Andrew Mann

Assistant Professor

University of North Carolina at Chapel Hill

United States

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Andrew Mann is an Assistant Professor at the University of North Carolina at Chapel Hill, USA. His research focuses on the exploration of exoplanets, including studies on super-Neptunes, mini-Neptunes, and the demographics of young exoplanets. Recent articles highlight his work on stellar rotation measurements, the characteristics of transiting planets, and their interactions with binary star systems.

Articles (20)

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2025

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2023

Collaborators (16)

Trent Dupuy

Reader

University of Edinburgh

UNITED KINGDOM

Andrew Mann

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Articles (20)

Investigating the eccentricity distribution of transiting, long-period giant planets

A 16 Myr Super-Neptune in Upper Centaurus Lupus and a Preliminary Survey of Transiting Planets in Sco-Cen with TESS

TESS Investigation—Demographics of Young Exoplanets (TI-DYE). III. An Inner Super-Earth in TOI 2076

Quantifying the Limits of TESS Stellar Rotation Measurements with the K2-TESS Overlap

Mass, gas, and Gauss around a T Tauri Star with SPIRou

A transiting multiplanet system in the 61 Myr old association Theia 116

TESS Hunt for Young and Maturing Exoplanets (THYME). XII. A Young Mini-Neptune on the Upper Edge of the Radius Valley in the Hyades Cluster

Revising Properties of Planet–Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation*

The Featherweight Giant: Unraveling the Atmosphere of a 17 Myr Planet with JWST

A giant planet transiting a 3-Myr protostar with a misaligned disk

TESS Observations of the Pleiades Cluster: A Nursery for δ Scuti Stars

Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star

The Variable Detection of Atmospheric Escape around the Young, Hot Neptune AU Mic b

Using the Gaia Excess Uncertainty as a Proxy for Stellar Variability and Age

A Search for Stellar Siblings of the ∼200 Myr TOI-251 b Planetary System

HIP 33609 b: An Eccentric Brown Dwarf Transiting a V = 7.3 Rapidly Rotating B Star

Revising Properties of Planet–Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems*

Erratum: “TESS Hunt for Young and Maturing Exoplanets (THYME). VII. Membership, Rotation, and Lithium in the Young Cluster Group-X and a New Young Exoplanet” (2022, AJ, 164, 119)

TESS Hunt for Young and Maturing Exoplanets (THYME). IX. A 27 Myr Extended Population of Lower Centaurus Crux with a Transiting Two-planet System

A Low-mass, Pre-main-sequence Eclipsing Binary in the 40 Myr Columba Association—Fundamental Stellar Parameters and Modeling the Effect of Star Spots

Collaborators (16)

Trent Dupuy

Daniel R Hey

David Lafrenière

Daisuke Kawata

Xu Huang

Elisabeth Newton

Adina D Feinstein

Luis Welbanks

Tim Bedding

KEVIN FRANCE

ALEXANDER BROWN

Yaguang Li

George Zhou

Zachory Berta-Thompson

Courtney Crawford

Gregory Feiden

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