activity
20092016
most citedThe MUSCLES Treasury Survey III: X-ray to Infrared Spectra of 11 M and K Stars Hosting Planets

232 citations · 314 across the 5 of their papers we have counts for

collaborators

21 papers

astro-ph.SR2016★ 232 cited

The MUSCLES Treasury Survey III: X-ray to Infrared Spectra of 11 M and K Stars Hosting Planets

R. O. Parke Loyd, Kevin France, Allison Youngblood +8

We present a catalog of panchromatic spectral energy distributions (SEDs) for 7 M and 4 K dwarf stars that span X-ray to infrared wavelengths (5 Å - 5.5 μm). These SEDs are composi…

astro-ph.HE2015★ 14 cited

KSwAGS: A Swift X-ray and UV Survey of the Kepler Field. I

Krista Lynne Smith, Patricia T. Boyd, Richard F. Mushotzky +6

We introduce the first phase of the Kepler-Swift Active Galaxies and Stars survey (KSwAGS), a simultaneous X-ray and UV survey of ~6 square degrees of the Kepler field using the Sw…

astro-ph.SR2015★ 24 cited

Temporal Evolution of the Size and Temperature of Betelgeuse's Extended Atmosphere

Eamon O'Gorman, Graham M. Harper, Alexander Brown +4

We use the Very Large Array (VLA) in the A configuration with the Pie Town (PT) Very Long Baseline Array (VLBA) antenna to spatially resolve the extended atmosphere of Betelgeuse o…

astro-ph.SR2014★ 44 cited

Variability of Disk Emission in Pre-Main Sequence and Related Stars. III. Exploring Structural Changes in the Pre-transitional Disk in HD 169142

Kevin R. Wagner, Michael L. Sitko, Carol A. Grady +17

We present near-IR and far-UV observations of the pre-transitional (gapped) disk in HD 169142 using NASA's Infrared Telescope Facility and Hubble Space Telescope. The combination o…

astro-ph.SR2014

X-ray Emission from Young Stars in the TW Hya Association

Alexander Brown, Gregory J. Herczeg, Thomas R. Ayres +2

The 9 Myr old TW Hya Association (TWA) is the nearest group (typical distances of 50 pc) of pre-main-sequence (PMS) stars with ages less than 10 Myr and contains stars with b…

astro-ph.GA2013

Direct Measurement of Interstellar Extinction Toward Young Stars Using Atomic Hydrogen Lyman- Absorption

Matthew McJunkin, Kevin France, P. C. Schneider +5

Interstellar reddening corrections are necessary to reconstruct the intrinsic spectral energy distributions (SEDs) of accreting protostellar systems. The stellar SED determines the…