Experimental study of a low-order wavefront sensor for the high-contrast coronagraphic imager EXCEDE

TL;DR

This study evaluates a low-order wavefront sensor for the EXCEDE mission, demonstrating significant contrast improvements by controlling tip/tilt aberrations in a high-contrast coronagraphic imaging system.

Contribution

It presents an experimental validation of a LOWFS that effectively reduces low-order aberrations, enhancing contrast performance in a simulated exoplanet imaging system.

Findings

LOWFS reduced tip/tilt disturbances to 1e-3 lambda/D rms

Contrast improved to 8e-7 between 1.2 and 2 lambda/D

LQG controller is being implemented for further improvements

Abstract

The mission EXCEDE (EXoplanetary Circumstellar Environments and Disk Explorer), selected by NASA for technology development, is designed to study the formation, evolution and architectures of exoplanetary systems and characterize circumstellar environments into stellar habitable zones. It is composed of a 0.7 m telescope equipped with a Phase-Induced Amplitude Apodization Coronagraph (PIAA-C) and a 2000-element MEMS deformable mirror, capable of raw contrasts of 1e-6 at 1.2 lambda/D and 1e-7 above 2 lambda/D. One of the key challenges to achieve those contrasts is to remove low-order aberrations, using a Low-Order WaveFront Sensor (LOWFS). An experiment simulating the starlight suppression system is currently developed at NASA Ames Research Center, and includes a LOWFS controlling tip/tilt modes in real time at 500 Hz. The LOWFS allowed us to reduce the tip/tilt disturbances to 1e-3 lambda/D rms, enhancing the previous contrast by a decade, to 8e-7 between 1.2 and 2 lambda/D. A Linear Quadratic Gaussian (LQG) controller is currently implemented to improve even more that result by reducing residual vibrations. This testbed shows that a good knowledge of the low-order disturbances is a key asset for high contrast imaging, whether for real-time control or for post processing.