New envelope binding energies derived from PARSEC stellar tracks alter compact binary merger rate densities by over an order of magnitude when used in population synthesis.
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FLAME pipeline derives stellar luminosities, radii, masses and ages for Gaia DR4 using analytical calculations followed by minimization and Bayesian model inference, with tests showing statistical agreement to literature values.
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The impact of envelope binding energies on the merger rate density of binary compact objects
New envelope binding energies derived from PARSEC stellar tracks alter compact binary merger rate densities by over an order of magnitude when used in population synthesis.
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Stellar masses and ages in Gaia Data Release 4 from the Final Luminosity Age Mass Estimator algorithm
FLAME pipeline derives stellar luminosities, radii, masses and ages for Gaia DR4 using analytical calculations followed by minimization and Bayesian model inference, with tests showing statistical agreement to literature values.