PHOEBE binary star modelling in the era of Kepler and TESS

Bibcode
2020sea..confE.150J
Jones, D.; Conroy, K.; Horvat, M.; Kochoska, A.; Giammarco, J.; Pablo, H.; Hambleton, K.; Prša, A.
Referencia bibliográfica

Contributions to the XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society

Fecha de publicación:
7
2020
Número de autores
8
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
PHOEBE2 (PHysics of Eclipsing BinariEs 2) is an open source binary star modelling code, which reproduces and fits light and radial velocity curves, spectral line profiles and astrometric orbits. The code represents a modern implementation of the Wilson-Devinney code with significant refinements, principally with the aim of providing an open, continuously-developed, robust and high-fidelity tool for the modelling of binary stars in the modern era of ultra-high precision space-based photometry.
Tipo
Sin árbitro

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