Myung Gyoon Lee
0000-0003-2713-6744
Seoul National University
19 papers found
Refreshing results…
Calibration of the Tip of the Red Giant Branch
The Carnegie-Chicago Hubble Program. VII. The Distance to M101 via the Optical Tip of the Red Giant Branch Method
The Next Generation Virgo Cluster Survey. XVII. A Search for Planetary Nebulae in Virgo Cluster Globular Clusters
The Carnegie Chicago Hubble Program. VI. Tip of the Red Giant Branch Distances to M66 and M96 of the Leo I Group
The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
A Wide-field Photometric Survey of Globular Clusters in the Peculiar Early-type Galaxy M85
The Carnegie-Chicago Hubble Program: Calibration of the Near-infrared RR Lyrae Period–Luminosity Relation with HST
The Carnegie–Chicago Hubble Program. V. The Distances to NGC 1448 and NGC 1316 via the Tip of the Red Giant Branch
The Carnegie-Chicago Hubble Program. IV. The Distance to NGC 4424, NGC 4526, and NGC 4356 via the Tip of the Red Giant Branch
Gemini/GMOS Spectroscopy of Globular Clusters in the Merger Remnant Galaxy M85
The Carnegie–Chicago Hubble Program. III. The Distance to NGC 1365 via the Tip of the Red Giant Branch
Optical and Near-infrared Polarimetry of Non-periodic Comet C/2013 US10 (Catalina)
The Carnegie-Chicago Hubble Program. II. The Distance to IC 1613: The Tip of the Red Giant Branch and RR Lyrae Period–luminosity Relations
New Observational Evidence of Active Asteroid P/2010 A2: Slow Rotation of the Largest Fragment
Erratum: “Optical Spectroscopy of Supernova Remnants in M81 AND M82” (2015, ApJ, 804, 63)
To the Edge of M87 and Beyond: Spectroscopy of Intracluster Globular Clusters and Ultracompact Dwarfs in the Virgo Cluster
The Carnegie-Chicago Hubble Program. I. An Independent Approach to the Extragalactic Distance Scale Using Only Population Ii Distance Indicators
Catalogs of Compact Groups of Galaxies From the Enhanced Sdss Dr12
The Mass Profile and Shape of Bars in the Spitzer Survey of Stellar Structure in Galaxies (S4g): Search for an Age Indicator for Bars
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