Source code for pybaselines.polynomial

# -*- coding: utf-8 -*-
"""Polynomial techniques for fitting baselines to experimental data.

Created on Feb. 27, 2021
@author: Donald Erb


The function penalized_poly was adapted from MATLAB code from
https://www.mathworks.com/matlabcentral/fileexchange/27429-background-correction
(accessed March 18, 2021), which was licensed under the BSD-2-clause below.

License: 2-clause BSD

Copyright (c) 2012, Vincent Mazet
All rights reserved.

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modification, are permitted provided that the following conditions are
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      notice, this list of conditions and the following disclaimer.
    * Redistributions in binary form must reproduce the above copyright
      notice, this list of conditions and the following disclaimer in
      the documentation and/or other materials provided with the distribution

THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS"
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The function loess was adapted from code from https://gist.github.com/agramfort/850437
(accessed March 25, 2021), which was licensed under the BSD-3-clause below.

# Authors: Alexandre Gramfort <alexandre.gramfort@telecom-paristech.fr>
#
# License: BSD (3-clause)
Copyright (c) 2015, Alexandre Gramfort
All rights reserved.

Redistribution and use in source and binary forms, with or without
modification, are permitted provided that the following conditions are met:

1. Redistributions of source code must retain the above copyright notice, this
   list of conditions and the following disclaimer.

2. Redistributions in binary form must reproduce the above copyright notice,
   this list of conditions and the following disclaimer in the documentation
   and/or other materials provided with the distribution.

3. Neither the name of the copyright holder nor the names of its
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   this software without specific prior written permission.

THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS "AS IS"
AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE
IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE
DISCLAIMED. IN NO EVENT SHALL THE COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE
FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL
DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR
SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY,
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"""

from math import ceil
import warnings

import numpy as np

from . import _weighting
from ._algorithm_setup import _Algorithm, _class_wrapper
from ._compat import _HAS_NUMBA, jit
from .utils import _MIN_FLOAT, ParameterWarning, _convert_coef, _interp_inplace, relative_difference


class _Polynomial(_Algorithm):
    """A base class for all polynomial algorithms."""

