VLBI fringe-fitting with antenna-based residuals

Details VLBI fringe-fitting with antenna-based residuals VLBI fringe-fitting with antenna-based residuals

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...168..365a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 168, no. 1-2, Nov. 1986, p. 365-368.

Astronomy and Astrophysics

Astronomy

40

Data Processing, Radio Antennas, Radio Interferometers, Radio Sources (Astronomy), Very Long Base Interferometry, Algorithms, Amplitudes, Correlation Coefficients, Frequency Standards, Signal To Noise Ratios

Scientific paper

A procedure for Very Long Baseline Interferometry (VLBI) fringe-fitting incorporating antenna-based delay and rate residuals is described. The method, although not as powerful as the Global Fringe Search technique of Schwab and Cotton (1983), makes only modest demands on computing resources and does not require an initial estimate of the source structure. The method is easily used for both narrowband and wideband VLBI data, and can be incorporated into the standard data reduction chain.

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