Research for Enhancing Weak Multi-Target's Tracks Based on Radon-Clean Algorithm

Author(s):  
Jun Wang ◽  
Junsheng Jiao
Keyword(s):  
2018 ◽  
Vol 618 ◽  
pp. A117 ◽  
Author(s):  
L. Zhang

Context. CLEAN algorithms are excellent deconvolution solvers that remove the sidelobes of the dirty beam to clean the dirty image. From the point of view of the scale, there are two types: scale-insensitive CLEAN algorithms, and scale-sensitive CLEAN algorithms. Scale-insensitive CLEAN algorithms perform excellently well for compact emission and perform poorly for diffuse emission, while scale-sensitive CLEAN algorithms are good for both point-like emission and diffuse emission but are often computationally expensive. However, observed images often contain both compact and diffuse emission. An algorithm that can simultaneously process compact and diffuse emission well is therefore required. Aims. We propose a new deconvolution algorithm by combining a scale-insensitive CLEAN algorithm and a scale-sensitive CLEAN algorithm. The new algorithm combines the advantages of scale-insensitive algorithms for compact emission and scale-sensitive algorithms for diffuse emission. At the same time, it avoids the poor performance of scale-insensitive algorithms for diffuse emission and the great computational load of scale-sensitive algorithms for compact emission in residuals. Methods. We propose a fuse mechanism to combine two algorithms: the Asp-Clean2016 algorithm, which solves the computationally expensive problem of convolution operation in the fitting procedure, and the classical Högbom CLEAN (Hg-Clean) algorithm, which is faster and works equally well for compact emission. It is called fused CLEAN (fused-Clean) in this paper. Results. We apply the fused-Clean algorithm to simulated EVLA data and compare it to widely used algorithms: the Hg-Clean algorithm, the multi-scale CLEAN (Ms-Clean), and the Asp-Clean2016 algorithm. The results show that it performs better and is computationally effective.


1988 ◽  
Vol 132 ◽  
pp. 291-294
Author(s):  
Peter H. Smith ◽  
Robert S. McMillan

A total of 48 nights of time series data have been obtained for the K giants: Arcturus, Pollux, and Aldebaran. A careful analysis of both single and multi–night sets using the earth's motion as a velocity calibrator has yielded stellar velocity time series accurate to ± 3 m/s per observation. Periodogram analyses of these sets have revealed the existence of oscillations with periods near 2.5 hrs and amplitudes of ± 5 m/s for both Pollux and Aldebaran, but not for Arcturus. Preliminary analysis of a 5-night set for Pollux using the CLEAN algorithm suggests at least three modes separated by about 35 microHertz.


2002 ◽  
Vol 199 ◽  
pp. 512-513
Author(s):  
Alan McPhail

The Filter CLEAN algorithm has been developed for CLEANing images containing a mixture of extended and fine-scale sources. Filter CLEAN requires fewer iterations and the residual rms is much lower than results from Högbom CLEAN. Filter CLEAN is particularly good at recovering extended sources while maintaining good resolution on fine-scale sources. The Filter CLEAN algorithm is described and results presented.


2017 ◽  
Vol 14 (1) ◽  
pp. 13-17 ◽  
Author(s):  
Fei Hu ◽  
Xiaohui Peng ◽  
Feng He ◽  
Liang Wu ◽  
Jun Li ◽  
...  

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