Paper 14145-287
Calibration of MEMS DM actuator gains using a Zernike wavefront sensor on the HiCAT testbed and implications for Habitable Worlds Observatory operations
9 July 2026 • 17:30 - 19:00 CEST | Room B4-M3
Abstract
Deformable mirrors (DMs) are critical for coronagraph operations on ground-based telescopes and future missions like HWO and Roman CGI. They enable wavefront control to create a high-contrast “dark zone” (DZ) for detecting faint companions. Achieving contrasts <1e-8 requires precise DM actuator-gain calibration, as picometer-level errors degrade DZ digging efficiency, increase overheads, and tighten stability requirements. Because DM gain varies with stroke, rapid in situ recalibration is needed. Zernike wavefront sensors (ZWFS) offer picometer sensitivity and will likely be onboard HWO, but their use for DM calibration remains unproven and has major operational implications. We present HiCAT testbed results calibrating gain maps for two 952-actuator BMC MEMS DMs with both a Fizeau interferometer and a ZWFS. We show that the ZWFS achieves sub-nm sensitivity and supports gain maps using local linear or quadratic models with implications for final DZ contrast and digging efficiency.
Presenter
Sarah Steiger
Space Telescope Science Institute (United States)
Sarah Steiger is an STScI Postdoctoral Research Fellow working with the Russell B. Makidon Optics Laboratory and Community Missions Office. She received her doctorate from the University of California, Santa Barbara in 2023 and is an expert in high-contrast imaging and superconducting detector technologies. Her current focus is in the development of new technologies to enable the exoplanet imaging goals of future flagship space observatories including detectors, coronagraphs, and wavefront sensing and control systems.