Source analysis on radio maps from the Cambridge Low Frequency Synthesis Telescope

An earlier paper by Waldram & McGilchrist has described the use of beam-sets in the analysis of wide-field maps from the Cambridge Low Frequency Synthesis Telescope (CLFST) to produce source catalogues. There the main emphasis was on the application of the method to unresolved point sources. Thi...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society Vol. 265; no. 4; pp. 853 - 866
Main Authors: Waldram, E. M., Riley, J. M.
Format: Journal Article
Language:English
Published: Oxford, UK Oxford University Press 15-12-1993
Blackwell Science
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Summary:An earlier paper by Waldram & McGilchrist has described the use of beam-sets in the analysis of wide-field maps from the Cambridge Low Frequency Synthesis Telescope (CLFST) to produce source catalogues. There the main emphasis was on the application of the method to unresolved point sources. This paper contains more details of source analysis on the CLFST, including the treatment of extended, complex and confused sources. We consider the errors – in particular, ionosphere phase errors – which can affect the synthesized beam-shape and hence the accuracy of the source parameters. Our aim is to make the whole process of reduction of maps to source catalogues as automatic and objective as possible.
Bibliography:istex:017996BD1DE0BE3B786BD476CE68A45ABE8D7747
ark:/67375/HXZ-MCNLN2XR-R
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/265.4.853