activity
20162026
most citedThe L 98-59 System: Three Transiting, Terrestrial-Sized Planets Orbiting a Nearby M-dwarf

135 citations · 411 across the 17 of their papers we have counts for

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5 papers · 1 filter

astro-ph.SR2024

A Multiwavelength Survey of Nearby M dwarfs: Optical and Near-Ultraviolet Flares and Activity with Contemporaneous TESS, Kepler/K2, \textit{Swift}, and HST Observations

Rishi R. Paudel, Thomas Barclay, Allison Youngblood +14

We present a comprehensive multiwavelength investigation into flares and activity in nearby M~dwarf stars. We leverage the most extensive contemporaneous dataset obtained through t…

astro-ph.SR2022★ 6 cited

A Pilot Survey of an M Dwarf Flare Star with Swift's UV Grism

Shashank Chavali, Allison Youngblood, Rishi R. Paudel +5

The near-ultraviolet (NUV) spectral region is a useful diagnostic for stellar flare physics and assessing the energy environment of young exoplanets, especially as relates to prebi…

astro-ph.SR2021★ 41 cited

Simultaneous Multiwavelength Flare Observations of EV Lacertae

Rishi R. Paudel, Thomas Barclay, Joshua E. Schlieder +17

We present the first results of our ongoing project conducting simultaneous multiwavelength observations of flares on nearby active M dwarfs. We acquired data of the nearby dM3.5e…

astro-ph.SR2021★ 5 cited

Multiwavelength Observations of the RV Tauri Variable System U Monocerotis: Long-Term Variability Phenomena That Can Be Explained by Binary Interactions with a Circumbinary Disk

Laura D. Vega, Keivan G. Stassun, Rodolfo Montez +7

We present X-ray through submillimeter observations of the classical RV Tauri (RVb-type) variable U Mon, a post-AGB binary with a circumbinary disk (CBD). Our SMA observations indi…

astro-ph.SR2017★ 18 cited

Evidence for Binarity and Possible Disk Obscuration in Kepler Observations of the Pulsating RV Tau Variable DF Cygni

Laura D. Vega, Keivan G. Stassun, Rodolfo Montez +2

The Kepler light curve of DF Cyg is unparalleled in precision and cadence for any RV Tau star to date spanning a baseline of 4 years and clearly displaying the signature puls…