593 citations · 3.8k across the 58 of their papers we have counts for
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Stellar Diameters and Temperatures V. Eleven Newly Characterized Exoplanet Host Stars
Kaspar von Braun, Tabetha S. Boyajian, Gerard T. van Belle +17
We use near-infrared interferometric data coupled with trigonometric parallax values and spectral energy distribution fitting to directly determine stellar radii, effective tempera…
Stellar Diameters and Temperatures IV. Predicting Stellar Angular Diameters
Tabetha Boyajian, Gerard van Belle, Kaspar von Braun
The number of stellar angular diameter measurements has greatly increased over the past few years due to innovations and developments in the field of long baseline optical interfer…
Predicting Stellar Angular Sizes
Kaspar von Braun, Tabetha S. Boyajian, Gerard T. van Belle
Our survey of long-baseline infrared and optical interferometry measurements is producing considerable numbers of directly determined stellar angular sizes. We use our sample of 12…
The PTI Carbon Star Angular Size Survey: Effective Temperatures and Non-Sphericity
Gerard T. van Belle, Claudia Paladini, Bernhard Aringer +2
We report new interferometric angular diameter observations of 41 carbon stars observed with the Palomar Testbed Interferometer (PTI). Two of these stars are CH carbon stars and re…
NPOI Observations of the Exoplanet Host kappa Coronae Borealis and Their Implications for the Star's and Planet's Masses and Ages
Ellyn K. Baines, J. Thomas Armstrong, Gerard T. van Belle
We used the Navy Precision Optical Interferometer to measure the limb-darkened angular diameter of the exoplanet host star kappa CrB and obtained a value of 1.543 +/- 0.009 mas. We…
Stellar Diameters and Temperatures III. Main Sequence A, F, G, & K Stars: Additional high-precision measurements and empirical relations
Tabetha S. Boyajian, Kaspar von Braun, Gerard van Belle +13
Based on CHARA Array measurements, we present the angular diameters of 23 nearby, main- sequence stars, ranging from spectral type A7 to K0, five of which are exoplanet host stars.…
Characterization of the Red Giant HR 2582 Using the CHARA Array
Ellyn K. Baines, Harold A. McAlister, Theo A. ten Brummelaar +7
We present the fundamental parameters of HR 2582, a high-mass red giant star whose evolutionary state is a mystery. We used the CHARA Array interferometer to directly measure the s…
Dynamical mass of the O-type supergiant in Zeta Orionis A
C. A. Hummel, Th. Rivinius, M. -F. Nieva +3
A close companion of Zeta Orionis A was found in 2000 with the Navy Precision Optical Interferometer (NPOI), and shown to be a physical companion. Because the primary is a supergia…