Millisecond and Binary Pulsars as Nature's Frequency Standards. III. Fourier Analysis and Spectral Sensitivity of Timing Observations to Low-Frequency Noise

Details Millisecond and Binary Pulsars as Nature's Frequency Standards. III. Fourier Analysis and Spectral Sensitivity of Timing Observations to Low-Frequency Noise Millisecond and Binary Pulsars as Nature's Frequency Standards. III. Fourier Analysis and Spectral Sensitivity of Timing Observations to Low-Frequency Noise

2004-08-19

arxiv.org/abs/astro-ph/0408366v1

Mon. Not. Roy. Astron. Soc. 355 (2004) 395-412

Astronomy and Astrophysics

Astrophysics

25 pages, 3 figures, accepted to MNRAS

Scientific paper

10.1111/j.1365-2966.2004.08331.x

This paper discusses spectral sensitivity of solitary and binary pulsars to a
low-frequency (colored) noise. It is a third paper in a series of papers
devoted to analysis of the low-frequency noise in pulsar timing observations
and its impact on observable fitting parameters of timing model.

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