[docs] @_Algorithm._register(sort_keys=('weights',)) def poly(self, data, poly_order=2, weights=None, return_coef=False): """ Computes a polynomial that fits the baseline of the data. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'coef': numpy.ndarray, shape (poly_order,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Notes ----- To only fit regions without peaks, supply a weight array with zero values at the indices where peaks are located. """ y, weight_array, pseudo_inverse = self._setup_polynomial( data, weights, poly_order, calc_vander=True, calc_pinv=True ) sqrt_w = np.sqrt(weight_array) coef = pseudo_inverse @ (sqrt_w * y) baseline = self._polynomial.vandermonde @ coef params = {'weights': weight_array} if return_coef: params['coef'] = _convert_coef(coef, self.x_domain) return baseline, params
[docs] @_Algorithm._register(sort_keys=('weights',)) def modpoly(self, data, poly_order=2, tol=1e-3, max_iter=250, weights=None, use_original=False, mask_initial_peaks=False, return_coef=False): """ The modified polynomial (ModPoly) baseline algorithm. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. x_data : array-like, shape (N,), optional The x-values of the measured data. Default is None, which will create an array from -1 to 1 with N points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. tol : float, optional The exit criteria. Default is 1e-3. max_iter : int, optional The maximum number of iterations. Default is 250. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. use_original : bool, optional If False (default), will compare the baseline of each iteration with the y-values of that iteration [1]_ when choosing minimum values. If True, will compare the baseline with the original y-values given by `data` [2]_. mask_initial_peaks : bool, optional If True, will mask any data where the initial baseline fit + the standard deviation of the residual is less than measured data [3]_. Default is False. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Notes ----- Algorithm originally developed in [2]_ and then slightly modified in [1]_. References ---------- .. [1] Gan, F., et al. Baseline correction by improved iterative polynomial fitting with automatic threshold. Chemometrics and Intelligent Laboratory Systems, 2006, 82, 59-65. .. [2] Lieber, C., et al. Automated method for subtraction of fluorescence from biological raman spectra. Applied Spectroscopy, 2003, 57(11), 1363-1367. .. [3] Zhao, J., et al. Automated Autofluorescence Background Subtraction Algorithm for Biomedical Raman Spectroscopy, Applied Spectroscopy, 2007, 61(11), 1225-1232. """ y, weight_array, pseudo_inverse = self._setup_polynomial( data, weights, poly_order, calc_vander=True, calc_pinv=True, copy_weights=True ) sqrt_w = np.sqrt(weight_array) if use_original: y0 = y coef = pseudo_inverse @ (sqrt_w * y) baseline = self._polynomial.vandermonde @ coef if mask_initial_peaks: # use baseline + deviation since without deviation, half of y should be above baseline weight_array[baseline + np.std(y - baseline) < y] = 0 sqrt_w = np.sqrt(weight_array) pseudo_inverse = np.linalg.pinv(sqrt_w[:, None] * self._polynomial.vandermonde) tol_history = np.empty(max_iter) for i in range(max_iter): baseline_old = baseline y = np.minimum(y0 if use_original else y, baseline) coef = pseudo_inverse @ (sqrt_w * y) baseline = self._polynomial.vandermonde @ coef calc_difference = relative_difference(baseline_old, baseline) tol_history[i] = calc_difference if calc_difference < tol: break params = {'weights': weight_array, 'tol_history': tol_history[:i + 1]} if return_coef: params['coef'] = _convert_coef(coef, self.x_domain) return baseline, params
[docs] @_Algorithm._register(sort_keys=('weights',)) def imodpoly(self, data, poly_order=2, tol=1e-3, max_iter=250, weights=None, use_original=False, mask_initial_peaks=True, return_coef=False, num_std=1.): """ The improved modofied polynomial (IModPoly) baseline algorithm. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. tol : float, optional The exit criteria. Default is 1e-3. max_iter : int, optional The maximum number of iterations. Default is 250. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. use_original : bool, optional If False (default), will compare the baseline of each iteration with the y-values of that iteration [1]_ when choosing minimum values. If True, will compare the baseline with the original y-values given by `data` [2]_. mask_initial_peaks : bool, optional If True (default), will mask any data where the initial baseline fit + the standard deviation of the residual is less than measured data [3]_. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. num_std : float, optional The number of standard deviations to include when thresholding. Default is 1. Must be greater or equal to 0. