JV
Jennifer van Saders
University of Hawai'i, Observatories of the Carnegie Institution of Washington, The Ohio State University, Rutgers, The State University of New Jersey
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Solar and Space Plasma Dynamics
0000-0002-4284-8638
Employment
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University of Hawai'i Assistant Astronomer2017 - Present
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Observatories of the Carnegie Institution of Washington Carnegie-Princeton Postdoctoral Fellow2014 - 2017
Education
- 2009 - 2014
- 2005 - 2009
Projects & Funding
Projects & funding information is unavailable.
Publications (153)
- The YREC Stellar Evolution Code: Public Data Release Save
- Antisolar Differential Rotation May Have Revived Magnetic Braking in the Subgiant 31 Aquilae Save
- Spectropolarimetric Constraints on the Maunder Minimum Analog HD 166620: Evidence for Weakened Magnetic Braking Save
- Weakened Magnetic Braking Signals the Collapse of the Global Stellar Dynamo Save
- Zeeman Doppler Imaging of τ Ceti: The Weakest Magnetic Field Detected in a Sun-like Star Save
- Testing the Rossby Paradigm: Weakened Magnetic Braking in Early K-type Stars Save
- K Dwarf Radius Inflation and a 10 Gyr Spin-down Clock Unveiled through Asteroseismology of HD 219134 from the Keck Planet Finder Save
- Rotation at the Fully Convective Boundary: Insights from Wide WD + MS Binary Systems Save
- The Prevalence of Resonance Among Young, Close-in Planets Save
- Extending the Asteroseismic Calibration of the Stellar Rossby Number Save
- Realistic Uncertainties for Fundamental Properties of Asteroseismic Red Giants and the Interplay between Mixing Length, Metallicity, and ν max Save
- TESS Asteroseismology of β Hydri: A Subgiant with a Born-again Dynamo Save
- Exploration of Stellar Variability in 20 s Cadence TESS Data Save
- A New Asteroseismic Kepler Benchmark Constrains the Onset of Weakened Magnetic Braking in Mature Sun-like Stars Save
- TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence Save
- Stellar flares are far-ultraviolet luminous Save
- A Test of Spectroscopic Age Estimates of White Dwarfs Using Wide WD+WD Binaries Save
- The Gasing Pangkah Collaboration. I. Asteroseismic Identification and Characterization of a Rapidly Rotating Engulfment Candidate* Save
- Stellar Cruise Control: Weakened Magnetic Braking Leads to Sustained Rapid Rotation of Old Stars Save
- TESS Stellar Rotation up to 80 Days in the Southern Continuous Viewing Zone Save