An optimized algorithm for multiscale wideband deconvolution of radio astronomical images

被引:225
|
作者
Offringa, A. R. [1 ]
Smirnov, O. [2 ,3 ]
机构
[1] Netherlands Inst Radio Astron ASTRON, POB 2, NL-7990 AA Dwingeloo, Netherlands
[2] Rhodes Univ, Dept Phys & Elect, POB 94, ZA-6140 Grahamstown, South Africa
[3] SKA South Africa, 3rd Floor,Pk,Pk Rd, ZA-7405 Pinelands, South Africa
基金
新加坡国家研究基金会; 欧洲研究理事会;
关键词
instrumentation: interferometers; methods: observational; techniques: interferometric; radio continuum: general; INTERFEROMETRY; IMPLEMENTATION; CALIBRATION;
D O I
10.1093/mnras/stx1547
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe a new multiscale deconvolution algorithm that can also be used in a multifrequency mode. The algorithm only affects the minor clean loop. In single-frequency mode, the minor loop of our improved multiscale algorithm is over an order of magnitude faster than the CASA multiscale algorithm, and produces results of similar quality. For multifrequency deconvolution, a technique named joined-channel cleaning is used. In this mode, the minor loop of our algorithm is two to three orders of magnitude faster than CASA MSMFS. We extend the multiscale mode with automated scale-dependent masking, which allows structures to be cleaned below the noise. We describe a new scale-bias function for use in multiscale cleaning. We test a second deconvolution method that is a variant of the MORESANE deconvolution technique, and uses a convex optimization technique with isotropic undecimated wavelets as dictionary. On simple well-calibrated data, the convex optimization algorithm produces visually more representative models. On complex or imperfect data, the convex optimization algorithm has stability issues.
引用
收藏
页码:301 / 316
页数:16
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