Jack Lubin

Teaching Assistent

United States

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About

Jack Lubin is a Teaching Assistant at UCI School of Physical Sciences in the United States. His research focuses on exoplanets and their characteristics, as evident from his recent articles exploring topics such as stellar resonances, planet alignment, and the impacts of stellar variability. Lubin's work contributes to advancements in understanding planetary systems, particularly in the context of ultra-short-period planets and the implications of multi-source photometry.

Articles (17)

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2025

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2025

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2025

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2025

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2025

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2025

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2024

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2024

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2024

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2024

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2023

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2023

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2022

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2022

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2022

Collaborators (10)

Jason Wright

Professor

Penn State

UNITED STATES

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Jaime A. Alvarado-Montes

Macquarie University

AUSTRALIA

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Paul Robertson

Assistant Professor

University of California, Irvine

UNITED STATES

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Benjamin Fulton

UNITED STATES

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Heather Knutson

Professor

California Institute of Technology

UNITED STATES

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Cullen Blake

Assistant Professor

University of Pennsylvania

UNITED STATES

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Rae Holcomb

University of California, Irvine

UNITED STATES

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Andrew Howard

Professor of Astronomy

California Institute of Technology

UNITED STATES

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Christian Schwab

Macquarie University

AUSTRALIA

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Natalie Batalha

Professor

University of California, Santa Cruz

UNITED STATES

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Jack Lubin

Research Interests

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Articles (17)

Peekaboo: Secular Resonances from Evolving Stellar Oblateness Impede Transit Detections

Stellar Obliquity of the Ultra-short-period Planet System HD 93963

The TESS–Keck Survey. XXIV. Outer Giants May Be More Prevalent in the Presence of Inner Small Planets

TOI-6324 b: An Earth-mass Ultra-short-period Planet Transiting a Nearby M Dwarf

Jitter Across 15 yr: Leveraging Precise Photometry from Kepler and TESS to Extract Exoplanets from Radial Velocity Time Series

Revised Masses for Low-density Planets Orbiting the Disordered M-dwarf System TOI-1266

The TESS-Keck Survey. XII. A Dense 1.8 R ⊕ Ultra-short-period Planet Possibly Clinging to a High-mean-molecular-weight Atmosphere after the First Gigayear

Utilizing Photometry from Multiple Sources to Mitigate Stellar Variability in Precise Radial Velocities: A Case Study of Kepler-21

The TESS-Keck Survey. XX. 15 New TESS Planets and a Uniform RV Analysis of All Survey Targets

Automated Scheduling of Doppler Exoplanet Observations at Keck Observatory

The TESS-Keck Survey. XVII. Precise Mass Measurements in a Young, High-multiplicity Transiting Planet System Using Radial Velocities and Transit Timing Variations

The HD 191939 Exoplanet System is Well Aligned and Flat

TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey

TOI-1670 c, a 40 day Orbital Period Warm Jupiter in a Compact System, Is Well Aligned

GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion

The TESS–Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-mass Outer Companion around TOI-1272

An Eccentric Brown Dwarf Eclipsing an M dwarf

Collaborators (10)

Jason Wright

Jaime A. Alvarado-Montes

Paul Robertson

Benjamin Fulton

Heather Knutson

Cullen Blake

Rae Holcomb

Andrew Howard

Christian Schwab

Natalie Batalha

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