activity
20152022
most citedThe Chemical Composition of τ Ceti and Possible Effects on Terrestrial Planets

42 citations · 85 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2022★ 1 cited

Continuous Habitable Zones: Using Bayesian Methods to Prioritize Characterization of Potentially Habitable Worlds

Austin Ware, Patrick Young, Amanda Truitt +1

The number of potentially habitable planets continues to increase, but we lack the time and resources to characterize all of them. With 30 known potentially habitable planets…

astro-ph.EP2019★ 14 cited

A Flexible Bayesian Framework for Assessing Habitability with Joint Observational and Model Constraints

Amanda R. Truitt, Patrick A. Young, Sara I. Walker +1

The catalog of stellar evolution tracks discussed in our previous work is meant to help characterize exoplanet host-stars of interest for follow-up observations with future mission…

astro-ph.SR2016★ 10 cited

Expanding the Catalog: Considering the Importance of Carbon, Magnesium, and Neon in the Evolution of Stars and Habitable Zones

Amanda Truitt, Patrick A. Young

Building on previous work, we have expanded our catalog of evolutionary models for stars with variable composition; here we present models for stars of mass 0.5 - 1.2 Msol, at scal…

astro-ph.SR2015★ 18 cited

A Catalog of Stellar Evolution Profiles and the Effects of Variable Composition on Habitable Systems

Amanda Truitt, Patrick A. Young, Alexander Spacek +2

We present stellar evolution models for 0.5 - 1.2 \Msol at scaled metallicities of 0.1 - 1.5 Z\sol and O/Fe values of 0.44 - 2.28 O/Fe\sol. The time dependent evolution of habitabl…

astro-ph.EP2015★ 42 cited

The Chemical Composition of τ Ceti and Possible Effects on Terrestrial Planets

Michael Pagano, Amanda Truitt, Patrick A. Young +1

τ Ceti (HD10700), a G8 dwarf with solar mass of 0.78, is a close (3.65 pc) sun-like star where 5 possibly terrestrial planet candidates (minimum masses of 2, 3.1, 3.5, 4.3, and 6.7…