430 citations · 2.3k across the 25 of their papers we have counts for
25 papers
Beyond 2-D Mass-Radius Relationships: A Nonparametric and Probabilistic Framework for Characterizing Planetary Samples in Higher Dimensions
Shubham Kanodia, Matthias Y. He, Eric B. Ford +2
Fundamental to our understanding of planetary bulk compositions is the relationship between their masses and radii, two properties that are often not simultaneously known for most…
A Decade of Linear and Circular Polarimetry with the POLISH2 Polarimeter
Sloane J. Wiktorowicz, Agnieszka Słowikowska, Larissa A. Nofi +15
The POLISH2 optical polarimeter has been in operation at the Lick Observatory 3-m Shane telescope since 2011, and it was commissioned at the Gemini North 8-m in 2016. This instrume…
Importance of Sample Selection in Exoplanet Atmosphere Population Studies
Natasha E. Batalha, Angie Wolfgang, Johanna Teske +5
Understanding planet formation requires robust population studies, which are designed to reveal trends in planet properties. In this work, we aim to determine if different methods…
The young HD 73583 (TOI-560) planetary system: Two 10-M mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf
O. Barragán, D. J. Armstrong, D. Gandolfi +103
We present the discovery and characterisation of two transiting planets observed by \textit{TESS} in the light curves of the young and bright (V=9.67) star HD73583 (TOI-560). We pe…
Following up the Kepler field: Masses of Targets for transit timing and atmospheric characterization
Daniel Jontof-Hutter, Angie Wolfgang, Eric B. Ford +3
We identify a set of planetary systems observed by Kepler that merit transit timing variation (TTV) analysis given the orbital periods of transiting planets, the uncertainties for…
The Magellan-TESS Survey I: Survey Description and Mid-Survey Results
Johanna Teske, Sharon Xuesong Wang, Angie Wolfgang +66
revealed that roughly one-third of Sun-like stars host planets orbiting within 100 days and between the size of Earth and Neptune. How do these planets form, what are they…