Fast Butterfly Epoch Folding-Based X-Ray Pulsar Period Estimation With a Few Distorted Profiles

The traditional pulsar period estimation method using a single distorted profile averts multiple epoch folding processes, but still has space for accuracy to improve. To give consideration to both accuracy and computational load, we combine the fast butterfly epoch folding (FBEF) with the single dis...

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Main Authors: Jin Liu, Lan-Lan Liu, Xiao-Lin Ning, Ting-Xuan Du, Zhi-Wei Kang
Format: Article
Language:English
Published: IEEE 2020-01-01
Series:IEEE Access
Subjects:
Online Access:https://ieeexplore.ieee.org/document/8945227/
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author Jin Liu
Lan-Lan Liu
Xiao-Lin Ning
Ting-Xuan Du
Zhi-Wei Kang
author_facet Jin Liu
Lan-Lan Liu
Xiao-Lin Ning
Ting-Xuan Du
Zhi-Wei Kang
author_sort Jin Liu
collection DOAJ
description The traditional pulsar period estimation method using a single distorted profile averts multiple epoch folding processes, but still has space for accuracy to improve. To give consideration to both accuracy and computational load, we combine the fast butterfly epoch folding (FBEF) with the single distorted profile (SDP)-based pulsar period estimation, and propose the FBEF-based pulsar period estimation with a few distorted profiles (FBEF-FDP), which merely uses a few epoch folding processes to enhance accuracy sharply. Firstly, the fast butterfly epoch folding is used to produce a few distorted pulsar profiles with different periods. And then the single distorted profile-based pulsar period estimation explores each distorted prolife to provide a corresponding distortion degree. Finally, using these distortion degree values, the nonlinear search method for multiple minimums can get an optimal distortion degree estimation. Besides, we prove that distortion degree estimation errors of different accumulative distorted profiles from the same pulsar photon sequence are incompletely correlated. This is the theorical basis that the distortion degree estimation values from the same pulsar photon sequence can be fitted to obtain more highly accurate distortion degree estimation. The computational complexity demonstrates that the computational load increases with the number of groups. Thus, to ensure the real-time of the FBEF-FDP, the number of groups should not be too large. Simulation results demonstrate that the accuracy of the fast butterfly epoch folding-based pulsar period estimation using a few distorted profiles enhances at the cost of a small computational load.
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spelling doaj.art-f1d85c90d63d4052ac0b3b29f875f0b82022-12-21T23:34:26ZengIEEEIEEE Access2169-35362020-01-0184211421910.1109/ACCESS.2019.29629778945227Fast Butterfly Epoch Folding-Based X-Ray Pulsar Period Estimation With a Few Distorted ProfilesJin Liu0https://orcid.org/0000-0002-1098-722XLan-Lan Liu1https://orcid.org/0000-0002-3414-522XXiao-Lin Ning2https://orcid.org/0000-0003-3563-3601Ting-Xuan Du3https://orcid.org/0000-0001-8674-0189Zhi-Wei Kang4https://orcid.org/0000-0002-3831-1811School of Information Science and Engineering, Wuhan University of Science and Technology, Wuhan, ChinaSchool of Information Science and Engineering, Wuhan University of Science and Technology, Wuhan, ChinaSchool of Instrumentation Science and Opto-Electronics Engineering, Beihang University (BUAA), Beijing, ChinaInternational School, Wuhan University of Science and Technology, Wuhan, ChinaCollege of Computer Science and Electronic Engineering, Hunan University, Changsha, ChinaThe traditional pulsar period estimation method using a single distorted profile averts multiple epoch folding processes, but still has space for accuracy to improve. To give consideration to both accuracy and computational load, we combine the fast butterfly epoch folding (FBEF) with the single distorted profile (SDP)-based pulsar period estimation, and propose the FBEF-based pulsar period estimation with a few distorted profiles (FBEF-FDP), which merely uses a few epoch folding processes to enhance accuracy sharply. Firstly, the fast butterfly epoch folding is used to produce a few distorted pulsar profiles with different periods. And then the single distorted profile-based pulsar period estimation explores each distorted prolife to provide a corresponding distortion degree. Finally, using these distortion degree values, the nonlinear search method for multiple minimums can get an optimal distortion degree estimation. Besides, we prove that distortion degree estimation errors of different accumulative distorted profiles from the same pulsar photon sequence are incompletely correlated. This is the theorical basis that the distortion degree estimation values from the same pulsar photon sequence can be fitted to obtain more highly accurate distortion degree estimation. The computational complexity demonstrates that the computational load increases with the number of groups. Thus, to ensure the real-time of the FBEF-FDP, the number of groups should not be too large. Simulation results demonstrate that the accuracy of the fast butterfly epoch folding-based pulsar period estimation using a few distorted profiles enhances at the cost of a small computational load.https://ieeexplore.ieee.org/document/8945227/Distortion measurementepoch foldingestimationsearch methodsX-ray pulsar
spellingShingle Jin Liu
Lan-Lan Liu
Xiao-Lin Ning
Ting-Xuan Du
Zhi-Wei Kang
Fast Butterfly Epoch Folding-Based X-Ray Pulsar Period Estimation With a Few Distorted Profiles
IEEE Access
Distortion measurement
epoch folding
estimation
search methods
X-ray pulsar
title Fast Butterfly Epoch Folding-Based X-Ray Pulsar Period Estimation With a Few Distorted Profiles
title_full Fast Butterfly Epoch Folding-Based X-Ray Pulsar Period Estimation With a Few Distorted Profiles
title_fullStr Fast Butterfly Epoch Folding-Based X-Ray Pulsar Period Estimation With a Few Distorted Profiles
title_full_unstemmed Fast Butterfly Epoch Folding-Based X-Ray Pulsar Period Estimation With a Few Distorted Profiles
title_short Fast Butterfly Epoch Folding-Based X-Ray Pulsar Period Estimation With a Few Distorted Profiles
title_sort fast butterfly epoch folding based x ray pulsar period estimation with a few distorted profiles
topic Distortion measurement
epoch folding
estimation
search methods
X-ray pulsar
url https://ieeexplore.ieee.org/document/8945227/
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