei Shi, Donald W. Kurtz, Daniel L. Holdsworth +5

We report the frequency analysis of a known roAp star, HD 86181 (TIC 469246567), with new inferences from TESS data. We derive the rotation frequency to be = 0.48753 $\pm…

astro-ph.SR2021

A triplet of the only pulsation mode detected in the DAV star G132-12

Wen-Chao Su, Jian-Ning Fu, Jian-Xing Chen +5

Hydrogen atmosphere pulsating white dwarfs, also known as DAV stars, are the most abundant type of pulsating white dwarfs. High-temperature DAV stars exhibit in general a small num…

astro-ph.SR2021★ 11 cited

Asteroseismology of RRab variable star EZ Cnc from K2 photometry and LAMOST spectroscopy

Jiangtao Wang, Jianning Fu, Weikai Zong +2

EZ Cnc, or EPIC 212182292, is a non-Blazhko RRab variable star located in the field of K2 Campaign 16. Its atmospheric parameters (, , [M/H]) and radial veloc…

astro-ph.SR2021★ 105 cited

Self-consistent Stellar Radial Velocities from LAMOST Medium-Resolution Survey (MRS) DR7

Bo Zhang, Jiao Li, Fan Yang +12

Radial velocity (RV) is among the most fundamental physical quantities obtainable from stellar spectra and is rather important in the analysis of time-domain phenomena. The LAMOST…

astro-ph.SR2020★ 26 cited

LAMOST Observations in 15 \textit{K}2 Campaigns: I. Low resolution spectra from LAMOST DR6

Jiangtao Wang, Jian-Ning Fu, Weikai Zong +12

The LAMOST-\textit{K}2 (L\textit{K}2) project, initiated in 2015, aims to collect low-resolution spectra of targets in the \textit{K}2 campaigns, similar to LAMOST-\textit{Kepler}…

astro-ph.SR2020★ 59 cited

Most Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy

Hong-Liang Yan, Yu-Tao Zhou, Xianfei Zhang +19

Lithium has confused scientists for decades at almost each scale of the universe. Lithium-rich giants are peculiar stars with lithium abundances over model prediction. A large frac…

astro-ph.SR2020★ 65 cited

Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution spectroscopic observations

Weikai Zong, Jian-Ning Fu, Peter De Cat +20

Phase \RNum{2} of the LAMOST-{\sl Kepler/K}2 survey (LK-MRS), initiated in 2018, aims at collecting medium-resolution spectra (; hereafter MRS) for more than s…

astro-ph.SR2020★ 42 cited

Overview of the LAMOST- project

J. N. Fu, P. De Cat, W. Zong +9

The NASA mission obtained long-term high-quality photometric observations for a large number of stars in its original field of view from 2009 to 2013. In order to provide…

astro-ph.SR2020

Pulsations of the roAp star KIC 10685175 revisited by TESS

Fangfei Shi, Donald Kurtz, Hideyuki Saio +2

KIC 10685175 (TIC 264509538) was discovered to be a rapidly oscillating Ap star from {\it Kepler} long cadence data using super-Nyquist frequency analysis. It was re-observed by TE…

astro-ph.SR2020★ 45 cited

LAMOST Medium-Resolution Spectroscopic Survey (LAMOST-MRS): Scientific goals and survey plan

Chao Liu, Jianning Fu, Jianrong Shi +38

Since September 2018, LAMOST starts a new 5-year medium-resolution spectroscopic survey (MRS) using bright/gray nights. We present the scientific goals of LAMOST-MRS and propose a…