4.3 Article

The adaptive-loop-gain adaptive-scale CLEAN deconvolution of radio interferometric images

Journal

ASTROPHYSICS AND SPACE SCIENCE
Volume 361, Issue 5, Pages -

Publisher

SPRINGER
DOI: 10.1007/s10509-016-2746-8

Keywords

Methods: data analysis; Techniques: image processing

Funding

  1. National Basic Research Program of China (973 program) [2012CB821804, 2015CB857100]
  2. National Science Foundation of China [11103055]
  3. West Light Foundation of the Chinese Academy of Sciences [RCPY201105]

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CLEAN algorithms are a class of deconvolution solvers which are widely used to remove the effect of the telescope Point Spread Function (PSF). Loop gain is one important parameter in CLEAN algorithms. Currently the parameter is fixed during deconvolution, which restricts the performance of CLEAN algorithms. In this paper, we propose a new deconvolution algorithm with an adaptive loop gain scheme, which is referred to as the adaptive-loop-gain adaptive-scale CLEAN (Algas-Clean) algorithm. The test results show that the new algorithm can give a more accurate model with faster convergence.

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