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Zach Claytor

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Astronomical Data Scientist

Space Telescope Science Institute

United States

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Recent Grants

Grant: Close

Spots, Faculae, and Ages: The Promise of Rotation with Roman and Deep Learning

Open Date: 2023-12-01

Close Date: 2025-12-01

Articles (15)

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2026

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Collaborators (8)

Lauren Weiss

Assistant Professor

University of Notre Dame

UNITED STATES

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Lars A. Buchhave

Technical University of Denmark

DENMARK

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Rachael Beaton

Assistant Astronomer

Space Telescope Science Institute

UNITED STATES

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Johanna Teske

UNITED STATES

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Adina D Feinstein

Assistant Professor

Michigan State University

UNITED STATES

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Antonio Jiménez

Instituto de Astrofísica de Andalucía

SPAIN

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Lisa BUGNET

Assistant Professor

Institute of Science and Technology Austria

AUSTRIA

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Gregory Feiden

Professor of Astronomy

University of North Georgia

UNITED STATES

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Zach Claytor

Research Interests

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Recent Grants

Articles (15)

200,000+ Deep Learning–inferred Periods of Stellar Variability from the All-Sky Automated Survey for Supernovae

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca II infrared triplet

The YREC Stellar Evolution Code: Public Data Release

The Impact of the MAST Data Archive

New Rotation Periods from the Kepler Bonus Background Light Curves

Model Choice Matters for Age Inference on the Red Giant Branch

Trials and Tribulations of Chemodynamical Tagging: Investigating the Recovery of Open Clusters in the Gaia Data Release 3 and GALAH Data Release 4 Catalogs

Magnetic Activity Evolution of Solar-like Stars. II. S ph–Ro Evolution of Kepler Main-sequence Targets

TESS Stellar Rotation up to 80 Days in the Southern Continuous Viewing Zone

TESS Asteroseismology of β Hydri: A Subgiant with a Born-again Dynamo

Magnetic Activity Evolution of Solar-like Stars. I. S ph–Age Relation Derived from Kepler Observations

The TIME Table: rotation and ages of cool exoplanet host stars

Kepler-102: Masses and Compositions for a Super-Earth and Sub-Neptune Orbiting an Active Star

Temporal variation of the photometric magnetic activity for the Sun and Kepler solar-like stars

The Importance of Neural Network Hyperparameters in Determining Age Inference Quality

Collaborators (8)

Lauren Weiss

Lars A. Buchhave

Rachael Beaton

Johanna Teske

Adina D Feinstein

Antonio Jiménez

Lisa BUGNET

Gregory Feiden

Make your next move.

Zach Claytor

Research Interests

Explore related searches

Recent Grants

Articles (15)

200,000+ Deep Learning–inferred Periods of Stellar Variability from the All-Sky Automated Survey for Supernovae

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca II infrared triplet

The YREC Stellar Evolution Code: Public Data Release

The Impact of the MAST Data Archive

New Rotation Periods from the Kepler Bonus Background Light Curves

Model Choice Matters for Age Inference on the Red Giant Branch

Trials and Tribulations of Chemodynamical Tagging: Investigating the Recovery of Open Clusters in the Gaia Data Release 3 and GALAH Data Release 4 Catalogs

Magnetic Activity Evolution of Solar-like Stars. II. S ph–Ro Evolution of Kepler Main-sequence Targets

TESS Stellar Rotation up to 80 Days in the Southern Continuous Viewing Zone

TESS Asteroseismology of β Hydri: A Subgiant with a Born-again Dynamo

Magnetic Activity Evolution of Solar-like Stars. I. S ph–Age Relation Derived from Kepler Observations

The TIME Table: rotation and ages of cool exoplanet host stars

Kepler-102: Masses and Compositions for a Super-Earth and Sub-Neptune Orbiting an Active Star

Temporal variation of the photometric magnetic activity for the Sun and Kepler solar-like stars

The Importance of Neural Network Hyperparameters in Determining Age Inference Quality

Collaborators (8)

Lauren Weiss

Lars A. Buchhave

Rachael Beaton

Johanna Teske

Adina D Feinstein

Antonio Jiménez

Lisa BUGNET

Gregory Feiden

Make your next move.

Hints of enhanced magnetic activity after the intermediate rotation period gap as traced by the chromospheric Ca II infrared triplet