< Pulsars and neutron stars
Introduction
Pulse numbering
Glitch events
In tempo/tempo2, glitch events are modelled as an offset in pulse phase, and the permanent increments in the pulse frequency and first frequency time derivative . In addition it is sometimes necessary to in a transient frequency increment which decays exponentially to zero with a timescale of . The phase model (caused by the glitch) is therefore taken as:
where is the glitch epoch and is the current time.
Frequency-dependent and frequency-independent noise
Spatially correlated timing residuals
Spectral analysis of timing residuals
Interpolation and extrapolation of pulsar timing residuals
This article is issued from Wikibooks. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.