about
Frame-to-frame image realignment assessment tool for dynamic brain positron emission tomography.Friends of hot Jupiters. I. A radial velocity search for massive, long-period companions to close-in gas giant planetsWASP-12b AND HAT-P-8b ARE MEMBERS OF TRIPLE STAR SYSTEMSCharacterizing the Performance of the NIRC2 Vortex Coronagraph at W. M. Keck ObservatoryEPIC 219217635: A Doubly Eclipsing Quadruple System Containing an Evolved BinaryNo Difference in Orbital Parameters of RV-detected Giant Planets between 0.1 and 5 au in Single versus Multi-stellar SystemsEPIC 220204960: A Quadruple Star System Containing Two Strongly Interacting Eclipsing BinariesOn-sky performance of the QACITS pointing control technique with the Keck/NIRC2 vortex coronagraphKELT-16b: A Highly Irradiated, Ultra-short Period Hot Jupiter Nearing Tidal DisruptionEPIC 201702477b: A TRANSITING BROWN DWARF FROMK2IN A 41 DAY ORBITNear-infrared emission spectrum of WASP-103b using Hubble Space Telescope/Wide Field Camera 3Planets around low-mass stars (PALMS). VI. Discovery of a remarkably red planetary-mass companion to the AB Dor moving group candidate 2MASS J22362452+4751425*A quintuple star system containing two eclipsing binariesFriends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migrationStatistics of long period gas giant planets in known planetary systemsKIC 7177553: a quadruple system of two close binariesFriends of hot jupiters. III. An infrared spectroscopic search for low-mass stellar companionsFriends of hot jupiters. II. No correspondence between Hot-Jupiter spin-orbit misalignment and the incidence of directly imaged stellar companionsCharacterization of the atmosphere of the hot Jupiter HAT-P-32Ab and the M-dwarf companion HAT-P-32BLIPAD Simulations of Giant Planet Core FormationProduction of near-earth asteroids on retrograde orbitsThe orbital distribution of Near-Earth Objects inside Earth’s orbitSubmillimetre observations of galaxy clusters with the BLAST: the star formation activity in Abell 3112BLAST: a far-infrared measurement of the history of star formationBLAST: resolving the cosmic submillimeter backgroundOver half of the far-infrared background light comes from galaxies at z ≥ 1.2
P50
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P50
description
hulumtues
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researcher
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wetenschapper
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հետազոտող
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name
Henry Ngo
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Henry Ngo
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Henry Ngo
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Henry Ngo
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Henry Ngo
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type
label
Henry Ngo
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Henry Ngo
@en
Henry Ngo
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Henry Ngo
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Henry Ngo
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prefLabel
Henry Ngo
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Henry Ngo
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Henry Ngo
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Henry Ngo
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Henry Ngo
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P21
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0000-0001-5172-4859