As instruments have become increasingly efficient and accurate, the detection and characterization of exoplanets has become a rapidly expanding field of research. However, the data provided are always dependent on the host stars' parameters. For example, the radial velocity measurements allow the ratio Mp sin(i)/M* to be determined, while the...
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November 20, 2013 (v1)PublicationUploaded on: March 25, 2023
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June 19, 2018 (v1)Journal article
The characterization of exoplanets relies on that of their host star. However, stellar evolution models cannot always be used to derive the mass and radius of individual stars, because many stellar internal parameters are poorly constrained. Here, we use the probability density functions (PDFs) of directly measured parameters to derive the...
Uploaded on: December 4, 2022 -
July 1, 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
July 17, 2022 (v1)Conference paper
Kernel phase is a method to interpret stellar point source images by considering their formation as the analytical result of an interferometric process. Using Fourier formalism, this method allows for observing planetary companions around nearby stars at separations down to half a telescope resolution element, typically 20 mas for a 8m class...
Uploaded on: December 3, 2022 -
August 2023 (v1)Journal article
Context. The conventional approach to direct imaging is to use a single aperture coronagraph with wavefront correction via extreme adaptive optics (AO). Such systems are limited to observing beyond an inner working angle (IWA) of a few λ / D. Nulling interferometry with two or more apertures will enable detections of companions at separations...
Uploaded on: November 25, 2023 -
August 25, 2021 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
June 10, 2022 (v1)Journal article
The use of interferometric nulling for the direct characterization of extrasolar planets is an exciting prospect, but one that faces many practical challenges when deployed on telescopes. The largest limitation is the extreme sensitivity of nullers to any residual optical path differences between the incoming telescope beams even after adaptive...
Uploaded on: December 3, 2022 -
December 2021 (v1)Journal article
Very Large Telescope Inerferometer (VLTI) schools have nearly a 20-year history and have trained a significant fraction of today's optical interferometrists who use high-angular-resolution techniques on a regular basis. Very early in the development of the VLTI, training was identified by the community as a necessary tool, as the expertise in...
Uploaded on: December 4, 2022 -
August 2022 (v1)Journal article
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Uploaded on: November 30, 2023