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

Abstract

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.

25 pages, 3 figures, accepted to MNRAS

References in corpus (5)

• Gravitational Waves Probe the Coalescence Rate of Massive Black Hole Binaries
• A test of general relativity from the three-dimensional orbital geometry of a binary pulsar
• A New Method for Obtaining Binary Pulsar Distances and its Implications for Tests of General Relativity
• Characterization of the Crab Pulsar's Timing Noise
• Millisecond and Binary Pulsars as Nature's Frequency Standards. II. Effects of Low-Frequency Timing Noise on Residuals and Measured Parameters

Cited by in corpus (9)

• Measuring the evolution of the most stable optical clock G 117-B15A
• Variance of the Hellings-Downs Correlation
• Searching For Stochastic Gravitational Waves Below a Nanohertz
• Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations
• Using Pulsar Parameter Drifts to Detect Sub-Nanohertz Gravitational Waves
• Sensitivity of new detection method for ultra-low frequency gravitational waves with pulsar spin-down rate statistics
• Shapiro Effect as a Possible Cause of the Low-Frequency Pulsar Timing Noise in Globular Clusters
• Noise reduction methods in analysis of near infrared lunar occultation light curves for high angular resolution measurements
• Stability of pulsar rotational and orbital periods