a a@snddlmZddlZddlZddlmZddlZddlmZm Z m Z m Z m Z m Z mZmZmZmZmZmZmZmZmZmZmZmZmZmZmZmZmZddlm Z ddlm!Z!ddl"m#Z#dd l"m$Z$dd l$m%Z%m&Z&m'Z'dd l(m)Z)dd l"m*Z*dd l+m,Z,ddl-m.Z.gdZ/eddZ0eddZ1eddZ2dddZ3ddZ4dddZ5dddZ6ddZ7dd!d"Z8d#d$Z9dd(d)Z:dd,d-Z;dd/d0Zdd5d6Z?dd8d9Z@dd:d;ZAddd?ZCd@dAZDdBdCZEddEdFZFddGdHZGedIdJZHdKdLZIegdMZJegdNZKegdOZLegdPZMedQdRZNddSdTZOdUdVZPdWdXZQedYdRZRddZd[ZSed\dJZTGd]d^d^ZUeUZVdd`daZWedbdJZXdcddZYededJZZdfdgdhdidjZ[ddldmZ\dndoZ]edpdJZ^dfdgdhdqdrZ_ddsdtZ`edudJZaddxdyZbdzd dd{d|d}d~ZcdddZddeddd{fddZededdd{fddZfdeddd{fddZgdS)) annotationsN) namedtuple)isscalarr_logarounduniqueasarrayzerosarangesortaminamax atleast_1dsqrtarraycompresspiexpravel count_nonzerosincosarctan2hypot)optimize)special)statlib)stats) find_repeats _contains_nan_normtest_finish)chi2_contingency) distributions) rv_generic)_get_wilcoxon_distr)mvsdist bayes_mvskstatkstatvarprobplotppcc_max ppcc_plot boxcox_llfboxcoxboxcox_normmaxboxcox_normplotshapiroandersonansaribartlettlevene binom_testflignermoodwilcoxon median_testcircmeancircvarcircstdanderson_ksampyeojohnson_llf yeojohnsonyeojohnson_normmaxyeojohnson_normplotMean) statisticZminmaxVarianceStd_dev?cCspt|\}}}|dks|dkr*td|t|||}t|||}t|||}|||fS)a- Bayesian confidence intervals for the mean, var, and std. Parameters ---------- data : array_like Input data, if multi-dimensional it is flattened to 1-D by `bayes_mvs`. Requires 2 or more data points. alpha : float, optional Probability that the returned confidence interval contains the true parameter. Returns ------- mean_cntr, var_cntr, std_cntr : tuple The three results are for the mean, variance and standard deviation, respectively. Each result is a tuple of the form:: (center, (lower, upper)) with `center` the mean of the conditional pdf of the value given the data, and `(lower, upper)` a confidence interval, centered on the median, containing the estimate to a probability ``alpha``. See Also -------- mvsdist Notes ----- Each tuple of mean, variance, and standard deviation estimates represent the (center, (lower, upper)) with center the mean of the conditional pdf of the value given the data and (lower, upper) is a confidence interval centered on the median, containing the estimate to a probability ``alpha``. Converts data to 1-D and assumes all data has the same mean and variance. Uses Jeffrey's prior for variance and std. Equivalent to ``tuple((x.mean(), x.interval(alpha)) for x in mvsdist(dat))`` References ---------- T.E. Oliphant, "A Bayesian perspective on estimating mean, variance, and standard-deviation from data", https://scholarsarchive.byu.edu/facpub/278, 2006. Examples -------- First a basic example to demonstrate the outputs: >>> from scipy import stats >>> data = [6, 9, 12, 7, 8, 8, 13] >>> mean, var, std = stats.bayes_mvs(data) >>> mean Mean(statistic=9.0, minmax=(7.103650222612533, 10.896349777387467)) >>> var Variance(statistic=10.0, minmax=(3.176724206..., 24.45910382...)) >>> std Std_dev(statistic=2.9724954732045084, minmax=(1.7823367265645143, 4.945614605014631)) Now we generate some normally distributed random data, and get estimates of mean and standard deviation with 95% confidence intervals for those estimates: >>> n_samples = 100000 >>> data = stats.norm.rvs(size=n_samples) >>> res_mean, res_var, res_std = stats.bayes_mvs(data, alpha=0.95) >>> import matplotlib.pyplot as plt >>> fig = plt.figure() >>> ax = fig.add_subplot(111) >>> ax.hist(data, bins=100, density=True, label='Histogram of data') >>> ax.vlines(res_mean.statistic, 0, 0.5, colors='r', label='Estimated mean') >>> ax.axvspan(res_mean.minmax[0],res_mean.minmax[1], facecolor='r', ... alpha=0.2, label=r'Estimated mean (95% limits)') >>> ax.vlines(res_std.statistic, 0, 0.5, colors='g', label='Estimated scale') >>> ax.axvspan(res_std.minmax[0],res_std.minmax[1], facecolor='g', alpha=0.2, ... label=r'Estimated scale (95% limits)') >>> ax.legend(fontsize=10) >>> ax.set_xlim([-4, 4]) >>> ax.set_ylim([0, 0.5]) >>> plt.show() rrz20 < alpha < 1 is required, but alpha=%s was given.)r' ValueErrorrDmeanintervalrFrG)dataalphamvsZm_resZv_resZs_resrQe/Users/vegardjervell/Documents/master/model/venv/lib/python3.9/site-packages/scipy/stats/morestats.pyr('sWr(c Cst|}t|}|dkr td|}|}|dkrtj|t||d}tjt|t|d|d}tj|td||d}nZ|d}||d} |d} tj ||t||d}tj | dt| d}tj | | d}|||fS) a 'Frozen' distributions for mean, variance, and standard deviation of data. Parameters ---------- data : array_like Input array. Converted to 1-D using ravel. Requires 2 or more data-points. Returns ------- mdist : "frozen" distribution object Distribution object representing the mean of the data. vdist : "frozen" distribution object Distribution object representing the variance of the data. sdist : "frozen" distribution object Distribution object representing the standard deviation of the data. See Also -------- bayes_mvs Notes ----- The return values from ``bayes_mvs(data)`` is equivalent to ``tuple((x.mean(), x.interval(0.90)) for x in mvsdist(data))``. In other words, calling ``.mean()`` and ``.interval(0.90)`` on the three distribution objects returned from this function will give the same results that are returned from `bayes_mvs`. References ---------- T.E. Oliphant, "A Bayesian perspective on estimating mean, variance, and standard-deviation from data", https://scholarsarchive.byu.edu/facpub/278, 2006. Examples -------- >>> from scipy import stats >>> data = [6, 9, 12, 7, 8, 8, 13] >>> mean, var, std = stats.mvsdist(data) We now have frozen distribution objects "mean", "var" and "std" that we can examine: >>> mean.mean() 9.0 >>> mean.interval(0.95) (6.6120585482655692, 11.387941451734431) >>> mean.std() 1.1952286093343936 zNeed at least 2 data-points.i)locscale@r)rU) rlenrIrJvarr$normmathrtZgengammaZinvgamma) rLxnxbarCZmdistsdistZvdistZnm1facvalrQrQrRr's"7" r'rScCs|dks|dkrtdt|}t|dtj}t|}|j}|dkrPtdtt|rftj St d|dD]}tj||dd||<qt|dkr|dd|S|dkr||d|dd ||dS|d kr*d|dd d ||d|d|||d ||d|d S|dkrd |ddd ||dd|dd ||d|ddd||d|d|d |||d|d||d|d |d StddS)a5 Return the nth k-statistic (1<=n<=4 so far). The nth k-statistic k_n is the unique symmetric unbiased estimator of the nth cumulant kappa_n. Parameters ---------- data : array_like Input array. Note that n-D input gets flattened. n : int, {1, 2, 3, 4}, optional Default is equal to 2. Returns ------- kstat : float The nth k-statistic. See Also -------- kstatvar: Returns an unbiased estimator of the variance of the k-statistic. moment: Returns the n-th central moment about the mean for a sample. Notes ----- For a sample size n, the first few k-statistics are given by: .. math:: k_{1} = \mu k_{2} = \frac{n}{n-1} m_{2} k_{3} = \frac{ n^{2} } {(n-1) (n-2)} m_{3} k_{4} = \frac{ n^{2} [(n + 1)m_{4} - 3(n - 1) m^2_{2}]} {(n-1) (n-2) (n-3)} where :math:`\mu` is the sample mean, :math:`m_2` is the sample variance, and :math:`m_i` is the i-th sample central moment. References ---------- http://mathworld.wolfram.com/k-Statistic.html http://mathworld.wolfram.com/Cumulant.html Examples -------- >>> from scipy import stats >>> from numpy.random import default_rng >>> rng = default_rng() As sample size increases, n-th moment and n-th k-statistic converge to the same number (although they aren't identical). In the case of the normal distribution, they converge to zero. >>> for n in [2, 3, 4, 5, 6, 7]: ... x = rng.normal(size=10**n) ... m, k = stats.moment(x, 3), stats.kstat(x, 3) ... print("%.3g %.3g %.3g" % (m, k, m-k)) -0.631 -0.651 0.0194 # random 0.0282 0.0283 -8.49e-05 -0.0454 -0.0454 1.36e-05 7.53e-05 7.53e-05 -2.26e-09 0.00166 0.00166 -4.99e-09 -2.88e-06 -2.88e-06 8.63e-13 rz'k-statistics only supported for 1<=n<=4rzData input must not be emptyaxis?rSrVi @zShould not be here.N) rIintnpr float64rsizeisnansumnanrange)rLr^SNkrQrQrRr)s6A$ L Fr)cCst|}t|}|dkr,t|ddd|S|dkrtt|dd}t|dd}d||d|d|||dStddS)a#Return an unbiased estimator of the variance of the k-statistic. See `kstat` for more details of the k-statistic. Parameters ---------- data : array_like Input array. Note that n-D input gets flattened. n : int, {1, 2}, optional Default is equal to 2. Returns ------- kstatvar : float The nth k-statistic variance. See Also -------- kstat: Returns the n-th k-statistic. moment: Returns the n-th central moment about the mean for a sample. Notes ----- The variances of the first few k-statistics are given by: .. math:: var(k_{1}) = \frac{\kappa^2}{n} var(k_{2}) = \frac{\kappa^4}{n} + \frac{2\kappa^2_{2}}{n - 1} var(k_{3}) = \frac{\kappa^6}{n} + \frac{9 \kappa_2 \kappa_4}{n - 1} + \frac{9 \kappa^2_{3}}{n - 1} + \frac{6 n \kappa^3_{2}}{(n-1) (n-2)} var(k_{4}) = \frac{\kappa^8}{n} + \frac{16 \kappa_2 \kappa_6}{n - 1} + \frac{48 \kappa_{3} \kappa_5}{n - 1} + \frac{34 \kappa^2_{4}}{n-1} + \frac{72 n \kappa^2_{2} \kappa_4}{(n - 1) (n - 2)} + \frac{144 n \kappa_{2} \kappa^2_{3}}{(n - 1) (n - 2)} + \frac{24 (n + 1) n \kappa^4_{2}}{(n - 1) (n - 2) (n - 3)} rrS)r^rgrdzOnly n=1 or n=2 supported.N)rrXr)rI)rLr^rtZk2Zk4rQrQrRr*5s'  (r*cCsXtj|tjd}dd||d<d|d|d<td|}|d|d |dd<|S) a'Approximations of uniform order statistic medians. Parameters ---------- n : int Sample size. Returns ------- v : 1d float array Approximations of the order statistic medians. References ---------- .. [1] James J. Filliben, "The Probability Plot Correlation Coefficient Test for Normality", Technometrics, Vol. 17, pp. 111-117, 1975. Examples -------- Order statistics of the uniform distribution on the unit interval are marginally distributed according to beta distributions. The expectations of these order statistic are evenly spaced across the interval, but the distributions are skewed in a way that pushes the medians slightly towards the endpoints of the unit interval: >>> n = 4 >>> k = np.arange(1, n+1) >>> from scipy.stats import beta >>> a = k >>> b = n-k+1 >>> beta.mean(a, b) array([0.2, 0.4, 0.6, 0.8]) >>> beta.median(a, b) array([0.15910358, 0.38572757, 0.61427243, 0.84089642]) The Filliben approximation uses the exact medians of the smallest and greatest order statistics, and the remaining medians are approximated by points spread evenly across a sub-interval of the unit interval: >>> from scipy.morestats import _calc_uniform_order_statistic_medians >>> _calc_uniform_order_statistic_medians(n) array([0.15910358, 0.38545246, 0.61454754, 0.84089642]) This plot shows the skewed distributions of the order statistics of a sample of size four from a uniform distribution on the unit interval: >>> import matplotlib.pyplot as plt >>> x = np.linspace(0.0, 1.0, num=50, endpoint=True) >>> pdfs = [beta.pdf(x, a[i], b[i]) for i in range(n)] >>> plt.figure() >>> plt.plot(x, pdfs[0], x, pdfs[1], x, pdfs[2], x, pdfs[3]) dtype?rgrrrSgRQ?g\(\?)rlemptyrmr )r^rOirQrQrR%_calc_uniform_order_statistic_medianshs 6 r|Tc Csnt|tr n^t|trZztt|}WqjtyV}ztd||WYd}~qjd}~00n|rjd}t||S)aParse `dist` keyword. Parameters ---------- dist : str or stats.distributions instance. Several functions take `dist` as a keyword, hence this utility function. enforce_subclass : bool, optional If True (default), `dist` needs to be a `_distn_infrastructure.rv_generic` instance. It can sometimes be useful to set this keyword to False, if a function wants to accept objects that just look somewhat like such an instance (for example, they have a ``ppf`` method). z#%s is not a valid distribution nameNza`dist` should be a stats.distributions instance or a string with the name of such a distribution.) isinstancer%strgetattrr$AttributeErrorrI)distenforce_subclassemsgrQrQrR_parse_dist_kws  &rcCsdzLt|dr,||||||n||||||Wnty^Yn0dS)z>Helper function to add axes labels and a title to stats plots. set_titleN)hasattrrZ set_xlabelZ set_ylabeltitlexlabelylabel Exception)plotrrrrQrQrR_add_axis_labels_titles       rrQrZFcCspt|}|jdkr6|r.||ftjtjdffS||fStt|}t|dd}|durZd}t|rh|f}t|t szt |}|j |g|R}t |}|rt ||\} } } } } |durL|||d|r||| || dt|d d d d |rLt|}t|}t|}t|}|d ||}|d||}|||d| d|rd||f| | | ffS||fSdS)a Calculate quantiles for a probability plot, and optionally show the plot. Generates a probability plot of sample data against the quantiles of a specified theoretical distribution (the normal distribution by default). `probplot` optionally calculates a best-fit line for the data and plots the results using Matplotlib or a given plot function. Parameters ---------- x : array_like Sample/response data from which `probplot` creates the plot. sparams : tuple, optional Distribution-specific shape parameters (shape parameters plus location and scale). dist : str or stats.distributions instance, optional Distribution or distribution function name. The default is 'norm' for a normal probability plot. Objects that look enough like a stats.distributions instance (i.e. they have a ``ppf`` method) are also accepted. fit : bool, optional Fit a least-squares regression (best-fit) line to the sample data if True (default). plot : object, optional If given, plots the quantiles. If given and `fit` is True, also plots the least squares fit. `plot` is an object that has to have methods "plot" and "text". The `matplotlib.pyplot` module or a Matplotlib Axes object can be used, or a custom object with the same methods. Default is None, which means that no plot is created. Returns ------- (osm, osr) : tuple of ndarrays Tuple of theoretical quantiles (osm, or order statistic medians) and ordered responses (osr). `osr` is simply sorted input `x`. For details on how `osm` is calculated see the Notes section. (slope, intercept, r) : tuple of floats, optional Tuple containing the result of the least-squares fit, if that is performed by `probplot`. `r` is the square root of the coefficient of determination. If ``fit=False`` and ``plot=None``, this tuple is not returned. Notes ----- Even if `plot` is given, the figure is not shown or saved by `probplot`; ``plt.show()`` or ``plt.savefig('figname.png')`` should be used after calling `probplot`. `probplot` generates a probability plot, which should not be confused with a Q-Q or a P-P plot. Statsmodels has more extensive functionality of this type, see ``statsmodels.api.ProbPlot``. The formula used for the theoretical quantiles (horizontal axis of the probability plot) is Filliben's estimate:: quantiles = dist.ppf(val), for 0.5**(1/n), for i = n val = (i - 0.3175) / (n + 0.365), for i = 2, ..., n-1 1 - 0.5**(1/n), for i = 1 where ``i`` indicates the i-th ordered value and ``n`` is the total number of values. Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt >>> nsample = 100 >>> rng = np.random.default_rng() A t distribution with small degrees of freedom: >>> ax1 = plt.subplot(221) >>> x = stats.t.rvs(3, size=nsample, random_state=rng) >>> res = stats.probplot(x, plot=plt) A t distribution with larger degrees of freedom: >>> ax2 = plt.subplot(222) >>> x = stats.t.rvs(25, size=nsample, random_state=rng) >>> res = stats.probplot(x, plot=plt) A mixture of two normal distributions with broadcasting: >>> ax3 = plt.subplot(223) >>> x = stats.norm.rvs(loc=[0,5], scale=[1,1.5], ... size=(nsample//2,2), random_state=rng).ravel() >>> res = stats.probplot(x, plot=plt) A standard normal distribution: >>> ax4 = plt.subplot(224) >>> x = stats.norm.rvs(loc=0, scale=1, size=nsample, random_state=rng) >>> res = stats.probplot(x, plot=plt) Produce a new figure with a loggamma distribution, using the ``dist`` and ``sparams`` keywords: >>> fig = plt.figure() >>> ax = fig.add_subplot(111) >>> x = stats.loggamma.rvs(c=2.5, size=500, random_state=rng) >>> res = stats.probplot(x, dist=stats.loggamma, sparams=(2.5,), plot=ax) >>> ax.set_title("Probplot for loggamma dist with shape parameter 2.5") Show the results with Matplotlib: >>> plt.show() rF)rNrQZbozr-zTheoretical quantileszOrdered ValueszProbability Plotrrrgffffff?{Gz?z $R^2=%1.4f$rS)rlr rnrqr|rXrrr}tupleppfr rZ linregressrrr rtext)r]ZsparamsrfitrZrvalue osm_uniformZosmosrZslopeZ interceptrprob_ZxminZxmaxZyminZymaxZposxZposyrQrQrRr+sHp      r+rrg tukeylambdacCs<t|}tt|}t|}dd}tj|||||jfdS)a Calculate the shape parameter that maximizes the PPCC. The probability plot correlation coefficient (PPCC) plot can be used to determine the optimal shape parameter for a one-parameter family of distributions. ``ppcc_max`` returns the shape parameter that would maximize the probability plot correlation coefficient for the given data to a one-parameter family of distributions. Parameters ---------- x : array_like Input array. brack : tuple, optional Triple (a,b,c) where (a>> from scipy import stats >>> import matplotlib.pyplot as plt >>> rng = np.random.default_rng() >>> c = 2.5 >>> x = stats.weibull_min.rvs(c, scale=4, size=2000, random_state=rng) Generate the PPCC plot for this data with the Weibull distribution. >>> fig, ax = plt.subplots(figsize=(8, 6)) >>> res = stats.ppcc_plot(x, c/2, 2*c, dist='weibull_min', plot=ax) We calculate the value where the shape should reach its maximum and a red line is drawn there. The line should coincide with the highest point in the PPCC graph. >>> cmax = stats.ppcc_max(x, brack=(c/2, 2*c), dist='weibull_min') >>> ax.axvline(cmax, color='r') >>> plt.show() cSs"|||}t||\}}d|SNr)rpearsonr)shapemiyvalsfuncxvalsrrrQrQrRtempfuncs zppcc_max..tempfuncbrackargs)rr|rXr rbrentr)r]rrrrrrQrQrRr,vsF  r,Pc Cs||krtdtj|||d}t|}t|D](\}} t|| |dd\} } | d||<q2|dur|||dt|dd d |d ||fS) a9 Calculate and optionally plot probability plot correlation coefficient. The probability plot correlation coefficient (PPCC) plot can be used to determine the optimal shape parameter for a one-parameter family of distributions. It cannot be used for distributions without shape parameters (like the normal distribution) or with multiple shape parameters. By default a Tukey-Lambda distribution (`stats.tukeylambda`) is used. A Tukey-Lambda PPCC plot interpolates from long-tailed to short-tailed distributions via an approximately normal one, and is therefore particularly useful in practice. Parameters ---------- x : array_like Input array. a, b : scalar Lower and upper bounds of the shape parameter to use. dist : str or stats.distributions instance, optional Distribution or distribution function name. Objects that look enough like a stats.distributions instance (i.e. they have a ``ppf`` method) are also accepted. The default is ``'tukeylambda'``. plot : object, optional If given, plots PPCC against the shape parameter. `plot` is an object that has to have methods "plot" and "text". The `matplotlib.pyplot` module or a Matplotlib Axes object can be used, or a custom object with the same methods. Default is None, which means that no plot is created. N : int, optional Number of points on the horizontal axis (equally distributed from `a` to `b`). Returns ------- svals : ndarray The shape values for which `ppcc` was calculated. ppcc : ndarray The calculated probability plot correlation coefficient values. See Also -------- ppcc_max, probplot, boxcox_normplot, tukeylambda References ---------- J.J. Filliben, "The Probability Plot Correlation Coefficient Test for Normality", Technometrics, Vol. 17, pp. 111-117, 1975. Examples -------- First we generate some random data from a Weibull distribution with shape parameter 2.5, and plot the histogram of the data: >>> from scipy import stats >>> import matplotlib.pyplot as plt >>> rng = np.random.default_rng() >>> c = 2.5 >>> x = stats.weibull_min.rvs(c, scale=4, size=2000, random_state=rng) Take a look at the histogram of the data. >>> fig1, ax = plt.subplots(figsize=(9, 4)) >>> ax.hist(x, bins=50) >>> ax.set_title('Histogram of x') >>> plt.show() Now we explore this data with a PPCC plot as well as the related probability plot and Box-Cox normplot. A red line is drawn where we expect the PPCC value to be maximal (at the shape parameter ``c`` used above): >>> fig2 = plt.figure(figsize=(12, 4)) >>> ax1 = fig2.add_subplot(1, 3, 1) >>> ax2 = fig2.add_subplot(1, 3, 2) >>> ax3 = fig2.add_subplot(1, 3, 3) >>> res = stats.probplot(x, plot=ax1) >>> res = stats.boxcox_normplot(x, -4, 4, plot=ax2) >>> res = stats.ppcc_plot(x, c/2, 2*c, dist='weibull_min', plot=ax3) >>> ax3.axvline(c, color='r') >>> plt.show() z`b` has to be larger than `a`.numTrrryNr]z Shape ValuesProb Plot Corr. Coef.z(%s) PPCC Plotr)rIrllinspace empty_like enumerater+rr) r]abrrrtZsvalsppccruZsvalrZr2rQrQrRr-sT r-cCst|}|jd}|dkr"tjSt|}|dkrDtj|dd}ntj|||dd}|dtj|dd|dt|S)aK The boxcox log-likelihood function. Parameters ---------- lmb : scalar Parameter for Box-Cox transformation. See `boxcox` for details. data : array_like Data to calculate Box-Cox log-likelihood for. If `data` is multi-dimensional, the log-likelihood is calculated along the first axis. Returns ------- llf : float or ndarray Box-Cox log-likelihood of `data` given `lmb`. A float for 1-D `data`, an array otherwise. See Also -------- boxcox, probplot, boxcox_normplot, boxcox_normmax Notes ----- The Box-Cox log-likelihood function is defined here as .. math:: llf = (\lambda - 1) \sum_i(\log(x_i)) - N/2 \log(\sum_i (y_i - \bar{y})^2 / N), where ``y`` is the Box-Cox transformed input data ``x``. Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt >>> from mpl_toolkits.axes_grid1.inset_locator import inset_axes Generate some random variates and calculate Box-Cox log-likelihood values for them for a range of ``lmbda`` values: >>> rng = np.random.default_rng() >>> x = stats.loggamma.rvs(5, loc=10, size=1000, random_state=rng) >>> lmbdas = np.linspace(-2, 10) >>> llf = np.zeros(lmbdas.shape, dtype=float) >>> for ii, lmbda in enumerate(lmbdas): ... llf[ii] = stats.boxcox_llf(lmbda, x) Also find the optimal lmbda value with `boxcox`: >>> x_most_normal, lmbda_optimal = stats.boxcox(x) Plot the log-likelihood as function of lmbda. Add the optimal lmbda as a horizontal line to check that that's really the optimum: >>> fig = plt.figure() >>> ax = fig.add_subplot(111) >>> ax.plot(lmbdas, llf, 'b.-') >>> ax.axhline(stats.boxcox_llf(lmbda_optimal, x), color='r') >>> ax.set_xlabel('lmbda parameter') >>> ax.set_ylabel('Box-Cox log-likelihood') Now add some probability plots to show that where the log-likelihood is maximized the data transformed with `boxcox` looks closest to normal: >>> locs = [3, 10, 4] # 'lower left', 'center', 'lower right' >>> for lmbda, loc in zip([-1, lmbda_optimal, 9], locs): ... xt = stats.boxcox(x, lmbda=lmbda) ... (osm, osr), (slope, intercept, r_sq) = stats.probplot(xt) ... ax_inset = inset_axes(ax, width="20%", height="20%", loc=loc) ... ax_inset.plot(osm, osr, 'c.', osm, slope*osm + intercept, 'k-') ... ax_inset.set_xticklabels([]) ... ax_inset.set_yticklabels([]) ... ax_inset.set_title(r'$\lambda=%1.2f$' % lmbda) >>> plt.show() rrerrS)rlr rrqrrYrp)lmbrLrtZlogdataZvariancerQrQrRr.3sO   r.c Csdtjd|d}t|||}dd}|d}d}||||dkrb|dkrb|d7}|d7}q8|dkrrtd tj|||||fd }|d}d}||||dkr|dkr|d8}|d7}q|dkrtd tj|||||fd } | |fS) NrxrcSst|||SNr.)lmbdarLtargetrQrQrRrootfuncsz'_boxcox_conf_interval..rootfuncrri皙?zCould not find endpoint.r)r$chi2rr. RuntimeErrorrZbrentq) r]lmaxrMrbrrZnewlmrtZlmplusZlmminusrQrQrR_boxcox_conf_intervals(  rcCst|}|jdkrtd|jdkr*|St||dkrDtdt|dkrZtd|durnt||St |d|d}t||}|dur||fSt |||}|||fSdS) a?Return a dataset transformed by a Box-Cox power transformation. Parameters ---------- x : ndarray Input array. Must be positive 1-dimensional. Must not be constant. lmbda : {None, scalar}, optional If `lmbda` is not None, do the transformation for that value. If `lmbda` is None, find the lambda that maximizes the log-likelihood function and return it as the second output argument. alpha : {None, float}, optional If ``alpha`` is not None, return the ``100 * (1-alpha)%`` confidence interval for `lmbda` as the third output argument. Must be between 0.0 and 1.0. optimizer : callable, optional If `lmbda` is None, `optimizer` is the scalar optimizer used to find the value of `lmbda` that minimizes the negative log-likelihood function. `optimizer` is a callable that accepts one argument: fun : callable The objective function, which evaluates the negative log-likelihood function at a provided value of `lmbda` and returns an object, such as an instance of `scipy.optimize.OptimizeResult`, which holds the optimal value of `lmbda` in an attribute `x`. See the example in `boxcox_normmax` or the documentation of `scipy.optimize.minimize_scalar` for more information. If `lmbda` is not None, `optimizer` is ignored. Returns ------- boxcox : ndarray Box-Cox power transformed array. maxlog : float, optional If the `lmbda` parameter is None, the second returned argument is the lambda that maximizes the log-likelihood function. (min_ci, max_ci) : tuple of float, optional If `lmbda` parameter is None and ``alpha`` is not None, this returned tuple of floats represents the minimum and maximum confidence limits given ``alpha``. See Also -------- probplot, boxcox_normplot, boxcox_normmax, boxcox_llf Notes ----- The Box-Cox transform is given by:: y = (x**lmbda - 1) / lmbda, for lmbda != 0 log(x), for lmbda = 0 `boxcox` requires the input data to be positive. Sometimes a Box-Cox transformation provides a shift parameter to achieve this; `boxcox` does not. Such a shift parameter is equivalent to adding a positive constant to `x` before calling `boxcox`. The confidence limits returned when ``alpha`` is provided give the interval where: .. math:: llf(\hat{\lambda}) - llf(\lambda) < \frac{1}{2}\chi^2(1 - \alpha, 1), with ``llf`` the log-likelihood function and :math:`\chi^2` the chi-squared function. References ---------- G.E.P. Box and D.R. Cox, "An Analysis of Transformations", Journal of the Royal Statistical Society B, 26, 211-252 (1964). Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt We generate some random variates from a non-normal distribution and make a probability plot for it, to show it is non-normal in the tails: >>> fig = plt.figure() >>> ax1 = fig.add_subplot(211) >>> x = stats.loggamma.rvs(5, size=500) + 5 >>> prob = stats.probplot(x, dist=stats.norm, plot=ax1) >>> ax1.set_xlabel('') >>> ax1.set_title('Probplot against normal distribution') We now use `boxcox` to transform the data so it's closest to normal: >>> ax2 = fig.add_subplot(212) >>> xt, _ = stats.boxcox(x) >>> prob = stats.probplot(xt, dist=stats.norm, plot=ax2) >>> ax2.set_title('Probplot after Box-Cox transformation') >>> plt.show() rzData must be 1-dimensional.rzData must not be constant.zData must be positive.Nmle)method optimizer) rlr ndimrIrnallanyrr/r0r)r]rrMrryrKrQrQrRr/s"e      r/rc sdur"durdfddn,ts2tddurBtdfddfdd fd d fd d }|d}||vrtd|||}||}|durd}t||S)aTCompute optimal Box-Cox transform parameter for input data. Parameters ---------- x : array_like Input array. brack : 2-tuple, optional, default (-2.0, 2.0) The starting interval for a downhill bracket search for the default `optimize.brent` solver. Note that this is in most cases not critical; the final result is allowed to be outside this bracket. If `optimizer` is passed, `brack` must be None. method : str, optional The method to determine the optimal transform parameter (`boxcox` ``lmbda`` parameter). Options are: 'pearsonr' (default) Maximizes the Pearson correlation coefficient between ``y = boxcox(x)`` and the expected values for ``y`` if `x` would be normally-distributed. 'mle' Minimizes the log-likelihood `boxcox_llf`. This is the method used in `boxcox`. 'all' Use all optimization methods available, and return all results. Useful to compare different methods. optimizer : callable, optional `optimizer` is a callable that accepts one argument: fun : callable The objective function to be optimized. `fun` accepts one argument, the Box-Cox transform parameter `lmbda`, and returns the negative log-likelihood function at the provided value. The job of `optimizer` is to find the value of `lmbda` that minimizes `fun`. and returns an object, such as an instance of `scipy.optimize.OptimizeResult`, which holds the optimal value of `lmbda` in an attribute `x`. See the example below or the documentation of `scipy.optimize.minimize_scalar` for more information. Returns ------- maxlog : float or ndarray The optimal transform parameter found. An array instead of a scalar for ``method='all'``. See Also -------- boxcox, boxcox_llf, boxcox_normplot, scipy.optimize.minimize_scalar Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt We can generate some data and determine the optimal ``lmbda`` in various ways: >>> rng = np.random.default_rng() >>> x = stats.loggamma.rvs(5, size=30, random_state=rng) + 5 >>> y, lmax_mle = stats.boxcox(x) >>> lmax_pearsonr = stats.boxcox_normmax(x) >>> lmax_mle 1.4613865614008015 >>> lmax_pearsonr 1.6685004886804342 >>> stats.boxcox_normmax(x, method='all') array([1.66850049, 1.46138656]) >>> fig = plt.figure() >>> ax = fig.add_subplot(111) >>> prob = stats.boxcox_normplot(x, -10, 10, plot=ax) >>> ax.axvline(lmax_mle, color='r') >>> ax.axvline(lmax_pearsonr, color='g', ls='--') >>> plt.show() Alternatively, we can define our own `optimizer` function. Suppose we are only interested in values of `lmbda` on the interval [6, 7], we want to use `scipy.optimize.minimize_scalar` with ``method='bounded'``, and we want to use tighter tolerances when optimizing the log-likelihood function. To do this, we define a function that accepts positional argument `fun` and uses `scipy.optimize.minimize_scalar` to minimize `fun` subject to the provided bounds and tolerances: >>> from scipy import optimize >>> options = {'xatol': 1e-12} # absolute tolerance on `x` >>> def optimizer(fun): ... return optimize.minimize_scalar(fun, bounds=(6, 7), ... method="bounded", options=options) >>> stats.boxcox_normmax(x, optimizer=optimizer) 6.000... N)grVcstj||dS)N)rrrr)rr)rrQrR _optimizersz"boxcox_normmax.._optimizerz`optimizer` must be a callablez,`brack` must be None if `optimizer` is givencsfdd}t|ddS)Ncs|gRSrrQr]rrrQrR func_wrappedsz8boxcox_normmax.._optimizer..func_wrappedr])r)rrr)rrrRrscs0tt|}tj|}dd}|||fdS)NcSs,t||}t|}t||\}}d|Sr)r/rlr rr)rrZsampsrrrrrQrQrR_eval_pearsonrs  z9boxcox_normmax.._pearsonr.._eval_pearsonrr)r|rXr$rZr)r]rrrrrQrR _pearsonrs   z!boxcox_normmax.._pearsonrcsdd}||fdS)NcSs t|| Srr)rrLrQrQrR _eval_mlesz/boxcox_normmax.._mle.._eval_mlerrQ)r]rrrQrR_mleszboxcox_normmax.._mlecs*tjdtd}||d<||d<|S)NrSrvrr)rlrzfloat)r]Zmaxlog)rrrQrR_alls  zboxcox_normmax.._all)rrrzMethod %s not recognized.zQ`optimizer` must return an object containing the optimal `lmbda` in attribute `x`)callablerIkeys) r]rrrrmethodsZ optimfuncresmessagerQ)rrrrrrRr09s0c     r0cCs|dkrd}t}nd}t}t|}|jdkr2|S||krBtdtj|||d}|d} t|D]4\} } ||| d} t| d d d \} \} } }|| | <qb|d ur| || d t |dd|d|| fS)zCompute parameters for a Box-Cox or Yeo-Johnson normality plot, optionally show it. See `boxcox_normplot` or `yeojohnson_normplot` for details. r/zBox-Cox Normality PlotzYeo-Johnson Normality Plotrz `lb` has to be larger than `la`.rr)rrZTrNr]z $\lambda$rr) r/rArlr rnrIrrr+rr)rr]lalbrrtrZtransform_funcZlmbdasrr{rczrrrQrQrR _normplots.    