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Clear power excess in a frequency range typical for solar-type oscillations in red giants has been detected in more than 1000 stars, which have been observed during the first 138 days of the science o...
We have studied solar-like oscillations in ~800 red-giant stars using Kepler long-cadence photometry. The sample includes stars ranging in evolution from the lower part of the red-giant branch to the ...
We simulate a Kepler-like observation of a theoretical exoplanet population and we show that the observed orbital period distribution of the Kepler giant planet candidates is best matched by an averag...
The Kepler Mission has acquired 33.5d of continuous one-minute photometry of KPD 1946+4340, a short-period binary system that consists of an sdB and a white dwarf. In the light curve, eclipses are cle...
Asteroseismology of stars in clusters has been a long-sought goal because the assumption of a common age, distance and initial chemical composition allows strong tests of the theory of stellar evoluti...
Kepler unveils its first five exoplanets(图)     Kepler  first five exoplanets       font style='font-size:12px;'> 2010/1/11
Scientists working on NASA's Kepler mission have unveiled the first five exoplanets discovered by the space telescope since it was launched in March 2009. The exoplanets – planets orbiting stars other...
NASA's Kepler Space Telescope Discovers Five Exoplanets     NASA's Kepler Space Telescope  Five Exoplanets       font style='font-size:12px;'> 2010/1/11
NASA's Kepler space telescope, designed to find Earth-size planets in the habitable zone of sun-like stars, has discovered its first five new exoplanets, or planets beyond our solar system.Kepler's hi...
In addition to its great potential for characterizing extra-solar planetary systems the Kepler mission is providing unique data on stellar oscillations. A key aspect of Kepler asteroseismology is the ...
Kepler到Newton —— 从万有引力定律的发现谈起     万有引力定律  Newton  Kepler       font style='font-size:12px;'> 2009/11/2
Kepler到Newton —— 从万有引力定律的发现谈起。
Precision Radial Velocities for the Kepler Era     Radial Velocities  Kepler Era       font style='font-size:12px;'> 2009/7/1
Precision Radial Velocities for the Kepler Era。
H 2-12, A Misidentified Planetary Nebula in Kepler SNR     H 2-12  Planetary Nebula  Kepler SNR       font style='font-size:12px;'> 2009/6/25
H 2-12, A Misidentified Planetary Nebula in Kepler SNR。
In this paper, an efficient iterative method of arbitrary integer order of convergence ≥ 2 has been established for solving the hyperbolic form of Kepler’s equation. The method is of a dynamic natur...
The research of Institute of Analytical Chemistry at the Johannes-Kepler-University Linz is in the frontline of organic analytical chemistry using state-of-the-art instrumentation in chromatography, e...
The Research Institute for Symbolic Computationis an institute of the Johannes Kepler University Linz, Austria.Symbolic Computation is for us:algorithmic solutions of mathematical problems, realizatio...
The Institute for Computational Mathematics, led by Prof. Ulrich Langer, is searching for a PostDoc with a strong background in the numerical treatment of partial differential equations, in particular...

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