A high-contrast coronagraph for the MMT using phase apodization: Design and observations at 5 microns and 2 λ/D radius

J. L. Codona, M. A. Kenworthy, P. M. Hinz, J. R.P. Angel, N. J. Woolf

Research output: Chapter in Book/Report/Conference proceedingConference contribution

32 Scopus citations

Abstract

We report on the first implementation of phase apodization for high-contrast imaging at close inner working angle. It is designed for use in the 5 μm M band with the adaptive optics system at the MMT, which uses a deformable secondary for low thermal background and achieves a Strehl ratio of 90% at 5 μm. The method uses a diamond-turned ZnSe phase plate located at a cold pupil stop to diffract starlight into an "anti-halo" which suppresses the Airy diffraction pattern over a semi-circular region around the star. The design was optimized for strong suppression from the first bright Airy ring out to the control radius achievable with the MMT deformable secondary, about 9λ/D. The time-averaged PSF of a bright star agrees well with the design profile, the core with FWHM of 0.18 arcsec showing the diffraction-limited resolution of the full aperture. At 0.34 arcsec radius (2λ/D) the floor level is 3.5 × 10 -3 of the central peak, limited by residual atmospheric errors with 3 m wavelength across the aperture. The measured fluctuations at this radius averaged over 20 seconds are 2.5 × 10 -4 rms (9 magnitudes down from the peak). With the addition of active feedback to control residual speckles caused by static wavefront errors and with longer exposures, we project that exoplanet searches should reach 5σ sensitivity level > 10 magnitudes in an hour of integration.

Original languageEnglish (US)
Title of host publicationGround-based and Airborne Instrumentation for Astronomy
DOIs
StatePublished - Oct 9 2006
EventGround-based and Airborne Instrumentation for Astronomy - Orlando, FL, United States
Duration: May 25 2006May 29 2006

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume6269 I
ISSN (Print)0277-786X

Other

OtherGround-based and Airborne Instrumentation for Astronomy
CountryUnited States
CityOrlando, FL
Period5/25/065/29/06

Keywords

  • Extrasolar Planets
  • Phase Apodization
  • Phase Masks
  • Stellar Coronagraphs

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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    Codona, J. L., Kenworthy, M. A., Hinz, P. M., Angel, J. R. P., & Woolf, N. J. (2006). A high-contrast coronagraph for the MMT using phase apodization: Design and observations at 5 microns and 2 λ/D radius. In Ground-based and Airborne Instrumentation for Astronomy [62691N] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 6269 I). https://doi.org/10.1117/12.672727