Source code for gammapy.stats.fit_statistics

# Licensed under a 3-clause BSD style license - see LICENSE.rst
"""Common fit statistics used in gamma-ray astronomy.

see :ref:`fit-statistics`
"""

from __future__ import absolute_import, division, print_function, unicode_literals
import numpy as np

__all__ = [
    'cash', 'cstat', 'wstat', 'get_wstat_mu_bkg', 'get_wstat_gof_terms',
    'lstat', 'pgstat',
    'chi2', 'chi2constvar', 'chi2datavar',
    'chi2gehrels', 'chi2modvar', 'chi2xspecvar',
]

N_ON_MIN = 1e-25


[docs]def cash(n_on, mu_on): r"""Cash statistic, for Poisson data. The Cash statistic is defined as: .. math:: C = 2 \left( n_{on} - n_{on} \log \mu_{on} \right) and :math:`C = 0` where :math:`\mu <= 0`. For more information see :ref:`fit-statistics` Parameters ---------- n_on : array_like Observed counts mu_on : array_like Expected counts Returns ------- stat : ndarray Statistic per bin References ---------- * `Sherpa statistics page section on the Cash statistic <http://cxc.cfa.harvard.edu/sherpa/statistics/#cash>`_ * `Sherpa help page on the Cash statistic <http://cxc.harvard.edu/sherpa/ahelp/cash.html>`_ * `Cash 1979, ApJ 228, 939 <http://adsabs.harvard.edu/abs/1979ApJ...228..939C>`_ """ n_on = np.asanyarray(n_on, dtype=np.float64) mu_on = np.asanyarray(mu_on, dtype=np.float64) stat = 2 * (mu_on - n_on * np.log(mu_on)) stat = np.where(mu_on > 0, stat, 0) return stat
[docs]def cstat(n_on, mu_on, n_on_min=N_ON_MIN): r"""C statistic, for Poisson data. The C statistic is defined as .. math:: C = 2 \left[ \mu_{on} - n_{on} + n_{on} (\log(n_{on}) - log(\mu_{on}) \right] and :math:`C = 0` where :math:`\mu_{on} <= 0`. ``n_on_min`` handles the case where ``n_on`` is 0 or less and the log cannot be taken. For more information see :ref:`fit-statistics` Parameters ---------- n_on : array_like Observed counts mu_on : array_like Expected counts n_on_min : array_like ``n_on`` = ``n_on_min`` where ``n_on`` <= ``n_on_min.`` Returns ------- stat : ndarray Statistic per bin References ---------- * `Sherpa stats page section on the C statistic <http://cxc.cfa.harvard.edu/sherpa/statistics/#cstat>`_ * `Sherpa help page on the C statistic <http://cxc.harvard.edu/sherpa/ahelp/cash.html>`_ * `Cash 1979, ApJ 228, 939 <http://adsabs.harvard.edu/abs/1979ApJ...228..939C>`_ """ n_on = np.asanyarray(n_on, dtype=np.float64) mu_on = np.asanyarray(mu_on, dtype=np.float64) n_on_min = np.asanyarray(n_on_min, dtype=np.float64) n_on = np.where(n_on <= n_on_min, n_on_min, n_on) term1 = np.log(n_on) - np.log(mu_on) stat = 2 * (mu_on - n_on + n_on * term1) stat = np.where(mu_on > 0, stat, 0) return stat
[docs]def wstat(n_on, n_off, alpha, mu_sig, mu_bkg=None, extra_terms=True): r"""W statistic, for Poisson data with Poisson background. For a definition of WStat see :ref:`wstat`. If ``mu_bkg`` is not provided it will be calculated according to the profile likelihood formula. Parameters ---------- n_on : array_like Total observed counts n_off : array_like Total observed background counts alpha : array_like Exposure ratio between on and off region mu_sig : array_like Signal expected counts mu_bkg : array_like, optional Background expected counts extra_terms : bool, optional Add model independent terms to convert stat into goodness-of-fit parameter, default: True Returns ------- stat : ndarray Statistic per bin References ---------- * `Habilitation M. de Naurois, p. 141 <http://inspirehep.net/record/1122589/files/these_short.pdf>`_ * `XSPEC page on Poisson data with Poisson background <http://heasarc.nasa.gov/xanadu/xspec/manual/XSappendixStatistics.html>`_ """ # Note: This is equivalent to what's defined on the XSPEC page under the # following assumptions # t_s * m_i = mu_sig # t_b * m_b = mu_bkg # t_s / t_b = alpha n_on = np.atleast_1d(np.asanyarray(n_on, dtype=np.float64)) n_off = np.atleast_1d(np.asanyarray(n_off, dtype=np.float64)) alpha = np.atleast_1d(np.asanyarray(alpha, dtype=np.float64)) mu_sig = np.atleast_1d(np.asanyarray(mu_sig, dtype=np.float64)) if mu_bkg is None: mu_bkg = get_wstat_mu_bkg(n_on, n_off, alpha, mu_sig) term1 = mu_sig + (1 + alpha) * mu_bkg term2_ = - n_on * np.log(mu_sig + alpha * mu_bkg) # Handle n_on == 0 condition = (n_on == 0) term2 = np.where(condition, 0, term2_) term3_ = - n_off * np.log(mu_bkg) # Handle n_off == 0 condition = (n_off == 0) term3 = np.where(condition, 0, term3_) stat = 2 * (term1 + term2 + term3) if extra_terms: stat += get_wstat_gof_terms(n_on, n_off) return stat
