Low wind and petaling effects, caused by the discontinuous apertures of telescopes, are poorly corrected -- if at all -- by commonly used workhorse wavefront sensors (WFSs). Wavefront petaling breaks the coherence of the point spread function core, splitting it into several side lobes, dramatically shutting off scientific throughput. We demonstrate the re-purposing of non-redundant sparse aperture masking (SAM) interferometers into low-order WFSs complementing the high-order pyramid WFS, on the SCExAO experimental platform at Subaru Telescope. The SAM far-field interferograms formed from a 7-hole mask are used for direct retrieval of petaling aberrations, which are almost invisible to the main AO loop. We implement a visible light dual-band SAM mode, using two disjoint 25 nm wide channels, that we recombine to overcome the one-lambda ambiguity of fringe-tracking techniques. This enables a control over petaling with sufficient capture range yet without conflicting with coronagraphic modes in the near-infrared. We present on-sky engineering results demonstrating that the design is able to measure petaling well beyond the range of a single-wavelength equivalent design.
@article{arxiv.2209.02898,
title = {Controlling petals using fringes: discontinuous wavefront sensing through sparse aperture interferometry at Subaru/SCExAO},
author = {Vincent Deo and Sébastien Vievard and Nick Cvetojevic and Kyohoon Ahn and Elsa Huby and Olivier Guyon and Sylvestre Lacour and Julien Lozi and Frantz Martinache and Barnaby Norris and Nour Skaf and Peter Tuthill},
journal= {arXiv preprint arXiv:2209.02898},
year = {2022}
}
Comments
Proc. SPIE 12185 (Adaptive Optics Systems VIII), 285-297