astrobase/periodbase/zgls.py
def analytic_false_alarm_probability(lspinfo,
                                     times,
                                     conservative_nfreq_eff=True,
                                     peakvals=None,
                                     inplace=True):

    '''This returns the analytic false alarm probabilities for periodogram
    peak values.

    The calculation follows that on page 3 of Zechmeister & Kurster (2009)::

        FAP = 1 − [1 − Prob(z > z0)]**M

    where::

        M is the number of independent frequencies
        Prob(z > z0) is the probability of peak with value > z0
        z0 is the peak value we're evaluating

    Parameters
    ----------

    lspinfo : dict
        The dict returned by the :py:func:`~astrobase.periodbase.zgls.pgen_lsp`
        function.

    times : np.array
        The times for which the periodogram result in ``lspinfo`` was
        calculated.

    conservative_nfreq_eff : bool
        If True, will follow the prescription given in Schwarzenberg-Czerny
        (2003):

        http://adsabs.harvard.edu/abs/2003ASPC..292..383S

        and estimate the effective number of independent frequences M_eff as::

            min(N_obs, N_freq, DELTA_f/delta_f)

    peakvals : sequence or None
        The peak values for which to evaluate the false-alarm probability. If
        None, will calculate this for each of the peak values in the
        ``nbestpeaks`` key of the ``lspinfo`` dict.

    inplace : bool
        If True, puts the results of the FAP calculation into the ``lspinfo``
        dict as a list available as ``lspinfo['falsealarmprob']``.

    Returns
    -------

    list
        The calculated false alarm probabilities for each of the peak values in
        ``peakvals``.

    '''

    frequencies = 1.0/lspinfo['periods']

    M = independent_freq_count(frequencies,
                               times,
                               conservative=conservative_nfreq_eff)

    if peakvals is None:
        peakvals = lspinfo['nbestlspvals']

    prob_exceed_vals = [
        probability_peak_exceeds_value(times, p) for p in peakvals
    ]

    false_alarm_probs = [
        1.0 - (1.0 - prob_exc)**M for prob_exc in prob_exceed_vals
    ]

    if inplace:
        lspinfo['falsealarmprob'] = false_alarm_probs

    return false_alarm_probs
def analytic_false_alarm_probability(lspinfo,
                                     times,
                                     conservative_nfreq_eff=True,
                                     peakvals=None,
                                     inplace=True):

    '''This returns the analytic false alarm probabilities for periodogram
    peak values.

    The calculation follows that on page 3 of Zechmeister & Kurster (2009)::

        FAP = 1 − [1 − Prob(z > z0)]**M

    where::

        M is the number of independent frequencies
        Prob(z > z0) is the probability of peak with value > z0
        z0 is the peak value we're evaluating

    Parameters
    ----------

    lspinfo : dict
        The dict returned by the :py:func:`~astrobase.periodbase.zgls.pgen_lsp`
        function.

    times : np.array
        The times for which the periodogram result in ``lspinfo`` was
        calculated.

    conservative_nfreq_eff : bool
        If True, will follow the prescription given in Schwarzenberg-Czerny
        (2003):

        http://adsabs.harvard.edu/abs/2003ASPC..292..383S

        and estimate the effective number of independent frequences M_eff as::

            min(N_obs, N_freq, DELTA_f/delta_f)

    peakvals : sequence or None
        The peak values for which to evaluate the false-alarm probability. If
        None, will calculate this for each of the peak values in the
        ``nbestpeaks`` key of the ``lspinfo`` dict.

    inplace : bool
        If True, puts the results of the FAP calculation into the ``lspinfo``
        dict as a list available as ``lspinfo['falsealarmprob']``.

    Returns
    -------

    list
        The calculated false alarm probabilities for each of the peak values in
        ``peakvals``.

    '''

    frequencies = 1.0/lspinfo['periods']

    M = independent_freq_count(frequencies,
                               times,
                               conservative=conservative_nfreq_eff)

    if peakvals is None:
        peakvals = lspinfo['nbestlspvals']

    prob_exceed_vals = [
        probability_peak_exceeds_value(times, p) for p in peakvals
    ]

    false_alarm_probs = [
        1.0 - (1.0 - prob_exc)**M for prob_exc in prob_exceed_vals
    ]

    if inplace:
        lspinfo['falsealarmprob'] = false_alarm_probs

    return false_alarm_probs
def analytic_false_alarm_probability ( lspinfo , times , conservative_nfreq_eff = True , peakvals = None , inplace = True ) : frequencies = 1.0 / lspinfo [ 'periods' ] M = independent_freq_count ( frequencies , times , conservative = conservative_nfreq_eff ) if peakvals is None : peakvals = lspinfo [ 'nbestlspvals' ] prob_exceed_vals = [ probability_peak_exceeds_value ( times , p ) for p in peakvals ] false_alarm_probs = [ 1.0 - ( 1.0 - prob_exc ) ** M for prob_exc in prob_exceed_vals ] if inplace : lspinfo [ 'falsealarmprob' ] = false_alarm_probs return false_alarm_probs
This returns the analytic false alarm probabilities for periodogram
    peak values.

    The calculation follows that on page 3 of Zechmeister & Kurster (2009)::

        FAP = 1 − [1 − Prob(z > z0)]**M

    where::

        M is the number of independent frequencies
        Prob(z > z0) is the probability of peak with value > z0
        z0 is the peak value we're evaluating

    Parameters
    ----------

    lspinfo : dict
        The dict returned by the :py:func:`~astrobase.periodbase.zgls.pgen_lsp`
        function.

    times : np.array
        The times for which the periodogram result in ``lspinfo`` was
        calculated.

    conservative_nfreq_eff : bool
        If True, will follow the prescription given in Schwarzenberg-Czerny
        (2003):

        http://adsabs.harvard.edu/abs/2003ASPC..292..383S

        and estimate the effective number of independent frequences M_eff as::

            min(N_obs, N_freq, DELTA_f/delta_f)

    peakvals : sequence or None
        The peak values for which to evaluate the false-alarm probability. If
        None, will calculate this for each of the peak values in the
        ``nbestpeaks`` key of the ``lspinfo`` dict.

    inplace : bool
        If True, puts the results of the FAP calculation into the ``lspinfo``
        dict as a list available as ``lspinfo['falsealarmprob']``.

    Returns
    -------

    list
        The calculated false alarm probabilities for each of the peak values in
        ``peakvals``.
This returns the analytic false alarm probabilities for periodogram peak values .