J
Jennifer L. van Saders
Researcher at Carnegie Institution for Science
Publications - 52
Citations - 1988
Jennifer L. van Saders is an academic researcher from Carnegie Institution for Science. The author has contributed to research in topics: Stars & Asteroseismology. The author has an hindex of 20, co-authored 52 publications receiving 1513 citations. Previous affiliations of Jennifer L. van Saders include Princeton University & Carnegie Learning.
Papers
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Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2
TL;DR: In this article, the authors report revised radii of 177,911 stars derived by combining parallaxes from $Gaia$ Data Release 2 with the DR25 $Kepler$ Stellar Properties Catalog.
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Fast star, slow star; old star, young star: subgiant rotation as a population and stellar physics diagnostic
TL;DR: In this article, the expected range of rotation periods for cool field stellar populations (∼0.4-2.0 M{sub ǫ} ) was studied. But the authors did not consider the effect of the number of stars in the stellar population.
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The Gaia-Kepler Stellar Properties Catalog. I. Homogeneous Fundamental Properties for 186,301 Kepler Stars
TL;DR: The Gaia-Kepler Stellar Properties Catalog as mentioned in this paper is a set of stellar properties of 186,301 Kepler stars, homogeneously derived from isochrones and broadband photometry, Gaia Data Release 2 parallaxes, and spectroscopic metallicities, where available.
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Stellar evidence that the solar dynamo may be in transition
Travis S. Metcalfe,Ricky Egeland,Ricky Egeland,Jennifer L. van Saders,Jennifer L. van Saders +4 more
TL;DR: In this article, the evolution of chromospheric activity has been linked to a fundamental shift in the character of differential rotation of stars older than the Sun, suggesting that the Sun may be in a transitional evolutionary phase, and that its magnetic cycle might represent a special case of stellar dynamo theory.
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The Gaia-Kepler Stellar Properties Catalog. II. Planet Radius Demographics as a Function of Stellar Mass and Age
TL;DR: In this article, the authors re-compute Kepler planet radii and incident fluxes and investigate their distributions with stellar mass and age, and find evidence of a stellar age dependence of the planet populations straddling the radius valley.