2025ApJ...983...63H


Query : 2025ApJ...983...63H

2025ApJ...983...63H - Astrophys. J., 983, 63 (2025/April-2)

A Linear Decomposition Method to Analyze and Study Pulsar Mode Changes.

HAO L., LI Z., SHEN F., XU Y., HUANG Y., LEE K., YU Q. and WANG H.

Abstract (from CDS):

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.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Radio pulsars

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 B0329+54 Psr 03 32 59.3370698592 +54 34 45.028206408           ~ 690 1
2 PSR B0355+54 Psr 03 58 53.7165 +54 13 13.727           ~ 465 1
3 PSR B1237+25 Psr 12 39 40.386 +24 53 49.87           ~ 497 1

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