activity
20082025
most citedThe H emission of nearby M dwarfs and its relation to stellar rotation

367 citations · 5.6k across the 79 of their papers we have counts for

collaborators

79 papers

astro-ph.EP2025

THYME XIII: Two young Neptunes orbiting a 75-Myr star in the Alpha Persei Cluster

Anne Dattilo, Andrew M. Vanderburg, Madyson G. Barber +28

Young planets with mass measurements are particularly valuable in studying atmospheric mass-loss processes, but these planets are rare and their masses difficult to measure due to…

astro-ph.EP2024★ 3 cited

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

Pa Chia Thao, Andrew W. Mann, Adina D. Feinstein +29

The characterization of young planets (< 300 Myr) is pivotal for understanding planet formation and evolution. We present the 3-5m transmission spectrum of the 17 Myr, Jupiter-s…

astro-ph.EP2024

Searching for Neutral Hydrogen Escape from the 120 Myr Old Sub-Neptune HIP94235b using HST

Ava Morrissey, George Zhou, Chelsea X. Huang +9

HIP94235 b, a 120 Myr old sub-Neptune, provides us the unique opportunity to study mass loss at a pivotal stage of the system's evolution: the end of a 100 million year (Myr) old p…

astro-ph.EP2024

TESS Hunt for Young and Maturing Exoplanets (THYME) X: a two-planet system in the 210 Myr MELANGE-5 Association

Pa Chia Thao, Andrew W. Mann, Madyson G. Barber +35

Young (<500 Myr) planets are critical to studying how planets form and evolve. Among these young planetary systems, multi-planet configurations are particularly useful as they prov…

astro-ph.EP2023★ 18 cited

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

Keighley E. Rockcliffe, Elisabeth R. Newton, Allison Youngblood +5

Photoevaporation is a potential explanation for several features within exoplanet demographics. Atmospheric escape observed in young Neptune-sized exoplanets can provide insight in…

astro-ph.SR2023★ 7 cited

Contemporaneous Observations of Luminosities and Photometric Amplitudes for M Dwarfs

Aylin García Soto, Elisabeth R. Newton, Stephanie T. Douglas +2

While many M dwarfs are known to have strong magnetic fields and high levels of magnetic activity, we are still unsure about the properties of their starspots and the origin of the…