Very long baseline interferometry. VI - Methods of spectral line VLBI

Details Very long baseline interferometry. VI - Methods of spectral line VLBI Very long baseline interferometry. VI - Methods of spectral line VLBI

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984poast..32..205b&link_type=abstract

Postepy Astronomii (ISSN 0032-5414), vol. 32, July-Dec. 1984, p. 205-219. In Polish.

Astronomy and Astrophysics

Astronomy

Data Reduction, Line Spectra, Very Long Base Interferometry, Data Correlation, Fourier Transformation, Theorem Proving

Scientific paper

This part deals with the final analysis of spectral line VLBI data obtained after correlation and postprocessing. The theoretical background for the analysis of differential observables is given. Principles of fringe rate mapping, multiple-point fringe rate mapping, phase modeling, aperture synthesis, and maser cluster distance determination are discussed. A generalized projection theorem is proved, which relates one-dimensional nonradial Fourier transforms taken on the spatial frequencies plane to these taken on the sky plane.

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