|The Australia Telescope National Facility Colloquium|
|15:00-16:00 Wed 04 Jul 2018|
Marsfield lecture theatre
(University of Manchester)
Chris Skipper Colloquium: Cleaning radio interferometric images using a spherical wavelet decomposition.
The deconvolution, or cleaning, of radio interferometric images requires that model visibilities are calculated from a list of clean components, in order that the contribution from the model can be subtracted from the observed visibilities. This step is normally performed using a forward fast Fourier transform (FFT), followed by a ’degridding’ step that interpolates over the uv plane to construct the model visibilities. An alternative approach is to the calculate the model visibilities directly by summing over all the members of the clean component list, which is a more accurate method that can also be much slower. However, if the clean components are used to construct a model image on the surface of the celestial sphere then the model visibilities can be generated directly from the wavelet coefficients, and the sparsity of the model means that most of these coefficients are zero, and can be ignored. We have constructed a prototype imager that uses a spherical-wavelet representation of the model image to generate model visibilities during each major cycle, and in this talk I will discuss the implementation, performance and potential advantages of using such a technique to clean wide-field radio images.
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