activity
20022025
most citedA Framework for Prioritizing the TESS Planetary Candidates Most Amenable to Atmospheric Characterization

593 citations · 8.7k across the 134 of their papers we have counts for

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Showing 2020Show all

7 papers · 1 filter

astro-ph.SR2020★ 28 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.EP2020★ 43 cited

Time-resolved rotational velocities in the upper atmosphere of WASP-33 b

P. Wilson Cauley, Ji Wang, Evgenya L. Shkolnik +4

While steady empirical progress has been made in understanding the structure and composition of hot planet atmospheres, direct measurements of velocity signatures, including winds,…

astro-ph.IM2020★ 1 cited

A High-Cadence UV-Optical Telescope Suite On The Lunar South Pole

Scott W. Fleming, Thomas Barclay, Keaton J. Bell +14

We propose a suite of telescopes be deployed as part of the Artemis III human-crewed expedition to the lunar south pole, able to collect wide-field simultaneous far-ultraviolet (UV…

astro-ph.SR2020★ 31 cited

Estimating the Ultraviolet Emission of M dwarfs with Exoplanets from Ca II and H

Katherine Melbourne, Allison Youngblood, Kevin France +29

M dwarf stars are excellent candidates around which to search for exoplanets, including temperate, Earth-sized planets. To evaluate the photochemistry of the planetary atmosphere,…

astro-ph.SR2020★ 16 cited

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.SR2020★ 3 cited

ACRONYM IV: Three New, Young, Low-mass Spectroscopic Binaries

Laura Flagg, Evgenya L. Shkolnik, Alycia Weinberger +4

As part of our search for new low-mass members of nearby young moving groups (YMG), we discovered three low-mass, spectroscopic binaries, two of which are not kinematically associa…