about
Cold molecular gas in merger remnants. I. Formation of molecular gas disksA massive protocluster of galaxies at a redshift of z ≈ 5.3.Multiwavelength Observations of the Gas‐rich Host Galaxy of PDS 456: A New Challenge for the ULIRG‐to‐QSO Transition ScenarioSpectroscopic Confirmation of an Extreme Starburst at Redshift 4.547ALMA Deep Field in SSA22: Source Catalog and Number CountsALMA Reveals Strong $[{\bf{C}}\,{\bf{II}}]$ Emission in a Galaxy Embedded in a Giant LyαBlob atz= 3.1ALMA deep field in SSA22: a concentration of dusty starbursts in a z = 3.09 protocluster coreEarly Science with the Large Millimeter Telescope: observations of dust continuum and CO emission lines of cluster-lensed submillimetre galaxies atz=2.0–4.7AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts and evidence for large-scale structureAn AzTEC 1.1-mm survey for ULIRGs in the field of the Galaxy Cluster MS 0451.6−0305AzTEC half square degree survey of the SHADES fields â I. Maps, catalogues and source countsMid-infrared spectroscopy of candidate active galactic nuclei-dominated submillimeter galaxiesThe far-infrared/submillimeter properties of galaxies located behind the Bullet clusterMolecular Gas in the z = 2.565 Submillimeter Galaxy SMM J14011+0252Submillimeter Imaging of the Luminous Infrared Galaxy Pair VV 114Molecular Gas in the z = 2.8 Submillimeter Galaxy SMM 02399−0136ISM of Galaxies in Extremely Different Environments: Isolated vs Compact GroupsA deep ALMA image of theHubble Ultra Deep FieldAn AzTEC 1.1 mm survey of the GOODS-N field - II. Multiwavelength identifications and redshift distributionAn AzTEC 1.1 mm survey of the GOODS-N field - I. Maps, catalogue and source statisticsDynamical modeling of galaxy mergers using identikitHerMES: THE CONTRIBUTION TO THE COSMIC INFRARED BACKGROUND FROM GALAXIES SELECTED BY MASS AND REDSHIFTERRATUM: "Unveiling the nature of submillimeter galaxy SXDF 850.6" (2010, ApJ, 711, 974)Unveiling the nature of submillimeter galaxy SXDF 850.6Star formation suppression in compact group galaxies: a new path to quenching?Strong far-infrared cooling lines, peculiar CO kinematics, and possible star-formation suppression in Hickson compact group 57Enhanced warm H_2_ emission in the compact group mid-infrared "Green valley"Spitzer IRS spectral mapping of the Toomre sequence: spatial variations of PAH, gas, and dust properties in nearby major mergersGOODS–Herschel: an infrared main sequence for star-forming galaxiesIRAS 15099-5856: remarkable mid-infrared source with prominent crystalline silicate emission embedded in the supernova remnant MSH15-52CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy SurveyCANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey--The Hubble Space Telescope observations, imaging data products, and mosaicsThe redshift and nature of AzTEC/COSMOS 1: a starburst galaxy at z = 4.6Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC 4449An investigation of the dust content in the galaxy pair NGC 1512/1510 from near-infrared to millimeter wavelengthsALMA imaging of gas and dust in a galaxy protocluster at redshift 5.3: [C II] emission in "typical" galaxies and dusty starbursts {approx}1 billion years after the Big BangQuest for COSMOS submillimeter galaxy counterparts using CARMA and VLA: identifying three high-redshift starburst galaxiesMolecular Gas in a Submillimeter Galaxy atz= 4.5: Evidence for a Major Merger at 1 Billion Years after the Big BangStar Formation Rates in Lyman Break Galaxies: Radio Stacking of LBGs in the COSMOS Field and the Sub‐μJy Radio Source PopulationEvidence for a Population of High‐Redshift Submillimeter Galaxies from Interferometric Imaging
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description
researcher ORCID ID = 0000-0001-7095-7543
@en
wetenschapper
@nl
name
Min Yun
@ast
Min Yun
@en
Min Yun
@es
Min Yun
@nl
type
label
Min Yun
@ast
Min Yun
@en
Min Yun
@es
Min Yun
@nl
prefLabel
Min Yun
@ast
Min Yun
@en
Min Yun
@es
Min Yun
@nl
P106
P31
P496
0000-0001-7095-7543