The paper presents quantitative metrics and thresholds for selecting the Prime Sample of 15,000 stars in the PLATO LOPS2 field to enable ground-based follow-up of exoplanet candidates.
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MESA gains simultaneous binary star evolution, large nuclear networks, implicit hydrodynamics, and GYRE pulsation coupling for better massive star and supernova modeling.
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.
citing papers explorer
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The PLATO field selection process III. Selection of the Prime Sample for the LOPS2 field
The paper presents quantitative metrics and thresholds for selecting the Prime Sample of 15,000 stars in the PLATO LOPS2 field to enable ground-based follow-up of exoplanet candidates.
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Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
MESA gains simultaneous binary star evolution, large nuclear networks, implicit hydrodynamics, and GYRE pulsation coupling for better massive star and supernova modeling.
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Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.