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Calibration::StandardData Class Reference Computes the normalized Stokes parameters in each phase bin. More...
Inheritance diagram for Calibration::StandardData:
Detailed DescriptionComputes the normalized Stokes parameters in each phase bin. The apparent pulsar flux varies with time, and it is necessary to normalize the observed Stokes parameters when modelling. Because the total intensity is distorted by polarimetric tranformations, it is necessary to estimate the apparent gain variations using the polarimetic invariant interval. Before this class was written, the NormalizeStokes class was used to normalize each set of Stokes parameters by their invariant. However, when the signal-to-noise ratio is low, the invariant can be less than or equal to zero and as a result many points had to be discarded. This problem is overcome by normalizing each set of Stokes parameters by the mean of the invariant interval over all on-pulse phase bins. This approach has the following benefits: 1) even when the Stokes parameters in a single phase bin are highly polarized, the other less polarized on-pulse phase bins will produce a mean invariant greater than zero 2) the mean invariant interval has sqrt(onpulse_nbin) greater S/N 3) the mean invariant is chi distributed with onpulse_nbin * 4 degrees of freedom (much more like normally distributed than 4 d.o.f) Constructor & Destructor Documentation◆ StandardData()
Default constructor. If specified, baseline and on-pulse regions are defined by select The documentation for this class was generated from the following files:
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