Readout along the maximal power component (ridge) in a wavelet spectrum in continuous wavelet transform (CWT) analysis.CWT performed on detrended and amplitude-unnormalized signals.
The paucity of known intermittent pulsars makes individual studies valuable from the perspective of understanding how these pulsars emit and how that emission is changing in time and as a function of
This data set contains the power spectral density of magnetic field fluctuations computed by onboard FFTs by the Digital Signal Processor (DSP) from from MMS-3 SCM waveforms during fast survey modes b
Pulsars with features in their radio spectra, such as curvature or breaks seem to be special cases among the known pulsar population, with only about 20 per cent exhibiting them. Unfortunately, reliab