rcCstd|||||S)adCompute parameters for a Box-Cox normality plot, optionally show it. A Box-Cox normality plot shows graphically what the best transformation parameter is to use in `boxcox` to obtain a distribution that is close to normal. Parameters ---------- x : array_like Input array. la, lb : scalar The lower and upper bounds for the ``lmbda`` values to pass to `boxcox` for Box-Cox transformations. These are also the limits of the horizontal axis of the plot if that is generated. plot : object, optional If given, plots the quantiles and least squares fit. `plot` is an object that has to have methods "plot" and "text". The `matplotlib.pyplot` module or a Matplotlib Axes object can be used, or a custom object with the same methods. Default is None, which means that no plot is created. N : int, optional Number of points on the horizontal axis (equally distributed from `la` to `lb`). Returns ------- lmbdas : ndarray The ``lmbda`` values for which a Box-Cox transform was done. ppcc : ndarray Probability Plot Correlelation Coefficient, as obtained from `probplot` when fitting the Box-Cox transformed input `x` against a normal distribution. See Also -------- probplot, boxcox, boxcox_normmax, boxcox_llf, ppcc_max Notes ----- Even if `plot` is given, the figure is not shown or saved by `boxcox_normplot`; ``plt.show()`` or ``plt.savefig('figname.png')`` should be used after calling `probplot`. Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt Generate some non-normally distributed data, and create a Box-Cox plot: >>> x = stats.loggamma.rvs(5, size=500) + 5 >>> fig = plt.figure() >>> ax = fig.add_subplot(111) >>> prob = stats.boxcox_normplot(x, -20, 20, plot=ax) Determine and plot the optimal ``lmbda`` to transform ``x`` and plot it in the same plot: >>> _, maxlog = stats.boxcox(x) >>> ax.axvline(maxlog, color='r') >>> plt.show() r/rr]rrrrtrQrQrRr1sAr1cCs|t|}|jdkr|St|jtjr0tdt|jtjrP|jtj dd}|durbt ||St |}t ||}||fS)aReturn a dataset transformed by a Yeo-Johnson power transformation. Parameters ---------- x : ndarray Input array. Should be 1-dimensional. lmbda : float, optional If ``lmbda`` is ``None``, find the lambda that maximizes the log-likelihood function and return it as the second output argument. Otherwise the transformation is done for the given value. Returns ------- yeojohnson: ndarray Yeo-Johnson power transformed array. maxlog : float, optional If the `lmbda` parameter is None, the second returned argument is the lambda that maximizes the log-likelihood function. See Also -------- probplot, yeojohnson_normplot, yeojohnson_normmax, yeojohnson_llf, boxcox Notes ----- The Yeo-Johnson transform is given by:: y = ((x + 1)**lmbda - 1) / lmbda, for x >= 0, lmbda != 0 log(x + 1), for x >= 0, lmbda = 0 -((-x + 1)**(2 - lmbda) - 1) / (2 - lmbda), for x < 0, lmbda != 2 -log(-x + 1), for x < 0, lmbda = 2 Unlike `boxcox`, `yeojohnson` does not require the input data to be positive. .. versionadded:: 1.2.0 References ---------- I. Yeo and R.A. Johnson, "A New Family of Power Transformations to Improve Normality or Symmetry", Biometrika 87.4 (2000): Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt We generate some random variates from a non-normal distribution and make a probability plot for it, to show it is non-normal in the tails: >>> fig = plt.figure() >>> ax1 = fig.add_subplot(211) >>> x = stats.loggamma.rvs(5, size=500) + 5 >>> prob = stats.probplot(x, dist=stats.norm, plot=ax1) >>> ax1.set_xlabel('') >>> ax1.set_title('Probplot against normal distribution') We now use `yeojohnson` to transform the data so it's closest to normal: >>> ax2 = fig.add_subplot(212) >>> xt, lmbda = stats.yeojohnson(x) >>> prob = stats.probplot(xt, dist=stats.norm, plot=ax2) >>> ax2.set_title('Probplot after Yeo-Johnson transformation') >>> plt.show() rz>Yeo-Johnson transformation is not defined for complex numbers.F)copyN) rlr rnZ issubdtyperwZcomplexfloatingrIintegerastyperm_yeojohnson_transformrB)r]rrrrQrQrRrAKsF    rAcCst|}|dk}t|tdkr8t||||<n t||d|d|||<t|dtdkrt|| dd|d d|||<nt||  ||<|S)zaReturns `x` transformed by the Yeo-Johnson power transform with given parameter `lmbda`. rrgrrS)rlZ zeros_likeabsspacinglog1ppower)r]routposrQrQrRrs  2rcCs~t|}|jd}|dkr"tjSt||}| dt|jdd}||dt|tt|dj dd7}|S)av The yeojohnson log-likelihood function. Parameters ---------- lmb : scalar Parameter for Yeo-Johnson transformation. See `yeojohnson` for details. data : array_like Data to calculate Yeo-Johnson log-likelihood for. If `data` is multi-dimensional, the log-likelihood is calculated along the first axis. Returns ------- llf : float Yeo-Johnson log-likelihood of `data` given `lmb`. See Also -------- yeojohnson, probplot, yeojohnson_normplot, yeojohnson_normmax Notes ----- The Yeo-Johnson log-likelihood function is defined here as .. math:: llf = -N/2 \log(\hat{\sigma}^2) + (\lambda - 1) \sum_i \text{ sign }(x_i)\log(|x_i| + 1) where :math:`\hat{\sigma}^2` is estimated variance of the the Yeo-Johnson transformed input data ``x``. .. versionadded:: 1.2.0 Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt >>> from mpl_toolkits.axes_grid1.inset_locator import inset_axes Generate some random variates and calculate Yeo-Johnson log-likelihood values for them for a range of ``lmbda`` values: >>> x = stats.loggamma.rvs(5, loc=10, size=1000) >>> lmbdas = np.linspace(-2, 10) >>> llf = np.zeros(lmbdas.shape, dtype=float) >>> for ii, lmbda in enumerate(lmbdas): ... llf[ii] = stats.yeojohnson_llf(lmbda, x) Also find the optimal lmbda value with `yeojohnson`: >>> x_most_normal, lmbda_optimal = stats.yeojohnson(x) Plot the log-likelihood as function of lmbda. Add the optimal lmbda as a horizontal line to check that that's really the optimum: >>> fig = plt.figure() >>> ax = fig.add_subplot(111) >>> ax.plot(lmbdas, llf, 'b.-') >>> ax.axhline(stats.yeojohnson_llf(lmbda_optimal, x), color='r') >>> ax.set_xlabel('lmbda parameter') >>> ax.set_ylabel('Yeo-Johnson log-likelihood') Now add some probability plots to show that where the log-likelihood is maximized the data transformed with `yeojohnson` looks closest to normal: >>> locs = [3, 10, 4] # 'lower left', 'center', 'lower right' >>> for lmbda, loc in zip([-1, lmbda_optimal, 9], locs): ... xt = stats.yeojohnson(x, lmbda=lmbda) ... (osm, osr), (slope, intercept, r_sq) = stats.probplot(xt) ... ax_inset = inset_axes(ax, width="20%", height="20%", loc=loc) ... ax_inset.plot(osm, osr, 'c.', osm, slope*osm + intercept, 'k-') ... ax_inset.set_xticklabels([]) ... ax_inset.set_yticklabels([]) ... ax_inset.set_title(r'$\lambda=%1.2f$' % lmbda) >>> plt.show() rrSrer) rlr rrqrrrYsignrrp)rrLZ n_samplesZtransZloglikerQrQrRr@sQ   2r@rWrScCsdd}tj|||fdS)aCompute optimal Yeo-Johnson transform parameter. Compute optimal Yeo-Johnson transform parameter for input data, using maximum likelihood estimation. Parameters ---------- x : array_like Input array. brack : 2-tuple, optional The starting interval for a downhill bracket search with `optimize.brent`. Note that this is in most cases not critical; the final result is allowed to be outside this bracket. Returns ------- maxlog : float The optimal transform parameter found. See Also -------- yeojohnson, yeojohnson_llf, yeojohnson_normplot Notes ----- .. versionadded:: 1.2.0 Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt Generate some data and determine optimal ``lmbda`` >>> rng = np.random.default_rng() >>> x = stats.loggamma.rvs(5, size=30, random_state=rng) + 5 >>> lmax = stats.yeojohnson_normmax(x) >>> fig = plt.figure() >>> ax = fig.add_subplot(111) >>> prob = stats.yeojohnson_normplot(x, -10, 10, plot=ax) >>> ax.axvline(lmax, color='r') >>> plt.show() cSs t|| Sr)r@)rrLrQrQrR_neg_llfJsz$yeojohnson_normmax.._neg_llfrr)r]rrrQrQrRrBs/rBcCstd|||||S)aCompute parameters for a Yeo-Johnson normality plot, optionally show it. A Yeo-Johnson normality plot shows graphically what the best transformation parameter is to use in `yeojohnson` to obtain a distribution that is close to normal. Parameters ---------- x : array_like Input array. la, lb : scalar The lower and upper bounds for the ``lmbda`` values to pass to `yeojohnson` for Yeo-Johnson transformations. These are also the limits of the horizontal axis of the plot if that is generated. plot : object, optional If given, plots the quantiles and least squares fit. `plot` is an object that has to have methods "plot" and "text". The `matplotlib.pyplot` module or a Matplotlib Axes object can be used, or a custom object with the same methods. Default is None, which means that no plot is created. N : int, optional Number of points on the horizontal axis (equally distributed from `la` to `lb`). Returns ------- lmbdas : ndarray The ``lmbda`` values for which a Yeo-Johnson transform was done. ppcc : ndarray Probability Plot Correlelation Coefficient, as obtained from `probplot` when fitting the Box-Cox transformed input `x` against a normal distribution. See Also -------- probplot, yeojohnson, yeojohnson_normmax, yeojohnson_llf, ppcc_max Notes ----- Even if `plot` is given, the figure is not shown or saved by `boxcox_normplot`; ``plt.show()`` or ``plt.savefig('figname.png')`` should be used after calling `probplot`. .. versionadded:: 1.2.0 Examples -------- >>> from scipy import stats >>> import matplotlib.pyplot as plt Generate some non-normally distributed data, and create a Yeo-Johnson plot: >>> x = stats.loggamma.rvs(5, size=500) + 5 >>> fig = plt.figure() >>> ax = fig.add_subplot(111) >>> prob = stats.yeojohnson_normplot(x, -20, 20, plot=ax) Determine and plot the optimal ``lmbda`` to transform ``x`` and plot it in the same plot: >>> _, maxlog = stats.yeojohnson(x) >>> ax.axvline(maxlog, color='r') >>> plt.show() rArrrQrQrRrCPsCrC