An improved method for polarimetric image restoration in interferometry

Interferometric radio astronomy data require the effects of limited coverage in the Fourier plane to be accounted for via a deconvolution process. For the last 40 years this process, known as ‘cleaning’, has been performed almost exclusively on all Stokes parameters individually as if they were inde...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-11, Vol.462 (4), p.3483-3501
Hauptverfasser:	Pratley, Luke, Johnston-Hollitt, Melanie
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Arrays Astronomical polarimetry Cleaning Deconvolution Fourier transforms Interferometry Mathematical analysis Radio astronomy Vectors (mathematics)
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