articleThe Astrophysical JournalApr 10, 2006BRONZE OA

Angular Differential Imaging: A Powerful High‐Contrast Imaging Technique

CMChristian MaroisDLDavid LafreniereRDRene DoyonBMBruce MacintoshDNDaniel Nadeau

Lawrence Livermore National Laboratory · Université du Québec à Montréal · +1 more institution

Indexed inarxivcrossrefdoaj

Abstract

Angular differential imaging is a high-contrast imaging technique that reduces quasi-static speckle noise and facilitates the detection of nearby companions. A sequence of images is acquired with an altitude/azimuth telescope while the instrument field derotator is switched off. This keeps the instrument and telescope optics aligned and allows the field of view to rotate with respect to the instrument. For each image, a reference PSF is constructed from other appropriately-selected images of the same sequence and subtracted to remove quasi-static PSF structure. All residual images are then rotated to align the field and are combined. Observed performances are reported for Gemini North data. It is shown that…

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Authors

5
  • CM
    Christian MaroisCorresponding

    Lawrence Livermore National Laboratory, Université du Québec à Montréal, Université de Montréal

  • DL
    David Lafreniere

    Université du Québec à Montréal, Université de Montréal

  • RD
    Rene Doyon

    Université du Québec à Montréal, Université de Montréal

  • BM
    Bruce Macintosh

    Lawrence Livermore National Laboratory

  • DN
    Daniel Nadeau

    Université du Québec à Montréal, Université de Montréal

Topics & keywords

Keywords
  • Speckle pattern
  • Telescope
  • Speckle noise
  • Noise (video)
  • Field of view
  • Residual
  • Exoplanet
  • Angular resolution (graph drawing)
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