ShapiroResult)rEZpvaluecCst|}t|}|dkr"tdt|d}d}t|}t||d|d|\}}}}|dvrlt d|d kr~t d t ||S) a Perform the Shapiro-Wilk test for normality. The Shapiro-Wilk test tests the null hypothesis that the data was drawn from a normal distribution. Parameters ---------- x : array_like Array of sample data. Returns ------- statistic : float The test statistic. p-value : float The p-value for the hypothesis test. See Also -------- anderson : The Anderson-Darling test for normality kstest : The Kolmogorov-Smirnov test for goodness of fit. Notes ----- The algorithm used is described in [4]_ but censoring parameters as described are not implemented. For N > 5000 the W test statistic is accurate but the p-value may not be. The chance of rejecting the null hypothesis when it is true is close to 5% regardless of sample size. References ---------- .. [1] https://www.itl.nist.gov/div898/handbook/prc/section2/prc213.htm .. [2] Shapiro, S. S. & Wilk, M.B (1965). An analysis of variance test for normality (complete samples), Biometrika, Vol. 52, pp. 591-611. .. [3] Razali, N. M. & Wah, Y. B. (2011) Power comparisons of Shapiro-Wilk, Kolmogorov-Smirnov, Lilliefors and Anderson-Darling tests, Journal of Statistical Modeling and Analytics, Vol. 2, pp. 21-33. .. [4] ALGORITHM AS R94 APPL. STATIST. (1995) VOL. 44, NO. 4. Examples -------- >>> from scipy import stats >>> rng = np.random.default_rng() >>> x = stats.norm.rvs(loc=5, scale=3, size=100, random_state=rng) >>> shapiro_test = stats.shapiro(x) >>> shapiro_test ShapiroResult(statistic=0.9813305735588074, pvalue=0.16855233907699585) >>> shapiro_test.statistic 0.9813305735588074 >>> shapiro_test.pvalue 0.16855233907699585 rhzData must be at least length 3.frNrS)rrSzGInput data for shapiro has range zero. The results may not be accurate.iz)p-value may not be accurate for N > 5000.) rlrrXrIr r rZswilkwarningswarnr)r]rtrinitrwpwZifaultrQrQrRr2s8  "  r2)g;On?gˡE?gv/?gK7A`?gFx?)g/$?gsh|??g~jt?gV-?gZd;O?)gtV?gMb?gMbX9?gMb?gS㥛?)g$C?gjt?gQ?gS㥛?gˡE?g)\(?AndersonResult)rEZcritical_valuesZsignificance_levelcCs|dvrtdt|}tj|dd}t|}|dkrtj|ddd}|||}tj|}tj |}t gd} t t d d |d ||d } n|d kr||}tj |}tj |}t gd} t td d|d } nP|dkrzdd} t |tj|dddg} tj| | ||fdd} || d| d}tj|}tj |}t gd} t td d|d } n|dkrtj|\}}|||}tj|}tj |}t gd} t td dt|d } nZtj|\}}|||}tj|}tj |}t gd} t td dt|d } td|d}| tjd|d |||ddddd}t|| | S)a Anderson-Darling test for data coming from a particular distribution. The Anderson-Darling test tests the null hypothesis that a sample is drawn from a population that follows a particular distribution. For the Anderson-Darling test, the critical values depend on which distribution is being tested against. This function works for normal, exponential, logistic, or Gumbel (Extreme Value Type I) distributions. Parameters ---------- x : array_like Array of sample data. dist : {'norm', 'expon', 'logistic', 'gumbel', 'gumbel_l', 'gumbel_r', 'extreme1'}, optional The type of distribution to test against. The default is 'norm'. The names 'extreme1', 'gumbel_l' and 'gumbel' are synonyms for the same distribution. Returns ------- statistic : float The Anderson-Darling test statistic. critical_values : list The critical values for this distribution. significance_level : list The significance levels for the corresponding critical values in percents. The function returns critical values for a differing set of significance levels depending on the distribution that is being tested against. See Also -------- kstest : The Kolmogorov-Smirnov test for goodness-of-fit. Notes ----- Critical values provided are for the following significance levels: normal/exponential 15%, 10%, 5%, 2.5%, 1% logistic 25%, 10%, 5%, 2.5%, 1%, 0.5% Gumbel 25%, 10%, 5%, 2.5%, 1% If the returned statistic is larger than these critical values then for the corresponding significance level, the null hypothesis that the data come from the chosen distribution can be rejected. The returned statistic is referred to as 'A2' in the references. References ---------- .. [1] https://www.itl.nist.gov/div898/handbook/prc/section2/prc213.htm .. [2] Stephens, M. A. (1974). EDF Statistics for Goodness of Fit and Some Comparisons, Journal of the American Statistical Association, Vol. 69, pp. 730-737. .. [3] Stephens, M. A. (1976). Asymptotic Results for Goodness-of-Fit Statistics with Unknown Parameters, Annals of Statistics, Vol. 4, pp. 357-369. .. [4] Stephens, M. A. (1977). Goodness of Fit for the Extreme Value Distribution, Biometrika, Vol. 64, pp. 583-588. .. [5] Stephens, M. A. (1977). Goodness of Fit with Special Reference to Tests for Exponentiality , Technical Report No. 262, Department of Statistics, Stanford University, Stanford, CA. .. [6] Stephens, M. A. (1979). Tests of Fit for the Logistic Distribution Based on the Empirical Distribution Function, Biometrika, Vol. 66, pp. 591-595. )rZexponZgumbelgumbel_lgumbel_rZextreme1logisticzWInvalid distribution; dist must be 'norm', 'expon', 'gumbel', 'extreme1' or 'logistic'.rrerZr)ddofrf) @rrg@g9@rhrg333333?rcSsd|\}}|||}t|}tjdd|ddd|tj|d|d|dd|g}t|S)Nrgrrrerx)rrlrpr)abZxjrtrrtmpZtmp2rcrQrQrRrSs  zanderson..rootfuncgh㈵>)rZxtol)rrrrrx?r)rrrrrg?rSNry)rIr rlrJrXZstdr$rZlogcdflogsfrr _Avals_normr _Avals_exponrZfsolver_Avals_logisticrr _Avals_gumbelrrr rpr)r]rrr_rtrPrrrsigcriticalrZsol0Zsolr{A2rQrQrRr3sVF    &                2r3cCsd}||d}||jkr d}n||d|}||d} td|D]} t|| } | j|dd} | t} | | |d}| |d8} |t||| | || d| || ||d }|||| 7}qF||d|9}|S) aCompute A2akN equation 7 of Scholz and Stephens. Parameters ---------- samples : sequence of 1-D array_like Array of sample arrays. Z : array_like Sorted array of all observations. Zstar : array_like Sorted array of unique observations. k : int Number of samples. n : array_like Number of observations in each sample. N : int Total number of observations. Returns ------- A2aKN : float The A2aKN statistics of Scholz and Stephens 1987. rleftrgrightrVrZsiderSr) searchsortedrnr rlr rrrp)samplesZZstarrur^rtZA2akNZZ_ssorted_leftljBjr{rPZs_ssorted_rightMijZfijinnerrQrQrR_anderson_ksamp_midrankws      <rc Csd}||ddd||ddd}|}td|D]l} t|| } | j|dddd} |t||| ||| d|||} || || 7}q>|S) aCompute A2akN equation 6 of Scholz & Stephens. Parameters ---------- samples : sequence of 1-D array_like Array of sample arrays. Z : array_like Sorted array of all observations. Zstar : array_like Sorted array of unique observations. k : int Number of samples. n : array_like Number of observations in each sample. N : int Total number of observations. Returns ------- A2KN : float The A2KN statistics of Scholz and Stephens 1987. rNryr r rr rS)r cumsumr rlr rrp) r rrrur^rtA2kNrrr{rPrrrQrQrR_anderson_ksamp_rights 0rAnderson_ksampResultcCst|}|dkrtdtttj|}tt|}|j}t |}|jdkrZtdt dd|D}t |dkrtd|rt ||||||}nt ||||||}d|}dt|d d d } | d d } | td|} d | d |d d d | |} d| d |dd| |d| d| d |d| d | d } d | d| d|dd | d | d |d| d |d | }d| d |dd | |}| |d| |d||||d|d|d}|d }||t|}t gd}t gd}t gd}||t|||}t gd}||kr|}tjd|ddnP||kr|}tjd|ddn$t|t|d}tt||}t|||S)aThe Anderson-Darling test for k-samples. The k-sample Anderson-Darling test is a modification of the one-sample Anderson-Darling test. It tests the null hypothesis that k-samples are drawn from the same population without having to specify the distribution function of that population. The critical values depend on the number of samples. Parameters ---------- samples : sequence of 1-D array_like Array of sample data in arrays. midrank : bool, optional Type of Anderson-Darling test which is computed. Default (True) is the midrank test applicable to continuous and discrete populations. If False, the right side empirical distribution is used. Returns ------- statistic : float Normalized k-sample Anderson-Darling test statistic. critical_values : array The critical values for significance levels 25%, 10%, 5%, 2.5%, 1%, 0.5%, 0.1%. significance_level : float An approximate significance level at which the null hypothesis for the provided samples can be rejected. The value is floored / capped at 0.1% / 25%. Raises ------ ValueError If less than 2 samples are provided, a sample is empty, or no distinct observations are in the samples. See Also -------- ks_2samp : 2 sample Kolmogorov-Smirnov test anderson : 1 sample Anderson-Darling test Notes ----- [1]_ defines three versions of the k-sample Anderson-Darling test: one for continuous distributions and two for discrete distributions, in which ties between samples may occur. The default of this routine is to compute the version based on the midrank empirical distribution function. This test is applicable to continuous and discrete data. If midrank is set to False, the right side empirical distribution is used for a test for discrete data. According to [1]_, the two discrete test statistics differ only slightly if a few collisions due to round-off errors occur in the test not adjusted for ties between samples. The critical values corresponding to the significance levels from 0.01 to 0.25 are taken from [1]_. p-values are floored / capped at 0.1% / 25%. Since the range of critical values might be extended in future releases, it is recommended not to test ``p == 0.25``, but rather ``p >= 0.25`` (analogously for the lower bound). .. versionadded:: 0.14.0 References ---------- .. [1] Scholz, F. W and Stephens, M. A. (1987), K-Sample Anderson-Darling Tests, Journal of the American Statistical Association, Vol. 82, pp. 918-924. Examples -------- >>> from scipy import stats >>> rng = np.random.default_rng() The null hypothesis that the two random samples come from the same distribution can be rejected at the 5% level because the returned test value is greater than the critical value for 5% (1.961) but not at the 2.5% level. The interpolation gives an approximate significance level of 3.2%: >>> stats.anderson_ksamp([rng.normal(size=50), ... rng.normal(loc=0.5, size=30)]) (1.974403288713695, array([0.325, 1.226, 1.961, 2.718, 3.752, 4.592, 6.546]), 0.04991293614572478) The null hypothesis cannot be rejected for three samples from an identical distribution. The reported p-value (25%) has been capped and may not be very accurate (since it corresponds to the value 0.449 whereas the statistic is -0.731): >>> stats.anderson_ksamp([rng.normal(size=50), ... rng.normal(size=30), rng.normal(size=20)]) (-0.29103725200789504, array([ 0.44925884, 1.3052767 , 1.9434184 , 2.57696569, 3.41634856, 4.07210043, 5.56419101]), 0.25) rSz)anderson_ksamp needs at least two samplesz7anderson_ksamp needs more than one distinct observationcSsg|] }|jqSrQ)rn).0samplerQrQrR ;z"anderson_ksamp..rz6anderson_ksamp encountered sample without observationsrgrryrdrrhrVrj)g?g"~?gRQ?g\(\?gS㥛@g/$@gGz@)g\(\ϿrgV-?gMb?gx&?gx@gQ @)gzGếgQӿg^I +׿g/$ٿgMbXٿgGzֿgʡEÿ)rr皙?g?rg{Gzt?gMbP?z)p-value capped: true value larger than {}) stacklevelz+p-value floored: true value smaller than {})rXrIlistmaprlr r Zhstackrnrrrrrrpr rr[rminmaxrrformatZpolyfitrrZpolyvalr)r Zmidrankrurrtrr^rHZhs_cshgrrcdZsigmasqrNrZb0b1b2rrppfrQrQrRr?sXd    $LL <  r? AnsariResultc@s8eZdZdZddZddZddZdd Zd d Zd S) _ABWzEDistribution of Ansari-Bradley W-statistic under the null hypothesis.cCs"d|_d|_d|_d|_d|_dS)zMinimal initializer.N)rNr^astarttotalfreqs)selfrQrQrR__init__ss z _ABW.