1k citations · 15.3k across the 224 of their papers we have counts for
10 papers · 1 filter
Stellar Diameters and Temperatures VI. High angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfs
Tabetha Boyajian, Kaspar von Braun, Gregory A. Feiden +24
We present direct radii measurements of the well-known transiting exoplanet host stars HD 189733 and HD 209458 using the CHARA Array interferometer. We find the limb-darkened angul…
Touchstone Stars: Highlights from the Cool Stars 18 Splinter Session
Andrew W. Mann, Adam Kraus, Tabetha Boyajian +11
We present a summary of the splinter session on "touchstone stars" -- stars with directly measured parameters -- that was organized as part of the Cool Stars 18 conference. We disc…
The Near-Ultraviolet Luminosity Function of Young, Early M-Type Dwarf Stars
Megan Ansdell, Eric Gaidos, Andrew W. Mann +8
Planets orbiting within the close-in habitable zones of M dwarf stars will be exposed to elevated high-energy radiation driven by strong magneto-hydrodynamic dynamos during stellar…
Characterizing the Parents: Exoplanets Around Cool Stars
Kaspar von Braun, Tabetha S. Boyajian, Gerard T. van Belle +2
The large majority of stars in the Milky Way are late-type dwarfs, and the frequency of low-mass exoplanets in orbits around these late-type dwarfs appears to be high. In order to…
Wide, Cool and Ultracool Companions to Nearby Stars from Pan-STARRS1
Niall R. Deacon, Michael C. Liu, Eugene A. Magnier +18
We present the discovery of 61 wide (>5 arcsecond) separation, low-mass (stellar and substellar) companions to stars in the solar neighborhood identified from Pan-STARRS\,1 (PS1) d…
Warm Ice Giant GJ 3470b. II Revised Planetary and Stellar Parameters from Optical to Near-infrared Transit Photometry
Lauren I. Biddle, Kyle A. Pearson, Ian J. M. Crossfield +19
It is important to explore the diversity of characteristics of low-mass, low-density planets to understand the nature and evolution of this class of planets. We present a homogeneo…