about
The Kepler-454 system: a small, not-rocky inner planet, a jovian world, and a distant companionPrecise stellar surface gravities from the time scales of convectively driven brightness variations.Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant starsEnsemble asteroseismology of solar-type stars with the NASA Kepler mission.A sub-Mercury-sized exoplanet.An Earth-sized planet in the habitable zone of a cool star.Hot super-Earths stripped by their host starsExoplanet orbital eccentricities derived from LAMOST-Kepler analysis.HD 181068: a red giant in a triply eclipsing compact hierarchical triple system.Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systemsThe GALAH survey: observational overview andGaiaDR1 companionKepler-22b: A 2.4 EARTH-RADIUS PLANET IN THE HABITABLE ZONE OF A SUN-LIKE STARThe TESS–HERMES survey data release 1: high-resolution spectroscopy of the TESS southern continuous viewing zoneThe eleventh and twelfth data releases of the Sloan Digital Sky Survey: final data from SDSS-IIIThe 13th Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-IV Survey Mapping Nearby Galaxies at Apache Point ObservatoryMasses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planetsThe Correlation between Mixing Length and Metallicity on the Giant Branch: Implications for Ages in the Gaia EraThe APOKASC catalog: an asteroseismic and spectroscopic joint survey of targets in the Kepler fieldsOscillating red giants observed during campaign 1 of the Kepler K2 mission: new prospects for galactic archaeologyFundamental properties of Kepler planet-candidate host stars using asteroseismologyKepler-68: three planets, one with a density between that of earth and ice giantsTesting scaling relations for solar-like oscillations from the main sequence to red giants using Kepler dataPlanetary candidates observed by Kepler VII. The first fully uniform catalog based on the entire 48-month data set (Q1-Q17 DR24)Terrestrial planet occurrence rates for the Kepler GK dwarf samplePlanetary candidates observed by Kepler. VI. Planet sample from Q1--Q16 (47 months)Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months)Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25The K2-HERMES Survey. I. Planet-candidate Properties from K2 Campaigns 1–3Stellar Population Synthesis-based Modeling of the Milky Way using Asteroseismology of Dwarfs and Subgiants from${\boldsymbol{Kepler}}$Stellar population synthesis based modeling of the Milky Way using asteroseismology of 13,000 Kepler red giantsThe K2 ecliptic plane input catalog (EPIC) and stellar classifications of 138,600 targets in campaigns 1-8Modelling Kepler red giants in eclipsing binaries: calibrating the mixing-length parameter with asteroseismologyVery regular high-frequency pulsation modes in young intermediate-mass stars
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description
researcher ORCID ID = 0000-0001-8832-4488
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wetenschapper
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name
Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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Daniel Huber
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1950-01-01T00:00:00Z