High performance piaa coronagraphy with complex amplitude focal plane masks

Olivier Guyon, Frantz Martinache, Ruslan Belikov, Remi Soummer

Research output: Contribution to journalArticle

82 Citations (Scopus)

Abstract

We describe a coronagraph approach where the performance of a Phase-Induced Amplitude Apodization (PIAA) coronagraph is improved by using a partially transmissive phase-shifting focal plane mask and a Lyot stop. This approach combines the low inner working angle offered by phase mask coronagraphy, the full throughput and uncompromized angular resolution of the PIAA approach, and the design flexibility of Apodized Pupil Lyot Coronagraph. A PIAA complex mask coronagraph (PIAACMC) is fully described by the focal plane mask size, or, equivalently, its complex transmission which ranges from 0 (opaque) to -1 (phase shifting). For all values of the transmission, the PIAACMC theoretically offers full on-axis extinction and 100% throughput at large angular separations. With a pure phase focal plane mask (complex transmission = -1), the PIAACMC offers 50% throughput at 0.64 λ/D while providing total extinction of an on-axis point source. This performance is very close to the "fundamental performance limit" of coronagraphy derived from first principles. For very high contrast level, imaging performance with PIAACMC is in practice limited by the angular size of the on-axis target (usually a star). We show that this fundamental limitation must be taken into account when choosing the optimal value of the focal plane mask size in the PIAACMC design. We show that the PIAACMC enables visible imaging of Jupiter-like planets at ≈1.2 λ/D from the host star, and can therefore offer almost three times more targets than a PIAA coronagraph optimized for this type of observation. We find that for visible imaging of Earthlike planets, the PIAACMC gain over a PIAA is probably much smaller, as coronagraphic performance is then strongly constrained by stellar angular size. For observations at "low" contrast (below ≈108), the PIAACMC offers significant performance enhancement over PIAA. This is especially relevant for ground-based high contrast imaging systems in the near-IR, where PIAACMC enables high contrast high efficiency imaging within 1 λ/D. Manufacturing tolerances for the focal plane mask are quantified for a few representative PIAACMC designs.

Original languageEnglish (US)
Pages (from-to)220-232
Number of pages13
JournalAstrophysical Journal, Supplement Series
Volume190
Issue number2
DOIs
StatePublished - Oct 2010

Fingerprint

coronagraphs
masks
apodization
planet
extinction
Jupiter
point source
manufacturing
tolerance
stars
pupils
angular resolution
Jupiter (planet)
point sources
planets
flexibility

Keywords

  • Instrumentation: adaptive optics
  • Techniques: high angular resolution

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

High performance piaa coronagraphy with complex amplitude focal plane masks. / Guyon, Olivier; Martinache, Frantz; Belikov, Ruslan; Soummer, Remi.

In: Astrophysical Journal, Supplement Series, Vol. 190, No. 2, 10.2010, p. 220-232.

Research output: Contribution to journalArticle

Guyon, Olivier ; Martinache, Frantz ; Belikov, Ruslan ; Soummer, Remi. / High performance piaa coronagraphy with complex amplitude focal plane masks. In: Astrophysical Journal, Supplement Series. 2010 ; Vol. 190, No. 2. pp. 220-232.
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