2018
conference-paper
OpenAlex
A. Boccaletti, Pierre Riaud, Pierre Baudoz, J. Baudrand et autres
MIRI, the mid-IR instrument of JWST (JamesWebb Space Telescope), will include a coronagraphic device for which the ultimate goal is the detection and caracterization of extrasolar planets around nearby stars. In this paper, we describe the optical concept of MIRI and the …
fr, be
(code pays fourni par la source)
2016
conference-paper
OpenAlex
Erick Bondoux, S. Bosio, Rijuparna Chakraborty, Wassila Dali-Ali et autres
Hypertelescopes are large optical interferometric arrays, employing many small mirrors and a miniature pupildensifier before the focal camera, expected to produce direct images of celestial sources at high resolution. Their peculiar imaging properties, initially explored through analytical derivations, had been verified with …
fr
(code pays fourni par la source)
Accès ouvert
2015
article
OpenAlex
Dominique Sluse, Damien Hutsemékers, T. Anguita, L. Braibant et autres
\n Testing the standard Shakura-Sunyaev model of accretion is a challenging task because the central region of quasars where accretion takes place is unresolved with telescopes. The analysis of microlensing in gravitationally lensed quasars is one of the few techniques that can …
be, cl, fr
(code pays fourni par la source)
Accès ouvert
2014
article
OpenAlex
Pierre Riaud
The vector vortex coronagraph is a phase mask creating a phase ramp around its optical axis to cancel on-axis starlight in the focal plane of a telescope. This phase ramp also induces an orbital angular momentum (OAM) on the output stellar photons, …
Accès ouvert
2014
conference-paper
OpenAlex
Denis Defrère, Olivier Absil, C. Hanot, Pierre Riaud et autres
Measuring the angular diameter of celestial bodies has long been the main purpose of stellar interferometry and was its historical motivation. Nowadays, stellar interferometry is widely used for various other scientific purposes that require very high angular resolution measurements. In terms of …
be, fr, de
(code pays fourni par la source)
Accès ouvert
2014
article
OpenAlex
Paul D. Nuñez, A. Labeyrie, Pierre Riaud
Optical interferometry has been successful at achieving milliarcsecond resolution on bright stars. Imaging performance can improve greatly by increasing the number of baselines, which has motivated proposals to build large (∼100 m) optical interferometers with tens to hundreds of telescopes. It is …
fr
(code pays fourni par la source)
2012
article
OpenAlex
Dimitri Mawet, Olivier Absil, G. Montagnier, Pierre Riaud et autres
Context. Most exoplanet imagers consist of ground-based adaptive optics coronagraphic cameras which are currently limited in contrast, sensitivity and astrometric precision, but advantageously observe in the near-infrared window (1–5 μm). Because of these practical limitations, our current observational aim at detecting and …
us, cl, be, fr
(code pays fourni par la source)
Accès ouvert
2012
article
OpenAlex
Pierre Riaud
This paper presents a new architecture for deformable mirrors, suitable for adaptive optics (AO) observations. The performance of these systems directly depends on the density of actuators, which correct for wavefront errors. Therefore, deformable mirrors of large sizes are difficult to build …
be
(code pays fourni par la source)
Accès ouvert
2012
article
OpenAlex
Pierre Riaud, Dimitri Mawet, A. Magette
Coronagraphs are used as high-contrast imaging tools. However, it is well-known that the achievable contrast is primarily limited by wavefront aberrations in the optical train. Various kinds of devices and methods have been proposed to correct and calibrate these errors and, hence, …
be, us, cl
(code pays fourni par la source)
Accès ouvert
2012
article
OpenAlex
Pierre Riaud, Dimitri Mawet, A. Magette
We introduce a novel phase retrieval method for astronomical applications based on the Nijboer-Zernike (NZ) theory of diffraction. We present a generalized NZ phase retrieval process that is not limited to small and symmetric aberrations and can therefore be directly applied to …
be, us, cl
(code pays fourni par la source)
Accès ouvert
2012
article
OpenAlex
Dimitri Mawet, Olivier Absil, G. Montagnier, Pierre Riaud et autres
Context. Most exoplanet imagers consist of ground-based adaptive optics coronagraphic cameras which are currently limited in contrast, sensitivity and astrometric precision, but advantageously observe in the near-infrared window (1–5 μm). Because of these practical limitations, our current observational aim at detecting and …
us, cl, be, fr
(code pays fourni par la source)
2012
article
OpenAlex
Pierre Riaud
be
(code pays fourni par la source)