[docs]def get_wstat_mu_bkg(n_on, n_off, alpha, mu_sig): """Calculate ``mu_bkg`` for wstat see :ref:`wstat`. """ # NOTE: Corner cases in the docs are all handled correcty by this formula C = alpha * (n_on + n_off) - (1 + alpha) * mu_sig D = np.sqrt(C ** 2 + 4 * alpha * (alpha + 1) * n_off * mu_sig) mu_bkg = (C + D) / (2 * alpha * (alpha + 1)) return mu_bkg
[docs]def get_wstat_gof_terms(n_on, n_off): """Calculate goodness of fit terms for wstat see :ref:`wstat`. """ term = np.zeros(len(n_on)) term1 = - n_on * (1 - np.log(n_on)) term2 = - n_off * (1 - np.log(n_off)) term += np.where(n_on == 0, 0, term1) term += np.where(n_off == 0, 0, term2) return 2 * term
[docs]def lstat(): r"""L statistic, for Poisson data with Poisson background (Bayesian). Reference: http://heasarc.nasa.gov/xanadu/xspec/manual/XSappendixStatistics.html """ pass
[docs]def pgstat(): r"""PG statistic, for Poisson data with Gaussian background. Reference: http://heasarc.nasa.gov/xanadu/xspec/manual/XSappendixStatistics.html """ pass
[docs]def chi2(N_S, B, S, sigma2): r"""Chi-square statistic with user-specified variance. .. math:: \chi^2 = \frac{(N_S - B - S) ^ 2}{\sigma ^ 2} Parameters ---------- N_S : array_like Number of observed counts B : array_like Model background S : array_like Model signal sigma2 : array_like Variance Returns ------- stat : ndarray Statistic per bin References ---------- * Sherpa stats page (http://cxc.cfa.harvard.edu/sherpa/statistics/#chisq) """ N_S = np.asanyarray(N_S, dtype=np.float64) B = np.asanyarray(B, dtype=np.float64) S = np.asanyarray(S, dtype=np.float64) sigma2 = np.asanyarray(sigma2, dtype=np.float64) stat = (N_S - B - S) ** 2 / sigma2 return stat
[docs]def chi2constvar(N_S, N_B, A_S, A_B): r"""Chi-square statistic with constant variance. """ N_S = np.asanyarray(N_S, dtype=np.float64) N_B = np.asanyarray(N_B, dtype=np.float64) A_S = np.asanyarray(A_S, dtype=np.float64) A_B = np.asanyarray(A_B, dtype=np.float64) alpha2 = (A_S / A_B) ** 2 # Need to mulitply with np.ones_like(N_S) here? sigma2 = (N_S + alpha2 * N_B).mean() stat = chi2(N_S, A_B, A_S, sigma2) return stat
[docs]def chi2datavar(N_S, N_B, A_S, A_B): r"""Chi-square statistic with data variance. """ N_S = np.asanyarray(N_S, dtype=np.float64) N_B = np.asanyarray(N_B, dtype=np.float64) A_S = np.asanyarray(A_S, dtype=np.float64) A_B = np.asanyarray(A_B, dtype=np.float64) alpha2 = (A_S / A_B) ** 2 sigma2 = N_S + alpha2 * N_B stat = chi2(N_S, A_B, A_S, sigma2) return stat
[docs]def chi2gehrels(N_S, N_B, A_S, A_B): r"""Chi-square statistic with Gehrel's variance. """ N_S = np.asanyarray(N_S, dtype=np.float64) N_B = np.asanyarray(N_B, dtype=np.float64) A_S = np.asanyarray(A_S, dtype=np.float64) A_B = np.asanyarray(A_B, dtype=np.float64) alpha2 = (A_S / A_B) ** 2 sigma_S = 1 + np.sqrt(N_S + 0.75) sigma_B = 1 + np.sqrt(N_B + 0.75) sigma2 = sigma_S ** 2 + alpha2 * sigma_B ** 2 stat = chi2(N_S, A_B, A_S, sigma2) return stat
[docs]def chi2modvar(S, B, A_S, A_B): r"""Chi-square statistic with model variance. """ S = np.asanyarray(S, dtype=np.float64) B = np.asanyarray(B, dtype=np.float64) A_S = np.asanyarray(A_S, dtype=np.float64) A_B = np.asanyarray(A_B, dtype=np.float64) stat = chi2datavar(S, B, A_S, A_B) return stat
[docs]def chi2xspecvar(N_S, N_B, A_S, A_B): r"""Chi-square statistic with XSPEC variance. """ N_S = np.asanyarray(N_S, dtype=np.float64) N_B = np.asanyarray(N_B, dtype=np.float64) A_S = np.asanyarray(A_S, dtype=np.float64) A_B = np.asanyarray(A_B, dtype=np.float64) # TODO: is this correct? mask = (N_S < 1) | (N_B < 1) # _stat = np.empty_like(mask, dtype='float') # _stat[mask] = 1 stat = np.where(mask, 1, chi2datavar(N_S, N_B, A_S, A_B)) return stat