Wavefront tolerances of space-based segmented telescopes at very high contrast: Experimental validation
Iva Laginja, Jean-Fran\c{c}ois Sauvage, Laurent M. Mugnier and, Laurent Pueyo, Marshall D. Perrin, James Noss, Scott D. Will and, Keira J. Brooks, Emiel H. Por, Peter Petrone, R\'emi Soummer

TL;DR
This study experimentally validates an analytical model for wavefront error tolerances in segmented space telescopes, crucial for high-contrast imaging of exoEarths, using the HiCAT testbed.
Contribution
We experimentally validate an analytical wavefront error tolerancing model for segmented telescopes, linking it to contrast performance in high-contrast imaging systems.
Findings
The optical influence matrix was successfully measured on HiCAT.
Segment tolerances derived from the model achieved targeted contrast levels.
Analytical predictions of contrast mean and variance were confirmed experimentally.
Abstract
Context: The detection and characterization of Earth-like exoplanets (exoEarths) from space requires exquisite wavefront stability at contrast levels of . On segmented telescopes in particular, aberrations induced by cophasing errors lead to a light leakage through the coronagraph, deteriorating the imaging performance. These need to be limited in order to facilitate the direct imaging of exoEarths. Aims: We perform a laboratory validation of an analytical tolerancing model that allows us to determine wavefront error requirements in the contrast regime, for a segmented pupil with a classical Lyot coronagraph. We intend to compare the results to simulations, and we aim to establish an error budget for the segmented mirror on the High-contrast imager for Complex Aperture Telescopes (HiCAT) testbed. Methods: We use the Pair-based Analytical model for Segmented…
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