Interferometric apodization by homothety -- I. Optimization of the device parameters

TL;DR

This paper introduces an interferometric apodization method using homothety for high-contrast imaging, optimizing device parameters to improve coronagraph sensitivity for exoplanet detection.

Contribution

It presents a novel apodization technique with experimental setup and optimization, achieving high light concentration and promising contrast levels for exoplanet imaging.

Findings

Achieved 93.6% light concentration for circular aperture

Simulated contrast of approximately 10^-4 at 1.8λ/D

Demonstrated effectiveness with various aperture geometries

Abstract

This study is focused on the very high dynamic imaging field, specifically the direct observation of exoplanetary systems. The coronagraph is an essential technique for suppressing the star's light, making it possible to detect an exoplanet with a very weak luminosity compared to its host star. Apodization improves the rejection of the coronagraph, thereby increasing its sensitivity. This work presents the apodization method by interferometry using homothety, with either a rectangular or circular aperture. We discuss the principle method, the proposed experimental setup, and present the obtained results by optimizing the free parameters of the system while concentrating the maximum of the light energy in the central diffraction lobe, with a concentration rate of 93.6\% for the circular aperture and 91.5\% for the rectangular geometry. The obtained results enabled scaling the various elements of the experiment in accordance with practical constraints. Simulation results are presented for both circular and rectangular apertures. We performed simulations on a hexagonal aperture, both with and without a central obstruction, as well as a segmented aperture similar to the one used in the Thirty Meter Telescope (TMT). This approach enables the attainment of a contrast of approximately $10^{-4}$ at small angular separations, specifically around $1.8\lambda/D$. When integrated with a coronagraph, this technique exhibits great promise. These findings confirm that our proposed technique can effectively enhance the performance of a coronagraph.