The LBTI Fizeau imager - I. Fundamental gain in high-contrast imaging

F. Patru, S. Esposito, A. Puglisi, A. Riccardi, E. Pinna, C. Arcidiacono, J. Antichi, B. Mennesson, D. Defrère, Philip M Hinz, J. M. Hill

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

We show by numerical simulations a fundamental gain in contrast when combining coherently monochromatic light from two adaptive optics (AO) telescopes instead of using a single stand-alone AO telescope, assuming efficient control and acquisition systems at high speed. A contrast gain map is defined as the normalized point spread functions (PSFs) ratio of a single Large Binocular Telescope (LBT) aperture over the dual Large Binocular Telescope Interferometer (LBTI) aperture in Fizeau mode. The global gain averaged across the AO-corrected field of view is improved by a factor of 2 in contrast in long exposures and by a factor of 10 in contrast in short exposures (i.e. in exposures, respectively, longer or shorter than the coherence time). The fringed speckle halo in short exposures contains not only highangular resolution information, as stated by speckle imaging and speckle interferometry, but also high-contrast imaging information. A high-gain zone is further produced in the valleys of the PSF formed by the dark Airy rings and/or the dark fringes. Earth rotation allows us to exploit various areas in the contrast gain map. A huge-contrast gain in narrow zones can be achieved when both a dark fringe and a dark ring overlap on to an exoplanet. Compared to a single 8-m LBT aperture, the 23-m LBTI Fizeau imager can provide a gain in sensitivity (by a factor of 4), a gain in angular resolution (by a factor of 3) and, as well, a gain in raw contrast (by a factor of 2-1000 varying over the AO-corrected field of view).

Original languageEnglish (US)
Pages (from-to)2544-2553
Number of pages10
JournalMonthly Notices of the Royal Astronomical Society
Volume472
Issue number3
DOIs
StatePublished - 2017

Fingerprint

interferometer
speckle
interferometers
telescopes
field of view
adaptive optics
Earth rotation
apertures
point spread functions
interferometry
valley
speckle interferometry
exposure
rings
extrasolar planets
angular resolution
high gain
simulation
valleys
halos

Keywords

  • Instrumentation: adaptive optics
  • Instrumentation: interferometers
  • Methods: numerical
  • Techniques: high angular resolution
  • Techniques: interferometric

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Patru, F., Esposito, S., Puglisi, A., Riccardi, A., Pinna, E., Arcidiacono, C., ... Hill, J. M. (2017). The LBTI Fizeau imager - I. Fundamental gain in high-contrast imaging. Monthly Notices of the Royal Astronomical Society, 472(3), 2544-2553. https://doi.org/10.1093/mnras/stx1961

The LBTI Fizeau imager - I. Fundamental gain in high-contrast imaging. / Patru, F.; Esposito, S.; Puglisi, A.; Riccardi, A.; Pinna, E.; Arcidiacono, C.; Antichi, J.; Mennesson, B.; Defrère, D.; Hinz, Philip M; Hill, J. M.

In: Monthly Notices of the Royal Astronomical Society, Vol. 472, No. 3, 2017, p. 2544-2553.

Research output: Contribution to journalArticle

Patru, F, Esposito, S, Puglisi, A, Riccardi, A, Pinna, E, Arcidiacono, C, Antichi, J, Mennesson, B, Defrère, D, Hinz, PM & Hill, JM 2017, 'The LBTI Fizeau imager - I. Fundamental gain in high-contrast imaging', Monthly Notices of the Royal Astronomical Society, vol. 472, no. 3, pp. 2544-2553. https://doi.org/10.1093/mnras/stx1961
Patru, F. ; Esposito, S. ; Puglisi, A. ; Riccardi, A. ; Pinna, E. ; Arcidiacono, C. ; Antichi, J. ; Mennesson, B. ; Defrère, D. ; Hinz, Philip M ; Hill, J. M. / The LBTI Fizeau imager - I. Fundamental gain in high-contrast imaging. In: Monthly Notices of the Royal Astronomical Society. 2017 ; Vol. 472, No. 3. pp. 2544-2553.
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AU - Puglisi, A.

AU - Riccardi, A.

AU - Pinna, E.

AU - Arcidiacono, C.

AU - Antichi, J.

AU - Mennesson, B.

AU - Defrère, D.

AU - Hinz, Philip M

AU - Hill, J. M.

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