__init__cCsX||jks||jkrT|||_|_t||\}}}||_|tj|_|j |_ dS)z/When necessary, recalculate exact distribution.N) r^rNrZgscaler2rrlrmr4rpr3)r5r^rNr2Za1rrQrQrR_recalc{s z _ABW._recalccCs2|||t||jt}|j||jS)zProbability mass function.)r7rlfloorr2rrkr4r3r5rur^rNindrQrQrRpmfs z_ABW.pmfcCs>|||t||jt}|jd|d|jS)z!Cumulative distribution function.Nr) r7rlceilr2rrkr4rpr3r9rQrQrRcdfs z_ABW.cdfcCs:|||t||jt}|j|d|jS)zSurvival function.N) r7rlr8r2rrkr4rpr3r9rQrQrRsfs z_ABW.sfN) __name__ __module__ __qualname____doc__r6r7r;r=r>rQrQrQrRr1ms r1 two-sidedc Cs|dvrtdt|t|}}t|}t|}|dkrBtd|dkrRtd||}t||f}t|}tt|||dfd}tj |d|dd} t |} t| t|k} |d ko|d ko| } | r|d ks|d krt d | rZ|d kr"d t t| ||t| ||} n(|d kr>> from scipy.stats import ansari >>> rng = np.random.default_rng() For these examples, we'll create three random data sets. The first two, with sizes 35 and 25, are drawn from a normal distribution with mean 0 and standard deviation 2. The third data set has size 25 and is drawn from a normal distribution with standard deviation 1.25. >>> x1 = rng.normal(loc=0, scale=2, size=35) >>> x2 = rng.normal(loc=0, scale=2, size=25) >>> x3 = rng.normal(loc=0, scale=1.25, size=25) First we apply `ansari` to `x1` and `x2`. These samples are drawn from the same distribution, so we expect the Ansari-Bradley test should not lead us to conclude that the scales of the distributions are different. >>> ansari(x1, x2) AnsariResult(statistic=541.0, pvalue=0.9762532927399098) With a p-value close to 1, we cannot conclude that there is a significant difference in the scales (as expected). Now apply the test to `x1` and `x3`: >>> ansari(x1, x3) AnsariResult(statistic=425.0, pvalue=0.0003087020407974518) The probability of observing such an extreme value of the statistic under the null hypothesis of equal scales is only 0.03087%. We take this as evidence against the null hypothesis in favor of the alternative: the scales of the distributions from which the samples were drawn are not equal. We can use the `alternative` parameter to perform a one-tailed test. In the above example, the scale of `x1` is greater than `x3` and so the ratio of scales of `x1` and `x3` is greater than 1. This means that the p-value when ``alternative='greater'`` should be near 0 and hence we should be able to reject the null hypothesis: >>> ansari(x1, x3, alternative='greater') AnsariResult(statistic=425.0, pvalue=0.0001543510203987259) As we can see, the p-value is indeed quite low. Use of ``alternative='less'`` should thus yield a large p-value: >>> ansari(x1, x3, alternative='less') AnsariResult(statistic=425.0, pvalue=0.9998643258449039) >rClessgreaterz8'alternative' must be 'two-sided', 'greater', or 'less'.rzNot enough other observations.zNot enough test observations.rNre7z%Ties preclude use of exact statistic.rCrVrErgrSrrhgH@0rdg0@)rIr rXrrrankdatar rrlrprrrminimum _abw_stater=r>r0r$rr")r]r alternativer^rNrtxyZrankZsymrankZABZuxyZrepeatsexactpvalZmnABZvarABrbrrQrQrRr4sRg       *$ 60r4BartlettResultc Gs^|D]>}t|jdkr*ttjtjSt|jdkrtdqt|}|dkr\tdt|}t|d}t |D]*}t||||<tj ||dd||<qztj |dd}tj |d|ddd ||}|d |t |tj |d t |dd}d d d |dtj d |d ddd ||} || } t j| |d} t| | S) a Perform Bartlett's test for equal variances. Bartlett's test tests the null hypothesis that all input samples are from populations with equal variances. For samples from significantly non-normal populations, Levene's test `levene` is more robust. Parameters ---------- sample1, sample2,... : array_like arrays of sample data. Only 1d arrays are accepted, they may have different lengths. Returns ------- statistic : float The test statistic. pvalue : float The p-value of the test. See Also -------- fligner : A non-parametric test for the equality of k variances levene : A robust parametric test for equality of k variances Notes ----- Conover et al. (1981) examine many of the existing parametric and nonparametric tests by extensive simulations and they conclude that the tests proposed by Fligner and Killeen (1976) and Levene (1960) appear to be superior in terms of robustness of departures from normality and power ([3]_). References ---------- .. [1] https://www.itl.nist.gov/div898/handbook/eda/section3/eda357.htm .. [2] Snedecor, George W. and Cochran, William G. (1989), Statistical Methods, Eighth Edition, Iowa State University Press. .. [3] Park, C. and Lindsay, B. G. (1999). Robust Scale Estimation and Hypothesis Testing based on Quadratic Inference Function. Technical Report #99-03, Center for Likelihood Studies, Pennsylvania State University. .. [4] Bartlett, M. S. (1937). Properties of Sufficiency and Statistical Tests. Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, Vol. 160, No.901, pp. 268-282. Examples -------- Test whether or not the lists `a`, `b` and `c` come from populations with equal variances. >>> from scipy.stats import bartlett >>> a = [8.88, 9.12, 9.04, 8.98, 9.00, 9.08, 9.01, 8.85, 9.06, 8.99] >>> b = [8.88, 8.95, 9.29, 9.44, 9.15, 9.58, 8.36, 9.18, 8.67, 9.05] >>> c = [8.95, 9.12, 8.95, 8.85, 9.03, 8.84, 9.07, 8.98, 8.86, 8.98] >>> stat, p = bartlett(a, b, c) >>> p 1.1254782518834628e-05 The very small p-value suggests that the populations do not have equal variances. This is not surprising, given that the sample variance of `b` is much larger than that of `a` and `c`: >>> [np.var(x, ddof=1) for x in [a, b, c]] [0.007054444444444413, 0.13073888888888888, 0.008890000000000002] rr Samples must be one-dimensional.rS-Must enter at least two input sample vectors.r+)rrergrh)rl asanyarrayrnrPrqrrIrXrzrrrYrprr$rr>) rrruNiZssqjNtotZspsqnumerdenomTrOrQrQrRr5I s,J    ".$ r5 LeveneResultmedianr )centerproportiontocutcs|dvrtdt|}|dkr(tdt|D] }t||jdkr0tdq0t|}t|d}|dkrzd d }n0|d krd d }ntfd d|D}dd }t|D]$}t||||<|||||<qtj|dd}dg|} t|D] } t t || || | | <qt|d} d} t|D]0} tj | | dd| | <| | | || 7} q2| |} ||tj|| | ddd} d}t|D](} |tj| | | | ddd7}q|d|}| |}t j ||d||}t||S)a Perform Levene test for equal variances. The Levene test tests the null hypothesis that all input samples are from populations with equal variances. Levene's test is an alternative to Bartlett's test `bartlett` in the case where there are significant deviations from normality. Parameters ---------- sample1, sample2, ... : array_like The sample data, possibly with different lengths. Only one-dimensional samples are accepted. center : {'mean', 'median', 'trimmed'}, optional Which function of the data to use in the test. The default is 'median'. proportiontocut : float, optional When `center` is 'trimmed', this gives the proportion of data points to cut from each end. (See `scipy.stats.trim_mean`.) Default is 0.05. Returns ------- statistic : float The test statistic. pvalue : float The p-value for the test. Notes ----- Three variations of Levene's test are possible. The possibilities and their recommended usages are: * 'median' : Recommended for skewed (non-normal) distributions> * 'mean' : Recommended for symmetric, moderate-tailed distributions. * 'trimmed' : Recommended for heavy-tailed distributions. The test version using the mean was proposed in the original article of Levene ([2]_) while the median and trimmed mean have been studied by Brown and Forsythe ([3]_), sometimes also referred to as Brown-Forsythe test. References ---------- .. [1] https://www.itl.nist.gov/div898/handbook/eda/section3/eda35a.htm .. [2] Levene, H. (1960). In Contributions to Probability and Statistics: Essays in Honor of Harold Hotelling, I. Olkin et al. eds., Stanford University Press, pp. 278-292. .. [3] Brown, M. B. and Forsythe, A. B. (1974), Journal of the American Statistical Association, 69, 364-367 Examples -------- Test whether or not the lists `a`, `b` and `c` come from populations with equal variances. >>> from scipy.stats import levene >>> a = [8.88, 9.12, 9.04, 8.98, 9.00, 9.08, 9.01, 8.85, 9.06, 8.99] >>> b = [8.88, 8.95, 9.29, 9.44, 9.15, 9.58, 8.36, 9.18, 8.67, 9.05] >>> c = [8.95, 9.12, 8.95, 8.85, 9.03, 8.84, 9.07, 8.98, 8.86, 8.98] >>> stat, p = levene(a, b, c) >>> p 0.002431505967249681 The small p-value suggests that the populations do not have equal variances. This is not surprising, given that the sample variance of `b` is much larger than that of `a` and `c`: >>> [np.var(x, ddof=1) for x in [a, b, c]] [0.007054444444444413, 0.13073888888888888, 0.008890000000000002] rJr[Ztrimmed-center must be 'mean', 'median' or 'trimmed'.rSrRrrQr+r[cSstj|ddSNrrerlr[rrQrQrR rzlevene..rJcSstj|ddSr`rlrJrrQrQrRrb rc3s |]}tt|VqdSr)rtrimbothrlr rargr]rQrR szlevene..cSstj|ddSr`rcrrQrQrRrb rrreNrrg)rIrXrrrlrSrrzrrprr rJr$rr>rZ)r\r]rrurUrTYcirrVZijr{ZZbariZZbarrWZdvarrXWrOrQrgrRr6 sNJ            " & r6rxc Cst|tj}t|dkr6|d|d}|d}n@t|dkrn|d}|dusZ||krbtdt|}ntd|dks|dkrtd |d vrtd |d krtj|||}|S|d krtj |d||}|Stj |||}d}|||krd}n|||krrt t |||d}tj tj |||||kdd}tj|||tj ||||}nbt t||d}tj tj |||||kdd}tj|d||tj |d||}td|S)aPerform a test that the probability of success is p. Note: `binom_test` is deprecated; it is recommended that `binomtest` be used instead. This is an exact, two-sided test of the null hypothesis that the probability of success in a Bernoulli experiment is `p`. Parameters ---------- x : int or array_like The number of successes, or if x has length 2, it is the number of successes and the number of failures. n : int The number of trials. This is ignored if x gives both the number of successes and failures. p : float, optional The hypothesized probability of success. ``0 <= p <= 1``. The default value is ``p = 0.5``. alternative : {'two-sided', 'greater', 'less'}, optional Indicates the alternative hypothesis. The default value is 'two-sided'. Returns ------- p-value : float The p-value of the hypothesis test. References ---------- .. [1] https://en.wikipedia.org/wiki/Binomial_test Examples -------- >>> from scipy import stats A car manufacturer claims that no more than 10% of their cars are unsafe. 