Min Yun
educated at: Harvard University
occupation: researcher
Works 8
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ALMA 26 arcmin2 Survey of GOODS-S at One-millimeter (ASAGAO): X-Ray AGN Properties of Millimeter-selected Galaxies
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ALMA Deep Field in SSA22: Source Catalog and Number Counts
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AzTEC/ASTE 1.1-mm survey of SSA22: Counterpart identification and photometric redshift survey of submillimetre galaxies
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AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts and evidence for large-scale structure
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AzTEC millimetre survey of the COSMOS field - III. Source catalogue over 0.72 deg2 and plausible boosting by large-scale structure
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Deep 1.1 mm-wavelength imaging of the GOODS-S field by AzTEC/ASTE - I. Source catalogue and number counts
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AzTEC half square degree survey of the SHADES fields â I. Maps, catalogues and source counts
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An AzTEC 1.1 mm survey of the GOODS-N field - I. Maps, catalogue and source statistics
Articles 139
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Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies
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Possible Ongoing Merger Discovered by Photometry and Spectroscopy in the Field of the Galaxy Cluster PLCK G165.7+67.0
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An Assessment of the In Situ Growth of the Intracluster Light in the High-redshift Galaxy Cluster SpARCS1049+56
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PASSAGES: the Large Millimeter Telescope and ALMA observations of extremely luminous high-redshift galaxies identified by the Planck
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The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years
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Early science with the Large Millimeter Telescope: a 1.1 mm AzTEC survey of red-Herschel dusty star-forming galaxies
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Star Formation Traced by Optical and Millimeter Hydrogen Recombination Lines and Free–Free Emissions in the Dusty Merging Galaxy NGC 3256—MUSE/VLT and ALMA Synergy
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The Redshift and Star Formation Mode of AzTEC2: A Pair of Massive Galaxies at <i>z</i> = 4.63
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Nature of Faint Radio Sources in GOODS-North and GOODS-South Fields. I. Spectral Index and Radio–FIR Correlation
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Environmental Effect on the Interstellar Medium in Galaxies across the Cosmic Web at z = 0.73
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Neutral Gas Properties and Lyα Escape in Extreme Green Pea Galaxies
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Physical Characterization of an Unlensed, Dusty Star-forming Galaxy at <i>z</i> = 5.85
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ALMA Observations of HCN and HCO+ Outflows in the Merging Galaxy NGC 3256
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ALMA twenty-six arcmin2 survey of GOODS-S at one millimeter (ASAGAO): Source catalog and number counts
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The Dust-selected Molecular Clouds in the Northeast Region of the Small Magellanic Cloud
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A High-resolution Mosaic of the Neutral Hydrogen in the M81 Triplet
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Spatially Resolved Dense Molecular Gas Excitation in the Nearby LIRG VV 114
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Early Science with the Large Millimeter Telescope: An Energy-driven Wind Revealed by Massive Molecular and Fast X-Ray Outflows in the Seyfert Galaxy IRAS 17020+4544
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CHILES: H i morphology and galaxy environment at z = 0.12 and z = 0.17
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Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC 4449
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H i Observations of Major-merger Pairs at z = 0: Atomic Gas and Star Formation
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The unexpectedly large dust and gas content of quiescent galaxies at z > 1.4
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AzTEC 1.1 mm observations of high-z protocluster environments: SMG overdensities and misalignment between AGN jets and SMG distribution
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ALMA Reveals Strong $[{\bf{C}}\,{\bf{II}}]$ Emission in a Galaxy Embedded in a Giant LyαBlob atz= 3.1
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ALMA Resolves the Nuclear Disks of Arp 220
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Early Science with the Large Millimeter Telescope: Detection of Dust Emission in Multiple Images of a Normal Galaxy at z > 4 Lensed by a Frontier Fields Cluster
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Detection of a Substantial Molecular Gas Reservoir in a Brightest Cluster Galaxy at z = 1.7
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A dusty star-forming galaxy at z = 6 revealed by strong gravitational lensing
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Erratum: ‘Early science with the Large Millimeter Telescope: observations of extremely luminous high-z sources identified by Planck’
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Very Compact Millimeter Sizes for Composite Star-forming/AGN Submillimeter Galaxies
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Multiwavelength Characterization of an ACT-selected, Lensed Dusty Star-forming Galaxy at z = 2.64
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A Radio-to-mm Census of Star-forming Galaxies in Protocluster 4C23.56 at Z = 2.5: Gas Mass and Its Fraction Revealed with ALMA
Human - wd:Q58929564