0000000000298902

AUTHOR

Rafael A. García

showing 2 related works from this author

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

2019

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unveil the composition and dynamics of the faint Universe and impact nearly every field of astrophysics across all spatial scales, from individual stars to the largest scale structures in the Universe. Major pillars in the science program for MSE include (i) the ultimate Gaia follow-up facility for understanding the chemistry and dynamics of the distant Milky Way, including the outer disk and faint stellar halo at high spectral resolution (ii) galaxy formation and evolution at cosmic noon, via the type of revolutionary…

[PHYS]Physics [physics]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of Galaxies[PHYS] Physics [physics][SDU] Sciences of the Universe [physics][SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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The Second APOKASC Catalog: The Empirical Approach

2018

We present a catalog of stellar properties for a large sample of 6676 evolved stars with APOGEE spectroscopic parameters and \textit{Kepler} asteroseismic data analyzed using five independent techniques. Our data includes evolutionary state, surface gravity, mean density, mass, radius, age, and the spectroscopic and asteroseismic measurements used to derive them. We employ a new empirical approach for combining asteroseismic measurements from different methods, calibrating the inferred stellar parameters, and estimating uncertainties. With high statistical significance, we find that asteroseismic parameters inferred from the different pipelines have systematic offsets that are not removed b…

Stellar populationoscillations (including pulsations) [stars]fundamental parameters [stars]KEPLERFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesOSCILLATIONSAstrophysics::Solar and Stellar AstrophysicsStatistical dispersionstars abundancesFIELD010303 astronomy & astrophysicsRed clumpScalingComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsMIXING-LENGTH010308 nuclear & particles physicsAstronomy and AstrophysicsRadiusSurface gravityAGESRED GIANTSStarsStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceOPEN CLUSTERSAstrophysics::Earth and Planetary AstrophysicsBOLOMETRIC CORRECTIONS[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSASTEROSEISMIC MASS
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