Wavelet analysis for rotation period extraction#
This notebook provide an example of analysis replacing the Lomb-Scargle periodogram by a wavelet analysis of the time series. The wavelet analysis is not a part of the PLATO MSAP4 rotation & activity baseline algorithms but it represents an interesting alternative in order to assess the performances of the framework.
import star_privateer as sp
A simple example#
import importlib
import tqdm
import os
import numpy as np
import matplotlib.pyplot as plt
if not os.path.exists ('stellar_analysis_features') :
os.mkdir ('stellar_analysis_features')
if not os.path.exists ('stellar_analysis_plots') :
os.mkdir ('stellar_analysis_plots')
Our working case is KIC 3733735.
filename = sp.get_target_filename (sp.timeseries, '003733735')
t, s, dt = sp.load_resource (filename)
In order to save computing time, we rebin the data in 4-hour bins.
dt *= 4
t = np.mean (t.reshape (-1,4), axis=1)
s = np.mean (s.reshape (-1,4), axis=1)
We now run the analysis pipeline. In particular, we can take a look at the plots made from the different analysis methods.
(p_acf, gwps, wps, acf,
cs, coi, features, feature_names, _) = sp.analysis_pipeline (t, s, figsize=(8,12),
wavelet_analysis=True, plot=True,
xlim=(0,50), normscale='log', ylogscale=True,
add_periodogram=True)
It is also possible to compute the wavelet power spectrum and plot it independently from the other methods.
dt = (t[1]-t[0])*86400
(periods, wps, gwps,
coi, scales) = sp.compute_wps(s, dt, normalise=True, mother=None)
fig = sp.plot_wps(t-t[0], periods, wps, gwps, coi,
scales, shading='auto', color_coi='darkgrey',
ylogscale=True, lw=1, normscale='log',
vmin=None, vmax=None, filename=None, dpi=300,
figsize=(8,4), ylim=(1, 100), show_contour=False)