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J. M. Clausse

Researcher at Centre national de la recherche scientifique

Publications -  26
Citations -  1409

J. M. Clausse is an academic researcher from Centre national de la recherche scientifique. The author has contributed to research in topics: Interferometry & Astronomical interferometer. The author has an hindex of 13, co-authored 26 publications receiving 1353 citations.

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AMBER, the near-infrared spectro-interferometric three-telescope VLTI instrument

Romain Petrov, +98 more
TL;DR: AMBER as mentioned in this paper is one of the VLTI instruments that combines up to three beams with low, moderate and high spectral resolutions in order to provide milli-arcsecond spatial resolution for compact astrophysical sources in the near-infrared wavelength domain.
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Interferometric data reduction with AMBER/VLTI. Principle, estimators, and illustration.

E. Tatulli, +101 more
TL;DR: In this article, a data reduction method for single-mode interferometry is presented based on a direct modelling of the fringes in the detector plane, which can be derived for any single-source interferometer.
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Near-infrared interferometry of eta Carinae with spectral resolutions of 1 500 and 12 000 using AMBER/VLTI

Gerd Weigelt, +103 more
TL;DR: The first NIR spectro-interferometry of the LBV? Carinae was performed with the AMBER instrument of the ESO Very Large Telescope Interferometer (VLTI) using baselines from 42 to 89 m as mentioned in this paper.
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Disk and wind interaction in the young stellar object MWC 297 spatially resolved with VLTI/AMBER

TL;DR: In this paper, a model of the stellar environment that combines a geometrically thin, optically thick accretion disk model consisting of gas and dust, and a latitude-dependent stellar wind outflowing above the disk surface is presented.
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Constraining the wind launching region in Herbig Ae stars: AMBER/VLTI spectroscopy of HD 104237

E. Tatulli, +103 more
TL;DR: In this paper, the authors investigated the origin of the Herbig-Ae star HD-104237 on AU-scale using AMBER/VLTI at a spectral resolution and showed that the line and the continuum emission have similar size scales.