We have recently shown that a posteriori co-phasing of multi-spectral interferograms was possible. 1 In this contribution, we extend our approach so that it can be applied to actual data as provided by Amber 2 or Matisse instruments. The main advantage of the proposed post-processing technique is that it requires no modifications of the...
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2016 (v1)Conference paperUploaded on: February 28, 2023
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October 9, 2018 (v1)Conference paper
The Evanescent Wave Coronagraph (EvWaCo) is a coronagraph with an occulting mask based on the frustration of total internal reflection to i) produce an achromatic extinction of the central star and ii) reveal the faint companion surrounding the star. Results obtained in laboratory conditions show contrast performance of a few 10-6 between 10...
Uploaded on: December 4, 2022 -
June 2008 (v1)Conference paper
LITpro is a software for fitting models on data obtained from various stellar optical interferometers, like the VLTI. As a baseline, for modeling the object, it provides a set of elementary geometrical and center-to-limb darkening functions, all combinable together. But it is also designed to make very easy the implementation of more specific...
Uploaded on: December 3, 2022 -
June 10, 2018 (v1)Conference paper
International audience
Uploaded on: December 3, 2022 -
2008 (v1)Journal article
International audience
Uploaded on: December 3, 2022 -
June 16, 2024 (v1)Conference paper
SAXO+ is a planned enhancement of the existing SAXO, the VLT/ SPHERE adaptive optics system, deployed on ESO's Very Large Telescope. This upgrade is designed to significantly enhance the instrument's capacity to detect and analyze young Jupiter-like planets. The pivotal addition in SAXO+ is a second-stage adaptive optics system featuring a...
Uploaded on: September 12, 2024 -
2009 (v1)Journal article
This paper presents a study of the atmospheric refraction and its effect on the light coupling efficiency in an instrument using single-mode optical fibers. We show the analytical approach which allowed us to assess the need to correct the refraction in J- and H-bands while observing with an 8-m Unit Telescope. We then developed numerical...
Uploaded on: December 3, 2022 -
August 1, 2014 (v1)Conference paper
International audience
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