Imaging in Interferometry

  • Oskar Von Der Lühe
  • Nancy Ageorges
Part of the NATO Science Series C: (closed) book series (ASIC, volume 501)

Abstract

The goal of imaging with interferometers is to obtain an estimate of the spectral flux Iλ(ā) of the source of interest, as a function of two-dimensional angular coordinates \(\bar \alpha \) on the celestial sphere, with an angular resolution that corresponds to the maximum baseline in the array, and which is consistent with the observations.

Keywords

Optical Path Difference Double Star Object Phase Radio Interferometer Projected Baseline 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. 1.
    Bracewell, Ronald N., The Fourier Transform and Its Applications, 2nd. Ed., McGraw-Hill 1992Google Scholar
  2. 2.
    Goodman, Joseph W., Statistical Optics, Wiley and Sons 1985Google Scholar
  3. 3.
    Perley, Schwab, Bridle, Synthesis Imaging in Radio Interferometry, A. S. P. Series 6, 1989Google Scholar

Copyright information

© Kluwer Academic Publishers 1997

Authors and Affiliations

  • Oskar Von Der Lühe
    • 1
  • Nancy Ageorges
    • 1
  1. 1.European Southern ObservatoryGarchingGermany

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