activity
20162020
most citedLyman- Observations of High Radial Velocity Low-Mass Stars Ross 1044 and Ross 825

13 citations · 38 across the 5 of their papers we have counts for

collaborators

12 papers

astro-ph.SR202120 cited

Stellar flares from blended and neighbouring stars in Kepler short cadence observations

James A. G. Jackman, Evgenya Shkolnik, R. O. Parke Loyd

We present the results of a search for stellar flares from stars neighbouring the target sources in the Kepler short cadence data. These flares have been discarded as contaminants…

astro-ph.IM20201 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.SR201913 cited

Lyman- Observations of High Radial Velocity Low-Mass Stars Ross 1044 and Ross 825

Adam C. Schneider, Evgenya L. Shkolnik, Travis S. Barman +1

The discovery of habitable zone (HZ) planets around low-mass stars has highlighted the need for a comprehensive understanding of the radiation environments in which such planets re…

astro-ph.SR20191 cited

A Hot Ultraviolet Flare on the M Dwarf Star GJ 674

C. S. Froning, A. Kowalski, K. France +10

As part of the Mega MUSCLES Hubble Space Telescope (HST) Treasury program, we obtained time-series ultraviolet spectroscopy of the M2.5V star, GJ~674. During the FUV monitoring obs…

astro-ph.SR2018

HAZMAT. IV. Flares and Superflares on Young M Stars in the Far Ultraviolet

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

M stars are powerful emitters of far-ultraviolet light. Over long timescales, a significant, possibly dominant, fraction of this emission is produced by stellar flares. Characteriz…

astro-ph.SR2018

The MUSCLES Treasury Survey. V. FUV Flares on Active and Inactive M Dwarfs

R. O. Parke Loyd, Kevin France, Allison Youngblood +10

M dwarf stars are known for their vigorous flaring. This flaring could impact the climate of orbiting planets, making it important to characterize M dwarf flares at the short wavel…