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Keiichi Ohnaka

Researcher at Catholic University of the North

Publications -  133
Citations -  4933

Keiichi Ohnaka is an academic researcher from Catholic University of the North. The author has contributed to research in topics: Very Large Telescope & Stars. The author has an hindex of 41, co-authored 131 publications receiving 4760 citations. Previous affiliations of Keiichi Ohnaka include Max Planck Society.

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Journal ArticleDOI

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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Radiative transfer modeling of three-dimensional clumpy AGN tori and its application to NGC 1068

TL;DR: In this article, a new method for modeling near-and mid-infrared emission of 3D clumpy tori using Monte Carlo simulations is presented, where the radiation fields of individual clouds at various distances from the AGN and distribute these clouds within the torus region are determined from a theoretical approach of self-gravitating clouds close to the shear limit.
Journal ArticleDOI

Radiative Transfer Modeling of Three-Dimensional Clumpy AGN Tori and its Application to NGC 1068

TL;DR: In this paper, the authors used Monte Carlo simulations to estimate the radiation fields of individual clouds at various distances from the AGN and distribute these clouds within the torus region, showing that clumpiness in AGN tori can overcome the problem of overpronounced silicate features.
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Tracing the young massive high-eccentricity binary system Theta 1 Orionis C through periastron passage

TL;DR: In this article, the authors used a near-infrared (H -a ndK-band) long-baseline interferometry with the ESO 3.6 m and the BTA 6 m telescopes (B � and V � -band) to reconstruct the first VLTI/AMBER closure-phase aperture synthesis image, showing the θ 1 Ori C system.