activity
20022023
most citedA Multi-wavelength study of the M dwarf binary YY Geminorum

199 citations · 389 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2023★ 39 cited

A Seven-Day Multi-Wavelength Flare Campaign on AU Mic I: High-Time Resolution Light Curves and the Thermal Empirical Neupert Effect

Isaiah I. Tristan, Yuta Notsu, Adam F. Kowalski +13

We present light curves and flares from a seven day, multi-wavelength observational campaign of AU Mic, a young and active dM1e star with exoplanets and a debris disk. We report on…

astro-ph.IM2018

Advanced Technologies and Instrumentation and the National Science Foundation

Peter Kurczynski, James E. Neff

Over its more than thirty-year history, the Advanced Technologies and Instrumentation (ATI) program has provided grants to support technology development for ground-based astronomy…

astro-ph.HE2015★ 17 cited

Swift Observations of Gamma-Ray Burst Pulse Shapes: GRB Pulse Spectral Evolution Clarified

Jon Hakkila, Amy Lien, Takanori Sakamoto +3

Isolated Swift gamma-ray burst (GRB) pulses, like their higher-energy BATSE counterparts, emit the bulk of their pulsed emission as a hard-to-soft component that can be fitted by t…

astro-ph.SR2015★ 41 cited

An evaluation of the membership probability of 212 Boo stars: I. A Catalogue

Simon J. Murphy, Christopher J. Corbally, Richard O. Gray +6

The literature on the Boo stars has grown to become somewhat heterogenous, as different authors have applied different criteria across the UV, optical and infrared regions to d…

astro-ph.SR2015★ 199 cited

A Multi-wavelength study of the M dwarf binary YY Geminorum

C. J. Butler, N. Erkan, E. Budding +8

We review the results of the 1988 multi-wavelength campaign on the late-type eclipsing binary YY Geminorum. Observations include: broad-band optical and near infra-red photometry,…

astro-ph2008★ 13 cited

O VI Observations of the Onset of Convection Zones in Main-Sequence A Stars

J. E. Neff, T. Simon

If magnetic activity in outer stellar atmospheres is due to an interplay between rotation and subsurface convection, as is generally presumed, then one would not expect to observe…