activity
20192022
most citedThe first view of Scuti and Doradus stars with the TESS mission

125 citations · 519 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR202237 cited

Extending Optical Flare Models to the UV: Results from Comparing of TESS and GALEX Flare Observations For M Dwarfs

James A. G. Jackman, Evgenya Shkolnik, Chase Million +3

The ultraviolet (UV) emission of stellar flares may have a pivotal role in the habitability of rocky exoplanets around low-mass stars. Previous studies have used white-light observ…

astro-ph.SR202221 cited

HAZMAT. VIII. A Spectroscopic Analysis of the Ultraviolet Evolution of K Stars: Additional Evidence for K Dwarf Rotational Stalling in the First Gigayear

Tyler Richey-Yowell, Evgenya L. Shkolnik, R. O. Parke Loyd +7

Efforts to discover and characterize habitable zone planets have primarily focused on Sun-like stars and M dwarfs. K stars, however, provide an appealing compromise between these t…

astro-ph.SR202135 cited

TESS Cycle 1 observations of roAp stars with 2-min cadence data

D. L. Holdsworth, M. S. Cunha, D. W. Kurtz +41

We present the results of a systematic search for new rapidly oscillating Ap (roAp) stars using the 2-min cadence data collected by the Transiting Exoplanet Survey Satellite (TESS)…

astro-ph.SR202028 cited

HAZMAT. VII. The Evolution of Ultraviolet Emission with Age and Rotation for Early M Dwarf Stars

R. O. Parke Loyd, Evgenya L. Shkolnik, Adam C. Schneider +6

The ultraviolet (UV) emission from the most numerous stars in the universe, M dwarfs, impacts the formation, chemistry, atmospheric stability, and surface habitability of their pla…

astro-ph.SR2020

On the Correlation between L Dwarf Optical and Infrared Variability and Radio Aurorae

Tyler Richey-Yowell, Melodie M. Kao, J. Sebastian Pineda +2

Photometric variability attributed to cloud phenomena is common in L/T transition brown dwarfs. Recent studies show that such variability may also trace aurorae, suggesting that lo…

astro-ph.EP201953 cited

Current Population Statistics Do Not Favor Photoevaporation over Core-Powered Mass Loss as the Dominant Cause of the Exoplanet Radius Gap

R. O. P. Loyd, Evgenya L. Shkolnik, Adam C. Schneider +4

We search for evidence of the cause of the exoplanet radius gap, i.e. the dearth of planets with radii near . If the cause was photoevaporation, the radius gap shoul…