MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project: I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby starsASTRONOMY & ASTROPHYSICSIF5.82025-01-150OA
[N I] 10400/10410 Å Lines as Possible Disk Wind Tracers in a Young Intermediate-mass StarASTROPHYSICAL JOURNALIF5.42024-04-080OA
The globular cluster VVV CL002 falling down to the hazardous Galactic centreASTRONOMY & ASTROPHYSICSIF5.82024-03-159OA
A High-resolution Non-detection of Escaping Helium in the Ultrahot Neptune LTT 9779b: Evidence for Weakened EvaporationASTROPHYSICAL JOURNAL LETTERSIF11.72024-02-081OA
WARP: The Data Reduction Pipeline for the WINERED SpectrographPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFICIF7.72024-02-014OA
Shock Excitation in Narrow-line Regions Powered by AGN OutflowsASTROPHYSICAL JOURNALIF5.42023-12-213OA
Metallicities of Classical Cepheids in the Inner Galactic DiskASTROPHYSICAL JOURNALIF5.42023-09-077OA
Star Formation Activity beyond the Outer Arm. II. Distribution and Properties of Star FormationASTROPHYSICAL JOURNALIF5.42022-09-132OA
Survey of Near-infrared Diffuse Interstellar Bands in Y and J Bands. I. Newly Identified BandsASTROPHYSICAL JOURNAL SUPPLEMENT SERIESIF8.52022-08-1710OA
Effective temperatures of red supergiants estimated from line-depth ratios of iron lines in the YJ bands, 0.97-1.32 μm (vol 502, pg 4210, 2021)MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82022-03-290OA
A Very Metal-poor RR Lyrae Star with a Disk Orbit Found in the Solar NeighborhoodASTROPHYSICAL JOURNALIF5.42022-01-204OA
Highly Sensitive, Non-cryogenic NIR High-resolution Spectrograph, WINEREDPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFICIF7.72022-01-1118OA
Absorption Lines in the 0.91-1.33 μm Spectra of Red Giants for Measuring Abundances of Mg, Si, Ca, Ti, Cr, and NiASTROPHYSICAL JOURNALIF5.42021-05-258OA
Mg ii and Fe ii Fluxes of Luminous Quasars at z ∼ 2.7 and the Evaluation of the Baldwin Effect in the Flux-to-abundance Conversion Method for QuasarsASTROPHYSICAL JOURNALIF5.42020-12-0111OA
The effect of surface gravity on line-depth ratios in the wavelength range 0.97-1.32 μmMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82020-04-039OAAI
Effective temperatures of red supergiants estimated from line-depth ratios of iron lines in the YJ bands, 0.97-1.32 μmMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYIF4.82020-02-2815OAAI
Identification of Absorption Lines of Heavy Metals in the Wavelength Range 0.97-1.32 μmASTROPHYSICAL JOURNAL SUPPLEMENT SERIESIF8.52020-01-089OAAI
Possible Progression of Mass-flow Processes around Young Intermediate-mass Stars Based on High-resolution Near-infrared Spectroscopy. I. TaurusASTROPHYSICAL JOURNALIF5.42019-11-275OA
First Detection of A-X (0,0) Bands of Interstellar C2 and CN星际C2和CN的A-X (0,0) 带的首次检测ASTROPHYSICAL JOURNALIF5.42019-08-228OAAI
WINERED High-resolution Near-infrared Line Catalog: A-type StarASTROPHYSICAL JOURNAL SUPPLEMENT SERIESIF8.52018-11-262OAAI
个人简介
教育背景
工作经历
荣誉奖项
未登录.png){kind=icon}
未登录个人简介教育背景工作经历荣誉奖项
研究方向