15 cars are inspected for safety, 3 were found to be unsafe. Test the manufacturer's claim: >>> stats.binom_test(3, n=15, p=0.1, alternative='greater') 0.18406106910639114 The null hypothesis cannot be rejected at the 5% level of significance because the returned p-value is greater than the critical value of 5%. rSrrNzn must be >= xzIncorrect length for x.rgrzp must be in range [0,1]rCrDrEzEalternative not recognized should be 'two-sided', 'less' or 'greater'rDrEg?re)rrrlint_rXrIr$Zbinomr=r>r;r r<rpr8r$) r]r^r.rLrOr+Zrerrr{rrQrQrRr70 sH1    ""r7cs@ttdtffddttdD}t|S)Nrcs(g|] }||dqS)rrQ)rrurr)r]rQrRr rz_apply_func..r)rrrXrrr )r]r)routputrQrnrR _apply_func s"rp FlignerResultcs|dvrtdD]&}t|jdkrttjtjSqt}|dkrTtd|dkrfddn0|d krxd dntfd d Dd dtfddt |D}tfddt |Dtj |dd}fddt |D}g}dg} t |D]&} | t || | t|qt|} tj| d|dd}t|| tj |} tj|dd} tj|ddd}tj |t| | ddd|}tj||d}t||S)ad Perform Fligner-Killeen test for equality of variance. Fligner's test tests the null hypothesis that all input samples are from populations with equal variances. Fligner-Killeen's test is distribution free when populations are identical [2]_. Parameters ---------- sample1, sample2, ... : array_like Arrays of sample data. Need not be the same length. center : {'mean', 'median', 'trimmed'}, optional Keyword argument controlling which function of the data is used in computing the test statistic. The default is 'median'. proportiontocut : float, optional When `center` is 'trimmed', this gives the proportion of data points to cut from each end. (See `scipy.stats.trim_mean`.) Default is 0.05. Returns ------- statistic : float The test statistic. pvalue : float The p-value for the hypothesis test. See Also -------- bartlett : A parametric test for equality of k variances in normal samples levene : A robust parametric test for equality of k variances Notes ----- As with Levene's test there are three variants of Fligner's test that differ by the measure of central tendency used in the test. See `levene` for more information. Conover et al. (1981) examine many of the existing parametric and nonparametric tests by extensive simulations and they conclude that the tests proposed by Fligner and Killeen (1976) and Levene (1960) appear to be superior in terms of robustness of departures from normality and power [3]_. References ---------- .. [1] Park, C. and Lindsay, B. G. (1999). Robust Scale Estimation and Hypothesis Testing based on Quadratic Inference Function. Technical Report #99-03, Center for Likelihood Studies, Pennsylvania State University. https://cecas.clemson.edu/~cspark/cv/paper/qif/draftqif2.pdf .. [2] Fligner, M.A. and Killeen, T.J. (1976). Distribution-free two-sample tests for scale. 'Journal of the American Statistical Association.' 71(353), 210-213. .. [3] Park, C. and Lindsay, B. G. (1999). Robust Scale Estimation and Hypothesis Testing based on Quadratic Inference Function. Technical Report #99-03, Center for Likelihood Studies, Pennsylvania State University. .. [4] Conover, W. J., Johnson, M. E. and Johnson M. M. (1981). A comparative study of tests for homogeneity of variances, with applications to the outer continental shelf biding data. Technometrics, 23(4), 351-361. Examples -------- Test whether or not the lists `a`, `b` and `c` come from populations with equal variances. >>> from scipy.stats import fligner >>> a = [8.88, 9.12, 9.04, 8.98, 9.00, 9.08, 9.01, 8.85, 9.06, 8.99] >>> b = [8.88, 8.95, 9.29, 9.44, 9.15, 9.58, 8.36, 9.18, 8.67, 9.05] >>> c = [8.95, 9.12, 8.95, 8.85, 9.03, 8.84, 9.07, 8.98, 8.86, 8.98] >>> stat, p = fligner(a, b, c) >>> p 0.00450826080004775 The small p-value suggests that the populations do not have equal variances. This is not surprising, given that the sample variance of `b` is much larger than that of `a` and `c`: >>> [np.var(x, ddof=1) for x in [a, b, c]] [0.007054444444444413, 0.13073888888888888, 0.008890000000000002] r^r_rrSrRr[cSstj|ddSr`rarrQrQrRrb rzfligner..rJcSstj|ddSr`rcrrQrQrRrb rc3s|]}t|VqdSr)rrdrergrQrRrh rzfligner..cSstj|ddSr`rcrrQrQrRrb rcsg|]}t|qSrQ)rXrrUrrQrRr rzfligner..csg|]}|qSrQrQrrrrQrRr rrecs$g|]}tt||qSrQ)rr )rr{)rirrQrRr rrgrxr)rfrrV)rIrlrSrnrqrqrXrr rrrpextendr"appendrrIr$rZrrprJrYrr>)r\r]rrrurTrVrjZallZijr)r{ZranksZAibarZanbarZvarsqZXsqrOrQ)rirrr]rRr8 s>W    "r8cstjtdtjtddur8ddkrJjtfddttjD}|tfddttjDkst dj}j}||}|dkrt d tj fd }dkrt |}| |jdd }t |} t|jd D](} t|dd| f| dd| f<q| d|} tj| |d dddd } |||d d} |||d |d|dd}| | t|}t||\}}|dkr|d}|d}n ||_||_||fS)a Perform Mood's test for equal scale parameters. Mood's two-sample test for scale parameters is a non-parametric test for the null hypothesis that two samples are drawn from the same distribution with the same scale parameter. Parameters ---------- x, y : array_like Arrays of sample data. axis : int, optional The axis along which the samples are tested. `x` and `y` can be of different length along `axis`. If `axis` is None, `x` and `y` are flattened and the test is done on all values in the flattened arrays. alternative : {'two-sided', 'less', 'greater'}, optional Defines the alternative hypothesis. Default is 'two-sided'. The following options are available: * 'two-sided': the scales of the distributions underlying `x` and `y` are different. * 'less': the scale of the distribution underlying `x` is less than the scale of the distribution underlying `y`. * 'greater': the scale of the distribution underlying `x` is greater than the scale of the distribution underlying `y`. .. versionadded:: 1.7.0 Returns ------- z : scalar or ndarray The z-score for the hypothesis test. For 1-D inputs a scalar is returned. p-value : scalar ndarray The p-value for the hypothesis test. See Also -------- fligner : A non-parametric test for the equality of k variances ansari : A non-parametric test for the equality of 2 variances bartlett : A parametric test for equality of k variances in normal samples levene : A parametric test for equality of k variances Notes ----- The data are assumed to be drawn from probability distributions ``f(x)`` and ``f(x/s) / s`` respectively, for some probability density function f. The null hypothesis is that ``s == 1``. For multi-dimensional arrays, if the inputs are of shapes ``(n0, n1, n2, n3)`` and ``(n0, m1, n2, n3)``, then if ``axis=1``, the resulting z and p values will have shape ``(n0, n2, n3)``. Note that ``n1`` and ``m1`` don't have to be equal, but the other dimensions do. Examples -------- >>> from scipy import stats >>> rng = np.random.default_rng() >>> x2 = rng.standard_normal((2, 45, 6, 7)) >>> x1 = rng.standard_normal((2, 30, 6, 7)) >>> z, p = stats.mood(x1, x2, axis=1) >>> p.shape (2, 6, 7) Find the number of points where the difference in scale is not significant: >>> (p > 0.1).sum() 78 Perform the test with different scales: >>> x1 = rng.standard_normal((2, 30)) >>> x2 = rng.standard_normal((2, 35)) * 10.0 >>> stats.mood(x1, x2, axis=1) (array([-5.76174136, -6.12650783]), array([8.32505043e-09, 8.98287869e-10])) rvNrcsg|]}|krj|qSrQrrax)rfr]rQrRry rzmood..csg|]}|krj|qSrQrurv)rfrrQrRrz sz 20 ([2]_, p. 383). References ---------- .. [1] https://en.wikipedia.org/wiki/Wilcoxon_signed-rank_test .. [2] Conover, W.J., Practical Nonparametric Statistics, 1971. .. [3] Pratt, J.W., Remarks on Zeros and Ties in the Wilcoxon Signed Rank Procedures, Journal of the American Statistical Association, Vol. 54, 1959, pp. 655-667. :doi:`10.1080/01621459.1959.10501526` .. [4] Wilcoxon, F., Individual Comparisons by Ranking Methods, Biometrics Bulletin, Vol. 1, 1945, pp. 80-83. :doi:`10.2307/3001968` .. [5] Cureton, E.E., The Normal Approximation to the Signed-Rank Sampling Distribution When Zero Differences are Present, Journal of the American Statistical Association, Vol. 62, 1967, pp. 1068-1069. :doi:`10.1080/01621459.1967.10500917` Examples -------- In [4]_, the differences in height between cross- and self-fertilized corn plants is given as follows: >>> d = [6, 8, 14, 16, 23, 24, 28, 29, 41, -48, 49, 56, 60, -67, 75] Cross-fertilized plants appear to be be higher. To test the null hypothesis that there is no height difference, we can apply the two-sided test: >>> from scipy.stats import wilcoxon >>> w, p = wilcoxon(d) >>> w, p (24.0, 0.041259765625) Hence, we would reject the null hypothesis at a confidence level of 5%, concluding that there is a difference in height between the groups. To confirm that the median of the differences can be assumed to be positive, we use: >>> w, p = wilcoxon(d, alternative='greater') >>> w, p (96.0, 0.0206298828125) This shows that the null hypothesis that the median is negative can be rejected at a confidence level of 5% in favor of the alternative that the median is greater than zero. The p-values above are exact. Using the normal approximation gives very similar values: >>> w, p = wilcoxon(d, mode='approx') >>> w, p (24.0, 0.04088813291185591) Note that the statistic changed to 96 in the one-sided case (the sum of ranks of positive differences) whereas it is 24 in the two-sided case (the minimum of sum of ranks above and below zero). )r~approxrNz/mode must be either 'auto', 'approx' or 'exact')r}prattzsplitz:Zero method must be either 'wilcox' or 'pratt' or 'zsplit'rlz;Alternative must be either 'two-sided', 'greater' or 'less'Nrz!Sample x must be one-dimensional.z(Samples x and y must be one-dimensional.z.The samples x and y must have the same length.r~rrNrrz]Exact p-value calculation