Lyot-based Low Order Wavefront Sensor for Phase-mask Coronagraphs: Principle, Simulations and Laboratory Experiments
Garima Singh, Frantz Martinache, Pierre Baudoz, Olivier Guyon, Taro, Matsuo, Nemanja Jovanovic, Christophe Clergeon

TL;DR
This paper introduces a Lyot-based low order wavefront sensor adapted for phase-mask coronagraphs, demonstrating high sensitivity and accuracy in simulations and laboratory experiments for correcting low order aberrations.
Contribution
The paper presents a novel Lyot-based wavefront sensor that effectively measures low order aberrations in phase-mask coronagraphs, enhancing high-contrast imaging capabilities.
Findings
Achieves approximately 10^-2 lambda/D measurement accuracy in simulations.
Demonstrates 10^-2 lambda/D accuracy in laboratory experiments.
Provides a linear reconstruction method with high sensitivity for tip-tilt errors.
Abstract
High performance coronagraphic imaging of faint structures around bright stars at small angular separations requires fine control of tip, tilt and other low order aberrations. When such errors occur upstream of a coronagraph, they results in starlight leakage which reduces the dynamic range of the instrument. This issue has been previously addressed for occulting coronagraphs by sensing the starlight before or at the coronagraphic focal plane. One such solution, the coronagraphic low order wave-front sensor (CLOWFS) uses a partially reflective focal plane mask to measure pointing errors for Lyot-type coronagraphs. To deal with pointing errors in low inner working angle phase mask coronagraphs which do not have a reflective focal plane mask, we have adapted the CLOWFS technique. This new concept relies on starlight diffracted by the focal plane phase mask being reflected by the Lyot…
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