LombScargle¶

class
astropy.timeseries.
LombScargle
(t, y, dy=None, fit_mean=True, center_data=True, nterms=1, normalization='standard')[source]¶ Bases:
astropy.timeseries.BasePeriodogram
Compute the LombScargle Periodogram.
This implementations here are based on code presented in [R14388b5a5a571] and [R14388b5a5a572]; if you use this functionality in an academic application, citation of those works would be appreciated.
 Parameters
 tarray_like or Quantity
sequence of observation times
 yarray_like or Quantity
sequence of observations associated with times t
 dyfloat, array_like or Quantity (optional)
error or sequence of observational errors associated with times t
 fit_meanbool (optional, default=True)
if True, include a constant offset as part of the model at each frequency. This can lead to more accurate results, especially in the case of incomplete phase coverage.
 center_databool (optional, default=True)
if True, precenter the data by subtracting the weighted mean of the input data. This is especially important if fit_mean = False
 ntermsint (optional, default=1)
number of terms to use in the Fourier fit
 normalization{‘standard’, ‘model’, ‘log’, ‘psd’}, optional
Normalization to use for the periodogram.
References
 R14388b5a5a571
Vanderplas, J., Connolly, A. Ivezic, Z. & Gray, A. Introduction to astroML: Machine learning for astrophysics. Proceedings of the Conference on Intelligent Data Understanding (2012)
 R14388b5a5a572
VanderPlas, J. & Ivezic, Z. Periodograms for Multiband Astronomical Time Series. ApJ 812.1:18 (2015)
Examples
Generate noisy periodic data:
>>> rand = np.random.RandomState(42) >>> t = 100 * rand.rand(100) >>> y = np.sin(2 * np.pi * t) + rand.randn(100)
Compute the LombScargle periodogram on an automaticallydetermined frequency grid & find the frequency of max power:
>>> frequency, power = LombScargle(t, y).autopower() >>> frequency[np.argmax(power)] # doctest: +FLOAT_CMP 1.0016662310392956
Compute the LombScargle periodogram at a userspecified frequency grid:
>>> freq = np.arange(0.8, 1.3, 0.1) >>> LombScargle(t, y).power(freq) # doctest: +FLOAT_CMP array([0.0204304 , 0.01393845, 0.35552682, 0.01358029, 0.03083737])
If the inputs are astropy Quantities with units, the units will be validated and the outputs will also be Quantities with appropriate units:
>>> from astropy import units as u >>> t = t * u.s >>> y = y * u.mag >>> frequency, power = LombScargle(t, y).autopower() >>> frequency.unit Unit("1 / s") >>> power.unit Unit(dimensionless)
Note here that the LombScargle power is always a unitless quantity, because it is related to the \(\chi^2\) of the bestfit periodic model at each frequency.
Attributes Summary
Methods Summary
autofrequency
(self[, samples_per_peak, …])Determine a suitable frequency grid for data.
autopower
(self[, method, method_kwds, …])Compute LombScargle power at automaticallydetermined frequencies.
design_matrix
(self, frequency[, t])Compute the design matrix for a given frequency
distribution
(self, power[, cumulative])Expected periodogram distribution under the null hypothesis.
false_alarm_level
(self, false_alarm_probability)Level of maximum at a given false alarm probability.
false_alarm_probability
(self, power[, …])False alarm probability of periodogram maxima under the null hypothesis.
from_timeseries
(timeseries[, …])Initialize a periodogram from a time series object.
model
(self, t, frequency)Compute the LombScargle model at the given frequency.
model_parameters
(self, frequency[, units])Compute the bestfit model parameters at the given frequency.
offset
(self)Return the offset of the model
power
(self, frequency[, normalization, …])Compute the LombScargle power at the given frequencies.
Attributes Documentation

available_methods
= ['auto', 'slow', 'chi2', 'cython', 'fast', 'fastchi2', 'scipy']¶
Methods Documentation

autofrequency
(self, samples_per_peak=5, nyquist_factor=5, minimum_frequency=None, maximum_frequency=None, return_freq_limits=False)[source]¶ Determine a suitable frequency grid for data.
Note that this assumes the peak width is driven by the observational baseline, which is generally a good assumption when the baseline is much larger than the oscillation period. If you are searching for periods longer than the baseline of your observations, this may not perform well.
Even with a large baseline, be aware that the maximum frequency returned is based on the concept of “average Nyquist frequency”, which may not be useful for irregularlysampled data. The maximum frequency can be adjusted via the nyquist_factor argument, or through the maximum_frequency argument.
 Parameters
 samples_per_peakfloat (optional, default=5)
The approximate number of desired samples across the typical peak
 nyquist_factorfloat (optional, default=5)
The multiple of the average nyquist frequency used to choose the maximum frequency if maximum_frequency is not provided.
 minimum_frequencyfloat (optional)
If specified, then use this minimum frequency rather than one chosen based on the size of the baseline.
 maximum_frequencyfloat (optional)
If specified, then use this maximum frequency rather than one chosen based on the average nyquist frequency.
 return_freq_limitsbool (optional)
if True, return only the frequency limits rather than the full frequency grid.
 Returns
 frequencyndarray or Quantity
The heuristicallydetermined optimal frequency bin

