activity
20042026
most citedHow to Constrain Your M Dwarf: measuring effective temperature, bolometric luminosity, mass, and radius

722 citations · 6.3k across the 102 of their papers we have counts for

collaborators
Showing 2011Show all

9 papers · 1 filter

astro-ph.SR2011★ 210 cited

Stellar Diameters and Temperatures I. Main Sequence A, F, & G Stars

Tabetha S. Boyajian, Harold A. McAlister, Gerard van Belle +15

We have executed a survey of nearby, main sequence A, F, and G-type stars with the CHARA Array, successfully measuring the angular diameters of fortyfour stars with an average prec…

astro-ph.EP2011★ 106 cited

The Dynamical Mass and Three-Dimensional Orbit of HR7672B: A Benchmark Brown Dwarf with High Eccentricity

Justin R. Crepp, John Asher Johnson, Debra A. Fischer +10

The companion to the G0V star HR7672 directly imaged by Liu et al. (2002) has moved measurably along its orbit since the discovery epoch, making it possible to determine its dynami…

astro-ph.EP2011★ 188 cited

Characterizing the Cool KOIs II. The M Dwarf KOI-254 and its Hot Jupiter

John Asher Johnson, J. Zachary Gazak, Kevin Apps +12

We report the confirmation and characterization of a transiting gas giant planet orbiting the M dwarf KOI-254 every 2.455239 days, which was originally discovered by the Kepler mis…

astro-ph.SR2011★ 6 cited

Observational Constraints, Stellar Models, and Kepler Data for theta Cyg, the Brightest Star Observable by Kepler

J. A. Guzik, G. Houdek, W. J. Chaplin +8

The V=4.48 F4 main-sequence star theta Cyg is the brightest star observable in the Kepler spacecraft field-of-view. Short-cadence (58.8 s) photometric data were obtained by Kepler…

astro-ph.SR2011★ 46 cited

The diameter of the CoRoT target HD 49933. Combining the 3D limb darkening, asteroseismology, and interferometry

L. Bigot, D. Mourard, P. Berio +21

Context. The interpretation of stellar pulsations in terms of internal structure depends on the knowledge of the fundamental stellar parameters. Long-base interferometers permit us…

astro-ph.SR2011★ 46 cited

The 2011 outburst of the recurrent novaT Pyx. Evidence for a face-on bipolar ejection

Olivier Chesneau, A. Meilland, D. P. K. Banerjee +19

We report on near-IR interferometric observations of the outburst of the recurrent nova T Pyx. We obtained near-IR observations of T Pyx at dates ranging from t=2.37d to t=48.2d af…

astro-ph.SR2011

Recent Results form the CHARA Array

T. A. ten Brummelaar, D. Huber, K. von Braun +11

The CHARA Array is a six 1-m telescope optical and near infrared interferometer located at the Mount Wilson Observatory in southern California and operated by the Center for High A…

astro-ph.EP2011★ 1 cited

The 55 Cancri System: Fundamental Stellar Parameters, Habitable Zone Planet, and Super-Earth Diameter

K. von Braun, T. S. Boyajian, T. A. ten Brummelaar +13

The bright star 55 Cancri is known to host five planets, including a transiting super-Earth. We use the CHARA Array to directly determine the following of 55 Cnc's stellar astrophy…

astro-ph.EP2011★ 117 cited

Astrophysical Parameters and Habitable Zone of the Exoplanet Hosting Star GJ 581

Kaspar von Braun, Tabetha S. Boyajian, Stephen R. Kane +18

GJ 581 is an M dwarf host of a multiplanet system. We use long-baseline interferometric measurements from the CHARA Array, coupled with trigonometric parallax information, to direc…