does not work if there are ties. Switching to normal approximation.)r}rzOzero_method 'wilcox' and 'pratt' do not work if x - y is zero for all elements.r}rz/Sample size too small for normal approximation.rrVrCrgrrrxrDgrErS)rIr rr#rXrlrprrr not_equalrrIrr$r rnrrr$rZr>r=r&rkr|)r]rZ zero_method correctionrLmoder+Zn_zerocountrZr_plusZr_minusZr_zerorYmnseZreplistZrepnumrrZcntZp_lessZ p_greaterrQrQrRr: s}                         r:below propagate)tiesrlambda_ nan_policycGsnt|dkrtdgd}||vr@td|t|ddfdd|D}t|D]B\}}|jd krxtd |d|jdkrVtd |d|jfqVt|} t| |\} }| r|d krtj tj tj d fS| rt | t | } n t | } tj dt|ftj d} t|D]\}} | t | } t| | k}t| | k}| j||}| d |f|7<| d|f|7<|dkr| d|f|7<n|dkr| d |f|7<q| jdd}|d d krtd| |dd krtd| |dkrLt| d kjd dd }t|d krLd|d d| f}t|t| ||d\}}}}||| | fS)alPerform a Mood's median test. Test that two or more samples come from populations with the same median. Let ``n = len(args)`` be the number of samples. The "grand median" of all the data is computed, and a contingency table is formed by classifying the values in each sample as being above or below the grand median. The contingency table, along with `correction` and `lambda_`, are passed to `scipy.stats.chi2_contingency` to compute the test statistic and p-value. Parameters ---------- sample1, sample2, ... : array_like The set of samples. There must be at least two samples. Each sample must be a one-dimensional sequence containing at least one value. The samples are not required to have the same length. ties : str, optional Determines how values equal to the grand median are classified in the contingency table. The string must be one of:: "below": Values equal to the grand median are counted as "below". "above": Values equal to the grand median are counted as "above". "ignore": Values equal to the grand median are not counted. The default is "below". correction : bool, optional If True, *and* there are just two samples, apply Yates' correction for continuity when computing the test statistic associated with the contingency table. Default is True. lambda_ : float or str, optional By default, the statistic computed in this test is Pearson's chi-squared statistic. `lambda_` allows a statistic from the Cressie-Read power divergence family to be used instead. See `power_divergence` for details. Default is 1 (Pearson's chi-squared statistic). nan_policy : {'propagate', 'raise', 'omit'}, optional Defines how to handle when input contains nan. 'propagate' returns nan, 'raise' throws an error, 'omit' performs the calculations ignoring nan values. Default is 'propagate'. Returns ------- stat : float The test statistic. The statistic that is returned is determined by `lambda_`. The default is Pearson's chi-squared statistic. p : float The p-value of the test. m : float The grand median. table : ndarray The contingency table. The shape of the table is (2, n), where n is the number of samples. The first row holds the counts of the values above the grand median, and the second row holds the counts of the values below the grand median. The table allows further analysis with, for example, `scipy.stats.chi2_contingency`, or with `scipy.stats.fisher_exact` if there are two samples, without having to recompute the table. If ``nan_policy`` is "propagate" and there are nans in the input, the return value for ``table`` is ``None``. See Also -------- kruskal : Compute the Kruskal-Wallis H-test for independent samples. mannwhitneyu : Computes the Mann-Whitney rank test on samples x and y. Notes ----- .. versionadded:: 0.15.0 References ---------- .. [1] Mood, A. M., Introduction to the Theory of Statistics. McGraw-Hill (1950), pp. 394-399. .. [2] Zar, J. H., Biostatistical Analysis, 5th ed. Prentice Hall (2010). See Sections 8.12 and 10.15. Examples -------- A biologist runs an experiment in which there are three groups of plants. Group 1 has 16 plants, group 2 has 15 plants, and group 3 has 17 plants. Each plant produces a number of seeds. The seed counts for each group are:: Group 1: 10 14 14 18 20 22 24 25 31 31 32 39 43 43 48 49 Group 2: 28 30 31 33 34 35 36 40 44 55 57 61 91 92 99 Group 3: 0 3 9 22 23 25 25 33 34 34 40 45 46 48 62 67 84 The following code applies Mood's median test to these samples. >>> g1 = [10, 14, 14, 18, 20, 22, 24, 25, 31, 31, 32, 39, 43, 43, 48, 49] >>> g2 = [28, 30, 31, 33, 34, 35, 36, 40, 44, 55, 57, 61, 91, 92, 99] >>> g3 = [0, 3, 9, 22, 23, 25, 25, 33, 34, 34, 40, 45, 46, 48, 62, 67, 84] >>> from scipy.stats import median_test >>> stat, p, med, tbl = median_test(g1, g2, g3) The median is >>> med 34.0 and the contingency table is >>> tbl array([[ 5, 10, 7], [11, 5, 10]]) `p` is too large to conclude that the medians are not the same: >>> p 0.12609082774093244 The "G-test" can be performed by passing ``lambda_="log-likelihood"`` to `median_test`. >>> g, p, med, tbl = median_test(g1, g2, g3, lambda_="log-likelihood") >>> p 0.12224779737117837 The median occurs several times in the data, so we'll get a different result if, for example, ``ties="above"`` is used: >>> stat, p, med, tbl = median_test(g1, g2, g3, ties="above") >>> p 0.063873276069553273 >>> tbl array([[ 5, 11, 9], [11, 4, 8]]) This example demonstrates that if the data set is not large and there are values equal to the median, the p-value can be sensitive to the choice of `ties`. rSz)median_test requires two or more samples.)raboveignorez5invalid 'ties' option '%s'; 'ties' must be one of: %srrycSsg|]}t|qSrQ)rlr rerQrQrRr7 rzmedian_test..rz@Sample %d is empty. All samples must contain at least one value.zLSample %d has %d dimensions. All samples must be one-dimensional sequences.rNrvrrrez+All values are below the grand median (%r).z+All values are above the grand median (%r).rznAll values in sample %d are equal to the grand median (%r), so they are ignored, resulting in an empty sample.)rr)rXrIr~rrnrrlrzr!rqr[ror Zint64rrpZnonzerorr#)rrrrrZ ties_optionsrLrur+cdata contains_nanZ grand_mediantablerZnaboveZnbelowZnequalZrowsumsZ zero_colsrstatr.ZdofexpectedrQrQrRr; sr             r;cCst|}|jdkr2tjttjttjdfSt||dt||}t||dt||}t||\}}|r|dkrt|}d||<d||<nd}||||fS)NrrVZomitr) rlr rnrqrrrr!ro)r highlowrsin_sampcos_samprmaskrQrQrR_circfuncs_commonz s     rcCst||||d\}}}}|j|d}|j|d} t|| } t| } | jdkr^| | dk} n| dk} | jdkr| | | <| | dt7<n| r| dt7} |dur|rtj| j tj d} n8|durdn|} |j | |j|dk}| rtj | |<| ||dt|S)aCompute the circular mean for samples in a range. Parameters ---------- samples : array_like Input array. high : float or int, optional High boundary for circular mean range. Default is ``2*pi``. low : float or int, optional Low boundary for circular mean range. Default is 0. axis : int, optional Axis along which means are computed. The default is to compute the mean of the flattened array. nan_policy : {'propagate', 'raise', 'omit'}, optional Defines how to handle when input contains nan. 'propagate' returns nan, 'raise' throws an error, 'omit' performs the calculations ignoring nan values. Default is 'propagate'. Returns ------- circmean : float Circular mean. Examples -------- >>> from scipy.stats import circmean >>> circmean([0.1, 2*np.pi+0.2, 6*np.pi+0.3]) 0.2 >>> from scipy.stats import circmean >>> circmean([0.2, 1.4, 2.6], high = 1, low = 0) 0.4 rrerrSN)rZ fill_valuerV) rrprrlrorrrfullrrqr)r rrrfrrrZnmaskZsin_sumZcos_sumrZmask_nanrZnshapeZsmaskrQrQrRr< s.#        r<c Cst||||d\}}}}|dur:|j|d}|j|d} nJttj||dt} tj| | dk<|j|d| }|j|d| } tjdd"t dt || } Wdn1s0Y||dt d d t | S) aZCompute the circular variance for samples assumed to be in a range. Parameters ---------- samples : array_like Input array. high : float or int, optional High boundary for circular variance range. Default is ``2*pi``. low : float or int, optional Low boundary for circular variance range. Default is 0. axis : int, optional Axis along which variances are computed. The default is to compute the variance of the flattened array. nan_policy : {'propagate', 'raise', 'omit'}, optional Defines how to handle when input contains nan. 'propagate' returns nan, 'raise' throws an error, 'omit' performs the calculations ignoring nan values. Default is 'propagate'. Returns ------- circvar : float Circular variance. Notes ----- This uses a definition of circular variance that in the limit of small angles returns a number close to the 'linear' variance. Examples -------- >>> from scipy.stats import circvar >>> circvar([0, 2*np.pi/3, 5*np.pi/3]) 2.19722457734 rNrerrinvalidrrVrSrW) rrJrlr rprrrqerrstaterJrrr r rrrfrrrrZsin_meanZcos_meanZnsumRrQrQrRr= s$ 0r=c Cst||||d\}}}}|dur:|j|d}|j|d} nJttj||dt} tj| | dk<|j|d| }|j|d| } tjdd"t dt || } Wdn1s0Y||dt t d t | S) a Compute the circular standard deviation for samples assumed to be in the range [low to high]. Parameters ---------- samples : array_like Input array. high : float or int, optional High boundary for circular standard deviation range. Default is ``2*pi``. low : float or int, optional Low boundary for circular standard deviation range. Default is 0. axis : int, optional Axis along which standard deviations are computed. The default is to compute the standard deviation of the flattened array. nan_policy : {'propagate', 'raise', 'omit'}, optional Defines how to handle when input contains nan. 'propagate' returns nan, 'raise' throws an error, 'omit' performs the calculations ignoring nan values. Default is 'propagate'. Returns ------- circstd : float Circular standard deviation. Notes ----- This uses a definition of circular standard deviation that in the limit of small angles returns a number close to the 'linear' standard deviation. Examples -------- >>> from scipy.stats import circstd >>> circstd([0, 0.1*np.pi/2, 0.001*np.pi, 0.03*np.pi/2]) 0.063564063306 rNrerrrrrVrW)rrJrlr rprrrqrrJrrrrrrQrQrRr> s' 0r>)rH)rS)rS)T)rQrZTNF)rr)rNr)NNN)NrN)Nr)Nr)N)r)Nr)rZ)T)rC)NrxrC)rrC)Nr}FrCr~)r)h __future__rr[r collectionsrZnumpyrlrrrrrr r r r r rrrrrrrrrrrrrZscipyrrrrr r!r"Z contingencyr#r$Z_distn_infrastructurer%Z _hypotestsr&__all__rDrFrGr(r'r)r*r|rrr+r,r-r.rr/r0rr1rArr@rBrCrr2rrrrrr3rrrr?r0r1rKr4rPr5rZr6r7rprqr8r9r|r:r;rr<r=r>rQrQrQrRs  d            cK ` 3>   W fb#  ( ' D [_ 5 F O      +$  7  c  `    } W D5