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20072026
most citedMolecfit: A general tool for telluric absorption correction. I. Method and application to ESO instruments

762 citations · 5.1k across the 111 of their papers we have counts for

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Showing 2016Show all

6 papers · 1 filter

astro-ph.SR2016★ 25 cited

The Surface Brightness--Color Relations Based on Eclipsing Binary Stars: Toward Precision Better than 1% in Angular Diameter Predictions

Dariusz Graczyk, Piotr Konorski, Grzegorz Pietrzynski +7

In this study we investigate the calibration of surface brightness--color (SBC) relations based solely on eclipsing binary stars. We selected a sample of 35 detached eclipsing bina…

astro-ph.SR2016★ 80 cited

The radii and limb darkenings of Alpha Centauri A and B - Interferometric measurements with VLTI/PIONIER

P. Kervella, L. Bigot, A. Gallenne +1

The photospheric radius is one of the fundamental parameters governing the radiative equilibrium of a star. We report new observations of the nearest solar-type stars Alpha Centaur…

astro-ph.SR2016★ 24 cited

VEGA/CHARA interferometric observations of Cepheids. I. A resolved structure around the prototype classical Cepheid delta Cep in the visible spectral range

N. Nardetto, A. Mérand, D. Mourard +23

The B-W method is used to determine the distance of Cepheids and consists in combining the angular size variations of the star, as derived from infrared surface-brightness relation…

astro-ph.IM2016★ 3 cited

Planet Formation Imager (PFI): science vision and key requirements

Stefan Kraus, John D. Monnier, Michael J. Ireland +75

The Planet Formation Imager (PFI) project aims to provide a strong scientific vision for ground-based optical astronomy beyond the upcoming generation of Extremely Large Telescopes…

astro-ph.SR2016★ 11 cited

Multiplicity of Galactic Cepheids from long-baseline interferometry~III. Sub-percent limits on the relative brightness of a close companion of ~Cephei

A. Gallenne, A. Merand, P. Kervella +11

We report new CHARA/MIRC interferometric observations of the Cepheid archetype Cep, which aimed at detecting the newly discovered spectroscopic companion. We reached a maximum…

astro-ph.IM2016★ 56 cited

Observational calibration of the projection factor of Cepheids. II. Application to nine Cepheids with HST/FGS parallax measurements

Joanne Breitfelder, Antoine Mérand, Pierre Kervella +4

The distance to pulsating stars is classically estimated using the parallax-of-pulsation (PoP) method, which combines spectroscopic radial velocity measurements and angular diamete…