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Optical Interferometry in the Multi-Speckle Mode

  • Conference paper
Very High Angular Resolution Imaging

Part of the book series: International Astronomical Union / Union Astronomique Internationale ((IAUS,volume 158))

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Abstract

We have studied interferometric imaging in the multi-speckle mode by computer sim­ulations. From various simulated data sets diffraction-limited images were reconstructed by the speckle masking method and the iterative building block method. The reconstructed images show the dependence of the signal-to-noise ratio on photon noise.

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References

  • Hofmann K.-H., Weigelt G.: 1990, ‘Image Reconstruction from the Bispectrum Using an Iterative Algorithm, Applications of the Method to Astronomical Objects’, in: Optics in Complex Sys­tems, ICO 1990, eds. F. Lanzl, H.-J. Preuss, G. Weigelt Soc. Photo-Opt. Instr. Eng. 1319, 444

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Author information

Authors and Affiliations

  1. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 5300 Bonn 1, Germany

    T. Reinheimer, K.-H. Hofmann & G. Weigelt

Authors
  1. T. Reinheimer
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  2. K.-H. Hofmann
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  3. G. Weigelt
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Editor information

Editors and Affiliations

  1. School of Physics, University of Sydney, New South Wales, Australia

    J. G. Robertson  & W. J. Tango  & 

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© 1994 Springer Science+Business Media Dordrecht

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Reinheimer, T., Hofmann, KH., Weigelt, G. (1994). Optical Interferometry in the Multi-Speckle Mode. In: Robertson, J.G., Tango, W.J. (eds) Very High Angular Resolution Imaging. International Astronomical Union / Union Astronomique Internationale, vol 158. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0880-5_71

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  • DOI: https://doi.org/10.1007/978-94-011-0880-5_71

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-2633-5

  • Online ISBN: 978-94-011-0880-5

  • eBook Packages: Springer Book Archive

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