activity
20052020
most citedStellar Diameters and Temperatures II. Main Sequence K & M Stars

593 citations · 7.2k across the 90 of their papers we have counts for

collaborators
Showing 2014Show all

5 papers · 1 filter

astro-ph.SR2014★ 116 cited

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…

astro-ph.SR2014★ 62 cited

Benchmark stars for Gaia: fundamental properties of the Population II star HD140283 from interferometric, spectroscopic and photometric data

O. Creevey, F. Thévenin, P. Berio +17

We determined the fundamental properties of HD 140283 by obtaining new interferometric and spectroscopic measurements and combining them with photometry from the literature. The in…

astro-ph.SR2014★ 37 cited

Improving the surface brightness-color relation for early-type stars using optical interferometry

M. Challouf, N. Nardetto, D. Mourard +18

The aim of this work is to improve the SBC relation for early-type stars in the color domain, using optical interferometry. Observations of eight B- and A-type…

astro-ph.SR2014★ 199 cited

Separated Fringe Packet Observations with the CHARA Array II: Andromeda, HD 178911, and ξ Cephei

Christopher D. Farrington, Theo A. ten Brummelaar, Brian D. Mason +7

When observed with optical long-baseline interferometers (OLBI), components of a binary star which are sufficiently separated produce their own interferometric fringe packets; thes…

astro-ph.SR2014★ 37 cited

CHARA/MIRC observations of two M supergiants in Perseus OB1: temperature, Bayesian modeling, and compressed sensing imaging

F. Baron, J. D. Monnier, L. L. Kiss +12

Two red supergiants of the Per OB1 association, RS Per and T Per, have been observed in H band using the MIRC instrument at the CHARA array. The data show clear evidence of departu…