autopower
(self, method='auto', method_kwds=None, normalization=None, samples_per_peak=5, nyquist_factor=5, minimum_frequency=None, maximum_frequency=None)[source]¶ Compute LombScargle power at automaticallydetermined frequencies.
 Parameters
 methodstring (optional)
specify the lomb scargle implementation to use. Options are:
‘auto’: choose the best method based on the input
‘fast’: use the O[N log N] fast method. Note that this requires evenlyspaced frequencies: by default this will be checked unless
assume_regular_frequency
is set to True.‘slow’: use the O[N^2] purepython implementation
‘cython’: use the O[N^2] cython implementation. This is slightly faster than method=’slow’, but much more memory efficient.
‘chi2’: use the O[N^2] chi2/linearfitting implementation
‘fastchi2’: use the O[N log N] chi2 implementation. Note that this requires evenlyspaced frequencies: by default this will be checked unless
assume_regular_frequency
is set to True.‘scipy’: use
scipy.signal.lombscargle
, which is an O[N^2] implementation written in C. Note that this does not support heteroskedastic errors.
 method_kwdsdict (optional)
additional keywords to pass to the lombscargle method
 normalization{‘standard’, ‘model’, ‘log’, ‘psd’}, optional
If specified, override the normalization specified at instantiation.
 samples_per_peakfloat (optional, default=5)
The approximate number of desired samples across the typical peak
 nyquist_factorfloat (optional, default=5)
The multiple of the average nyquist frequency used to choose the maximum frequency if maximum_frequency is not provided.
 minimum_frequencyfloat (optional)
If specified, then use this minimum frequency rather than one chosen based on the size of the baseline.
 maximum_frequencyfloat (optional)
If specified, then use this maximum frequency rather than one chosen based on the average nyquist frequency.
 Returns
 frequency, powerndarrays
The frequency and LombScargle power

design_matrix
(self, frequency, t=None)[source]¶ Compute the design matrix for a given frequency
 Parameters
 Returns
 Xnp.ndarray (len(t), n_parameters)
The design matrix for the model at the given frequency.
See also

distribution
(self, power, cumulative=False)[source]¶ Expected periodogram distribution under the null hypothesis.
This computes the expected probability distribution or cumulative probability distribution of periodogram power, under the null hypothesis of a nonvarying signal with Gaussian noise. Note that this is not the same as the expected distribution of peak values; for that see the
false_alarm_probability()
method. Parameters
 powerarray_like
The periodogram power at which to compute the distribution.
 cumulativebool (optional)
If True, then return the cumulative distribution.
 Returns
 distnp.ndarray
The probability density or cumulative probability associated with the provided powers.
See also

false_alarm_level
(self, false_alarm_probability, method='baluev', samples_per_peak=5, nyquist_factor=5, minimum_frequency=None, maximum_frequency=None, method_kwds=None)[source]¶ Level of maximum at a given false alarm probability.
This gives an estimate of the periodogram level corresponding to a specified false alarm probability for the largest peak, assuming a null hypothesis of nonvarying data with Gaussian noise.
 Parameters
 false_alarm_probabilityarraylike
The false alarm probability (0 < fap < 1).
 maximum_frequencyfloat
The maximum frequency of the periodogram.
 method{‘baluev’, ‘davies’, ‘naive’, ‘bootstrap’}, optional
The approximation method to use; default=’baluev’.
 method_kwdsdict, optional
Additional methodspecific keywords.
 Returns
 powernp.ndarray
The periodogram peak height corresponding to the specified false alarm probability.
See also
Notes
The true probability distribution for the largest peak cannot be determined analytically, so each method here provides an approximation to the value. The available methods are:
“baluev” (default): the upperlimit to the aliasfree probability, using the approach of Baluev (2008) [1].
“davies” : the Davies upper bound from Baluev (2008) [1].
“naive” : the approximate probability based on an estimated effective number of independent frequencies.
“bootstrap” : the approximate probability based on bootstrap resamplings of the input data.
Note also that for normalization=’psd’, the distribution can only be computed for periodograms constructed with errors specified.
References

