A population-synthesis framework shows rotation and unresolved companions bias isochrone ages by a factor of at least 2 near the ZAMS and by 31% for older A stars, adding ~0.1 solar mass and ~180 Myr random uncertainties.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
A parametric avoidance model based on stellar age, metallicity, and multiplicity excludes ~50% of 1.74M Gaia DR3 stars as poor candidates for complex life, retaining 777835 targets and releasing the catalog publicly.
citing papers explorer
-
Quantifying isochrone-based age uncertainties for rapidly rotating A-type stars
A population-synthesis framework shows rotation and unresolved companions bias isochrone ages by a factor of at least 2 near the ZAMS and by 31% for older A stars, adding ~0.1 solar mass and ~180 Myr random uncertainties.
-
Where Not to Look: A Parametric Avoidance Model for SETI Target Selection
A parametric avoidance model based on stellar age, metallicity, and multiplicity excludes ~50% of 1.74M Gaia DR3 stars as poor candidates for complex life, retaining 777835 targets and releasing the catalog publicly.