most citedInterferometric data reduction with AMBER/VLTI.Principle,estimators and illustration

291 citations · 588 across the 5 of their papers we have counts for

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astro-ph20087 cited

VSI: the VLTI spectro-imager

F. Malbet, D. Buscher, G. Weigelt +51

The VLTI Spectro Imager (VSI) was proposed as a second-generation instrument of the Very Large Telescope Interferometer providing the ESO community with spectrally-resolved, near-i…

astro-ph2008

Milli-arcsecond astrophysics with VSI, the VLTI spectro-imager in the ELT era

F. Malbet, D. Buscher, G. Weigelt +49

Nowadays, compact sources like surfaces of nearby stars, circumstellar environments of stars from early stages to the most evolved ones and surroundings of active galactic nuclei c…

astro-ph200649 cited

An asymmetry detected in the disk of Kappa CMa with the AMBER/VLTI

Anthony Meilland, Florentin Millour, Philippe Stee +7

Aims. We study the geometry and kinematics of the circumstellar environment of the Be star Kappa CMa in the Br gamma emission line and its nearby continuum. Methods. We use the VLT…

astro-ph200674 cited

Direct constraint on the distance of y2 Velorum from AMBER/VLTI observations

F. Millour, R. G. Petrov, O. Chesneau +95

In this work, we present the first AMBER observations, of the Wolf-Rayet and O (WR+O) star binary system y2 Velorum. The AMBER instrument was used with the telescopes UT2, UT3, and…

astro-ph2006108 cited

Near-Infrared interferometry of Eta Carinae with high spatial and spectral resolution using the VLTI and the AMBER instrument

G. Weigelt

We present the first NIR spectro-interferometry of the LBV Eta Carinae. The K band observations were performed with the AMBER instrument of the ESO Very Large Telescope Interferome…

astro-ph200666 cited

Constraining the wind launching region in Herbig Ae stars: AMBER/VLTI spectroscopy of HD104237

E. Tatulli, A. Isella, A. Natta +3

We investigate the origin of the emission of the Herbig Ae star HD104237 on Astronomical Unit (AU) scales. Using AMBER/VLTI at a spectral resolution R=1500 spatially…