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

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dc.creatorKopeikin, Sergei M.
dc.creatorPotapov, Vladimir A.
dc.date2004-08-19
dc.date.accessioned2026-07-07T06:29:34Z
dc.date.available2026-07-07T06:29:34Z
dc.descriptionThis 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.
dc.description25 pages, 3 figures, accepted to MNRAS
dc.identifierhttps://arxiv.org/abs/astro-ph/0408366
dc.identifierhttp://arxiv.org/abs/astro-ph/0408366
dc.identifierMon. Not. Roy. Astron. Soc. 355 (2004) 395-412
dc.identifierdoi:10.1111/j.1365-2966.2004.08331.x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98075
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectData Analysis, Statistics and Probability
dc.titleMillisecond and Binary Pulsars as Nature's Frequency Standards. III. Fourier Analysis and Spectral Sensitivity of Timing Observations to Low-Frequency Noise
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