This version of ExoPlaSim has an overhauled orbital geometry routine, accessible with keplerian=True when configuring models, which permits obliquities from -180 to 180 degrees and eccentricities in the range [0,1)
Neuss: Bruno Buike 2015 - 8 p. - E66 - make 2 lists from wikipedia a) list of excentricity of planet...
Context. The mutual orbital alignment in multiple planetary systems is an important parameter for un...
International audienceContext. The 51 Eridani system harbors a complex architecture with its primary...
This release incorporates a large array of changes meant to allow PlaSim to model almost any vaguely...
The first release where documentation is fully-functioning. Also now officially including the random...
For some eccentric planetary orbits, the host star appears to move backwards in the sky as the orbit...
Version of SysSim used for papers: He, Ford, & Ragozzine (2020a) AJ 161, 16 (24pp). "Architectures ...
Aims. With the purpose of determining the orbital parameters of exoplanetary systems from observatio...
Copyright c © 2013 Daisuke Toyoda et al. This is an open access article distributed under the Creati...
Adds a more robust and faster Kepler solver [ref])(http://adsabs.harvard.edu/abs/1991CeMDA..51..319N...
Adds support for light travel time when computing positions in Keplerian orbits Adds SecondaryEclips...
We confirm the Kepler planet candidate Kepler-410A b (KOI-42b) as a Neptune-sized exoplanet on a 17....
Package to support the analysis of high-precision astrometry timeseries, in particular the determina...
The obliquity is the physical property that can be used to probe the history of formation and evolut...
We confirm the Kepler planet candidate Kepler-410A b (KOI-42b) as a Neptune-sized exoplanet on a 17....
Neuss: Bruno Buike 2015 - 8 p. - E66 - make 2 lists from wikipedia a) list of excentricity of planet...
Context. The mutual orbital alignment in multiple planetary systems is an important parameter for un...
International audienceContext. The 51 Eridani system harbors a complex architecture with its primary...
This release incorporates a large array of changes meant to allow PlaSim to model almost any vaguely...
The first release where documentation is fully-functioning. Also now officially including the random...
For some eccentric planetary orbits, the host star appears to move backwards in the sky as the orbit...
Version of SysSim used for papers: He, Ford, & Ragozzine (2020a) AJ 161, 16 (24pp). "Architectures ...
Aims. With the purpose of determining the orbital parameters of exoplanetary systems from observatio...
Copyright c © 2013 Daisuke Toyoda et al. This is an open access article distributed under the Creati...
Adds a more robust and faster Kepler solver [ref])(http://adsabs.harvard.edu/abs/1991CeMDA..51..319N...
Adds support for light travel time when computing positions in Keplerian orbits Adds SecondaryEclips...
We confirm the Kepler planet candidate Kepler-410A b (KOI-42b) as a Neptune-sized exoplanet on a 17....
Package to support the analysis of high-precision astrometry timeseries, in particular the determina...
The obliquity is the physical property that can be used to probe the history of formation and evolut...
We confirm the Kepler planet candidate Kepler-410A b (KOI-42b) as a Neptune-sized exoplanet on a 17....
Neuss: Bruno Buike 2015 - 8 p. - E66 - make 2 lists from wikipedia a) list of excentricity of planet...
Context. The mutual orbital alignment in multiple planetary systems is an important parameter for un...
International audienceContext. The 51 Eridani system harbors a complex architecture with its primary...
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