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A Linear Decomposition Method to Analyze and Study Pulsar Mode Changes

delete2025-04-07
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OA
AI
L
Longfei Hao *
Z
Zhixuan Li
F
Faxin Shen
Y
Yonghua Xu
Y
Y. Huang
K
Kejia Lee
Q
Qingzheng Yu
H
H. G. Wang
DOI:10.3847/1538-4357/adbdb8delete
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Abstract

Abstract

En 中文
In this paper, we present the linear decomposition method (LDM), which we developed to detect and analyze pulsar profile variations and mode-changing behavior. We developed LDM utilizing the likelihood function approach assuming the Gaussian noise. The LDM projects pulse profiles onto significance-ordered orthonormal vector bases. We show that the method is similar to the principal component analysis, but the LDM can handle more general situations. We use a simulated data set and data from the Kunming 40 m radio telescope to demonstrate the application of the LDM. We found that the LDM successfully identified mode changes for well-known mode-changing PSR B0329+54 and found a continuous pulse profile evolution for PSR B0355+54. We also show that the LDM can be used to improve the timing precision for mode-changing PSR B0329+54.
Keywords:
RAY

Journal

Astrophysical Journal cover
Astrophysical Journal
IF:
5.4
Papers:
8.3W
Citations:
32.0W

Organization

B
beijing laser accelerat innovat ctr
Scholars:
7
Papers: 6
Citations: 0
C
chinese acad sci
Scholars:
1.8W
Papers: 1.1W
Citations: 4.6K