How Robust Is the Cosmic Distance with the Tip of Red Giant Branch against Stellar Population Variations?红巨星支顶端天体测距对星族变化的鲁棒性如何?Astrophysical JournalIF5.42026-05-100PRE
Comparison of the Chemical Compositions between the Bright and Faint Red Clumps for the Metal-poor and Metal-rich Populations in the Milky Way BulgeASTROPHYSICAL JOURNALIF5.42024-12-030OA
Two stellar populations with different metallicities in the low-mass globular cluster Gran 5ASTRONOMY & ASTROPHYSICSIF5.82024-11-270PRE
Chemical Homogeneity of Wide Binary Systems: An Approach from Near-Infrared SpectroscopyASTRONOMICAL JOURNALIF5.12023-12-042OA
High-resolution near-infrared spectroscopy of globular cluster and field stars toward the Galactic bulgeASTRONOMY & ASTROPHYSICSIF5.82022-10-067OA
New Subgrouping of Multiple Stellar Populations in NGC 2808 Based on Low-resolution SpectroscopyASTRONOMICAL JOURNALIF5.12021-09-015OA
Difference in Chemical Composition between the Bright and Faint Red Clump Stars in the Milky Way BulgeASTROPHYSICAL JOURNALIF5.42021-01-2711OA
The CN-CH Positive Correlation in the Globular Cluster NGC 5286ASTROPHYSICAL JOURNALIF5.42017-07-1810OAAI
Corrugation-assisted metal-coated angled fiber facet for wavelength-dependent off-axis directional beamingOPTICS EXPRESSIF3.32017-03-3117OAAI
Three-dimensional infrared models of the interplanetary dust distributionEARTH PLANETS AND SPACEIF2.52014-06-0610OAAI
Brightness map of the zodiacal emission from the AKARI IRC All-Sky SurveyASTRONOMY & ASTROPHYSICSIF5.82010-11-1614OA
Residual gas survey of stainless steel 304 extreme high vacuum chamber with hot cathode ionization gaugeMEASUREMENTIF5.62008-11-0135PREAI