pint.models.noise_model
Pulsar timing noise models.
Functions
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Create quantization matrix mapping TOAs to observing epochs. |
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Construct fourier design matrix from eq 11 of Lentati et al, 2013 |
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Find only epochs with more than 1 TOA for applying ECORR. |
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Get the number of epochs associated with each ECORR. |
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Frequency components for creating the red noise basis matrix. |
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Power-law PSD. |
Classes
Noise correlated between nearby TOAs. |
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Model of DM variations as radio frequency-dependent noise with a power-law spectrum. |
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Timing noise with a power-law spectrum. |
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Correction for estimated wideband DM measurement uncertainty. |
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Correct reported template fitting uncertainties. |