2016AJ....152..131W


Query : 2016AJ....152..131W

2016AJ....152..131W - Astron. J., 152, 131-131 (2016/November-0)

Pulsar signal denoising method based on Laplace distribution in no-subsampling wavelet packet domain.

WENBO W., YANCHAO Z. and XIANGLI W.

Abstract (from CDS):

In order to improve the denoising effect of the pulsar signal, a new denoising method is proposed in the no-subsampling wavelet packet domain based on the local Laplace prior model. First, we count the true noise-free pulsar signal's wavelet packet coefficient distribution characteristics and construct the true signal wavelet packet coefficients' Laplace probability density function model. Then, we estimate the denosied wavelet packet coefficients by using the noisy pulsar wavelet coefficients based on maximum a posteriori criteria. Finally, we obtain the denoisied pulsar signal through no-subsampling wavelet packet reconstruction of the estimated coefficients. The experimental results show that the proposed method performs better when calculating the pulsar time of arrival than the translation-invariant wavelet denoising method.

Abstract Copyright: © 2016. The American Astronomical Society. All rights reserved.

Journal keyword(s): astrometry - galaxies: fundamental parameters - methods: data analysis - pulsars: general - pulsars: general

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR B1451-68 Psr 14 56 00.0175876848 -68 43 40.034742348           ~ 203 0
2 PSR B1919+21 Psr 19 21 44.815 +21 53 02.25           ~ 411 0
3 PSR B1953+29 Psr 19 55 27.8680959374 +29 08 43.499227152           ~ 303 1

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