KEPLER: A Unified Model for Knowledge Embedding and Pre-trained Language Representation [PDF]
Pre-trained language representation models (PLMs) cannot well capture factual knowledge from text. In contrast, knowledge embedding (KE) methods can effectively represent the relational facts in knowledge graphs (KGs) with informative entity embeddings ...
Zhi-yuan Liu
exaly +4 more sources
Exoplanet Characterization by Proxy: a Transiting 2.15 R_Earth Planet Near the Habitable Zone of the Late K dwarf Kepler-61 [PDF]
We present the validation and characterization of Kepler-61b: a 2.15 R_Earth planet orbiting near the inner edge of the habitable zone of a low-mass star.
Ballard, Sarah +15 more
core +2 more sources
Near Mean-motion Resonances in the Systems Observed by Kepler: Affected by Mass Accretion and Type I Migration [PDF]
The Kepler mission has released over 4496 planetary candidates, among which 3483 planets have been confirmed as of April 2017. The statistical results of the planets show that there are two peaks around 1.5 and 2.0 in the distribution of orbital period ...
Ji, Jianghui, Wang, Su
core +2 more sources
Cosmological Ideas of Johannes Kepler in Their Relation to Antiquity Based on the Treatise Harmonices Mundi [PDF]
The article presents the results of the authors’ research on the cosmological views of Johannes Keppler in his Latin treatise Harmonices Mundi. The authors discuss the background of composing the treatise concerning the philosophical, religious, and ...
Sergii Rudenko, Mariia Lastovets
doaj +1 more source
Solar-Like Oscillators in the Kepler Era: A Review
Many late-type stars across the Milky Way exhibit observable pulsations similar to our Sun that open up a window into stellar interiors. The NASA Kepler mission, a space-based photometric telescope, measured the micro-magnitude luminosity fluctuations ...
Jason Jackiewicz
doaj +1 more source
Circumbinary Habitable Zones in the Presence of a Giant Planet
Determining habitable zones in binary star systems can be a challenging task due to the combination of perturbed planetary orbits and varying stellar irradiation conditions.
Nikolaos Georgakarakos +8 more
doaj +1 more source
An Improved Algorithm For The Solution of Kepler‘s Equation For An Elliptical Orbit [PDF]
In this paper, a root finding method due to iterative method is used first to thesolution of Kepler's equation for an elliptical orbit. Then the extrapolationtechnique in the form of Aitken D2 - acceleration is applied to improve theconvergence of the ...
Mohammed S. Rasheed
doaj +1 more source
Investigating the Variation of Selected Kepler Objects Mid-Transit Times
We derived minima times from the transit curves of star-planet systems, Kepler-412, Kepler-422, Kepler-427 ve Kepler-435 observed by Kepler space telescope, using the Kwee - van Woerden method and Gauss function fitting.
Çağlar Püsküllü, Oguz Ozturk
doaj +1 more source
Improved parameters of seven Kepler giant companions characterized with SOPHIE and HARPS-N [PDF]
Radial-velocity observations of Kepler candidates obtained with the SOPHIE and HARPS-N spectrographs have permitted unveiling the nature of the five giant planets Kepler-41b, Kepler-43b, Kepler-44b, Kepler-74b, and Kepler-75b, the massive companion ...
Almenara, J. -M. +8 more
core +9 more sources
Confirming Resonance in Three Transiting Systems
Although resonant planets have orbital periods near commensurability, resonance is also dictated by other factors, such as the planets’ eccentricities and masses, and therefore must be confirmed through a study of the system’s dynamics.
Tyler Quinn, Mariah G. MacDonald
doaj +1 more source

