English

Characterization of deformable mirrors for the MagAO-X project

Instrumentation and Methods for Astrophysics 2018-07-13 v1 Earth and Planetary Astrophysics

Abstract

The MagAO-X instrument is an upgrade of the Magellan AO system that will introduce extreme adaptive optics capabilities for high-contrast imaging at visible and near-infrared wavelengths. A central component of this system is a 2040-actuator microelectromechanical (MEMS) deformable mirror (DM) from Boston Micromachines Corp. (BMC) that will operate at 3.63 kHz for high-order wavefront control. Two additional DMs from ALPAO will perform low-order and non-common-path science-arm wavefront correction. The accuracy of the wavefront correction is limited by our ability to command these DMs to a desired shape, which requires a careful characterization of each DM surface. We have developed a characterization pipeline that uses a Zygo Verifire Interferometer to measure the surface response and a Karhunen-Lo\`eve transform to remove noise from our measurements. We present our progress in the characterization process and the results of our pipeline applied to an ALPAO DM97 and a BMC Kilo-DM, demonstrating the ability to drive the DMs to a flat of \lesssim 2nm and \lesssim 4nm RMS in our beam footprint on the University of Arizona Wavefront Control (UAWFC) testbed.

Keywords

Cite

@article{arxiv.1807.04370,
  title  = {Characterization of deformable mirrors for the MagAO-X project},
  author = {Kyle Van Gorkom and Kelsey L. Miller and Jared R. Males and Olivier Guyon and Alexander T. Rodack and Jennifer Lumbres and Justin M. Knight},
  journal= {arXiv preprint arXiv:1807.04370},
  year   = {2018}
}

Comments

7 pages, 10 figures, SPIE Astronomical Telescopes + Instrumentation 2018