false_alarm_probability
(self, power, method='baluev', samples_per_peak=5, nyquist_factor=5, minimum_frequency=None, maximum_frequency=None, method_kwds=None)[source]¶ False alarm probability of periodogram maxima under the null hypothesis.
This gives an estimate of the false alarm probability given the height of the largest peak in the periodogram, based on the null hypothesis of nonvarying data with Gaussian noise.
 Parameters
 powerarraylike
The periodogram value.
 method{‘baluev’, ‘davies’, ‘naive’, ‘bootstrap’}, optional
The approximation method to use.
 maximum_frequencyfloat
The maximum frequency of the periodogram.
 method_kwdsdict (optional)
Additional methodspecific keywords.
 Returns
 false_alarm_probabilitynp.ndarray
The false alarm probability
See also
Notes
The true probability distribution for the largest peak cannot be determined analytically, so each method here provides an approximation to the value. The available methods are:
“baluev” (default): the upperlimit to the aliasfree probability, using the approach of Baluev (2008) [1].
“davies” : the Davies upper bound from Baluev (2008) [1].
“naive” : the approximate probability based on an estimated effective number of independent frequencies.
“bootstrap” : the approximate probability based on bootstrap resamplings of the input data.
Note also that for normalization=’psd’, the distribution can only be computed for periodograms constructed with errors specified.
References

classmethod
from_timeseries
(timeseries, signal_column_name=None, uncertainty=None, **kwargs)¶ Initialize a periodogram from a time series object.
If a binned time series is passed, the time at the center of the bins is used. Also note that this method automatically gets rid of NaN/undefined values when initalizing the periodogram.
 Parameters
 signal_column_namestr
The name of the column containing the signal values to use.
 uncertaintystr or float or
Quantity
, optional The name of the column containing the errors on the signal, or the value to use for the error, if a scalar.
 **kwargs
Additional keyword arguments are passed to the initializer for this periodogram class.

model
(self, t, frequency)[source]¶ Compute the LombScargle model at the given frequency.
The model at a particular frequency is a linear model: model = offset + dot(design_matrix, model_parameters)
 Parameters
 tarray_like or Quantity, length n_samples
times at which to compute the model
 frequencyfloat
the frequency for the model
 Returns
 ynp.ndarray, length n_samples
The model fit corresponding to the input times
See also

model_parameters
(self, frequency, units=True)[source]¶ Compute the bestfit model parameters at the given frequency.
The model described by these parameters is:
\[y(t; f, \vec{\theta}) = \theta_0 + \sum_{n=1}^{\tt nterms} [\theta_{2n1}\sin(2\pi n f t) + \theta_{2n}\cos(2\pi n f t)]\]where \(\vec{\theta}\) is the array of parameters returned by this function.
 Parameters
 frequencyfloat
the frequency for the model
 unitsbool
If True (default), return design matrix with data units.
 Returns
 thetanp.ndarray (n_parameters,)
The bestfit model parameters at the given frequency.
See also

offset
(self)[source]¶ Return the offset of the model
The offset of the model is the (weighted) mean of the y values. Note that if self.center_data is False, the offset is 0 by definition.
 Returns
 offsetscalar
See also

power
(self, frequency, normalization=None, method='auto', assume_regular_frequency=False, method_kwds=None)[source]¶ Compute the LombScargle power at the given frequencies.
 Parameters
 frequencyarray_like or Quantity
frequencies (not angular frequencies) at which to evaluate the periodogram. Note that in order to use method=’fast’, frequencies must be regularlyspaced.
 methodstring (optional)
specify the lomb scargle implementation to use. Options are:
‘auto’: choose the best method based on the input
‘fast’: use the O[N log N] fast method. Note that this requires evenlyspaced frequencies: by default this will be checked unless
assume_regular_frequency
is set to True.‘slow’: use the O[N^2] purepython implementation
‘cython’: use the O[N^2] cython implementation. This is slightly faster than method=’slow’, but much more memory efficient.
‘chi2’: use the O[N^2] chi2/linearfitting implementation
‘fastchi2’: use the O[N log N] chi2 implementation. Note that this requires evenlyspaced frequencies: by default this will be checked unless
assume_regular_frequency
is set to True.‘scipy’: use
scipy.signal.lombscargle
, which is an O[N^2] implementation written in C. Note that this does not support heteroskedastic errors.
 assume_regular_frequencybool (optional)
if True, assume that the input frequency is of the form freq = f0 + df * np.arange(N). Only referenced if method is ‘auto’ or ‘fast’.
 normalization{‘standard’, ‘model’, ‘log’, ‘psd’}, optional
If specified, override the normalization specified at instantiation.
 fit_meanbool (optional, default=True)
If True, include a constant offset as part of the model at each frequency. This can lead to more accurate results, especially in the case of incomplete phase coverage.
 center_databool (optional, default=True)
If True, precenter the data by subtracting the weighted mean of the input data. This is especially important if fit_mean = False.
 method_kwdsdict (optional)
additional keywords to pass to the lombscargle method
 Returns
 powerndarray
The LombScargle power at the specified frequency