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Raises ------ ValueError Raised if `num_std` is less than 0. Notes ----- Algorithm originally developed in [3]_. References ---------- .. [1] Gan, F., et al. Baseline correction by improved iterative polynomial fitting with automatic threshold. Chemometrics and Intelligent Laboratory Systems, 2006, 82, 59-65. .. [2] Lieber, C., et al. Automated method for subtraction of fluorescence from biological raman spectra. Applied Spectroscopy, 2003, 57(11), 1363-1367. .. [3] Zhao, J., et al. Automated Autofluorescence Background Subtraction Algorithm for Biomedical Raman Spectroscopy, Applied Spectroscopy, 2007, 61(11), 1225-1232. """ if num_std < 0: raise ValueError('num_std must be greater than or equal to 0') y, weight_array, pseudo_inverse = self._setup_polynomial( data, weights, poly_order, calc_vander=True, calc_pinv=True, copy_weights=True ) sqrt_w = np.sqrt(weight_array) if use_original: y0 = y coef = pseudo_inverse @ (sqrt_w * y) baseline = self._polynomial.vandermonde @ coef deviation = np.std(y - baseline) if mask_initial_peaks: weight_array[baseline + deviation < y] = 0 sqrt_w = np.sqrt(weight_array) pseudo_inverse = np.linalg.pinv(sqrt_w[:, None] * self._polynomial.vandermonde) tol_history = np.empty(max_iter) for i in range(max_iter): y = np.minimum(y0 if use_original else y, baseline + num_std * deviation) coef = pseudo_inverse @ (sqrt_w * y) baseline = self._polynomial.vandermonde @ coef new_deviation = np.std(y - baseline) # use new_deviation as dividing term in relative difference calc_difference = relative_difference(new_deviation, deviation) tol_history[i] = calc_difference if calc_difference < tol: break deviation = new_deviation params = {'weights': weight_array, 'tol_history': tol_history[:i + 1]} if return_coef: params['coef'] = _convert_coef(coef, self.x_domain) return baseline, params
# adapted from # https://www.mathworks.com/matlabcentral/fileexchange/27429-background-correction; # see license above
[docs] @_Algorithm._register(sort_keys=('weights',)) def penalized_poly(self, data, poly_order=2, tol=1e-3, max_iter=250, weights=None, cost_function='asymmetric_truncated_quadratic', threshold=None, alpha_factor=0.99, return_coef=False): """ Fits a polynomial baseline using a non-quadratic cost function. The non-quadratic cost functions penalize residuals with larger values, giving a more robust fit compared to normal least-squares. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. tol : float, optional The exit criteria. Default is 1e-3. max_iter : int, optional The maximum number of iterations. Default is 250. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. cost_function : str, optional The non-quadratic cost function to minimize. Must indicate symmetry of the method by appending 'a' or 'asymmetric' for asymmetric loss, and 's' or 'symmetric' for symmetric loss. Default is 'asymmetric_truncated_quadratic'. Available methods, and their associated reference, are: * 'asymmetric_truncated_quadratic'[1]_ * 'symmetric_truncated_quadratic'[1]_ * 'asymmetric_huber'[1]_ * 'symmetric_huber'[1]_ * 'asymmetric_indec'[2]_ * 'symmetric_indec'[2]_ threshold : float, optional The threshold value for the loss method, where the function goes from quadratic loss (such as used for least squares) to non-quadratic. For symmetric loss methods, residual values with absolute value less than threshold will have quadratic loss. For asymmetric loss methods, residual values less than the threshold will have quadratic loss. Default is None, which sets `threshold` to one-tenth of the standard deviation of the input data. alpha_factor : float, optional A value between 0 and 1 that controls the value of the penalty. Default is 0.99. Typically should not need to change this value. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Raises ------ ValueError Raised if `alpha_factor` is not between 0 and 1. Notes ----- In baseline literature, this procedure is sometimes called "backcor". References ---------- .. [1] Mazet, V., et al. Background removal from spectra by designing and minimising a non-quadratic cost function. Chemometrics and Intelligent Laboratory Systems, 2005, 76(2), 121-133. .. [2] Liu, J., et al. Goldindec: A Novel Algorithm for Raman Spectrum Baseline Correction. Applied Spectroscopy, 2015, 69(7), 834-842. """ if not 0 < alpha_factor <= 1: raise ValueError('alpha_factor must be between 0 and 1') symmetric_loss, method = _identify_loss_method(cost_function) loss_function = { 'huber': _huber_loss, 'truncated_quadratic': _truncated_quadratic_loss, 'indec': _indec_loss }[method] y, weight_array, pseudo_inverse = self._setup_polynomial( data, weights, poly_order, calc_vander=True, calc_pinv=True ) if threshold is None: threshold = np.std(y) / 10 loss_kwargs = { 'threshold': threshold, 'alpha_factor': alpha_factor, 'symmetric': symmetric_loss } sqrt_w = np.sqrt(weight_array) y = sqrt_w * y coef = pseudo_inverse @ y baseline = self._polynomial.vandermonde @ coef tol_history = np.empty(max_iter) for i in range(max_iter): baseline_old = baseline coef = pseudo_inverse @ (y + loss_function(y - sqrt_w * baseline, **loss_kwargs)) baseline = self._polynomial.vandermonde @ coef calc_difference = relative_difference(baseline_old, baseline) tol_history[i] = calc_difference if calc_difference < tol: break params = {'weights': weight_array, 'tol_history': tol_history[:i + 1]} if return_coef: params['coef'] = _convert_coef(coef, self.x_domain) return baseline, params
[docs] @_Algorithm._register(sort_keys=('weights', 'coef'), require_unique_x=True) def loess(self, data, fraction=0.2, total_points=None, poly_order=1, scale=3.0, tol=1e-3, max_iter=10, symmetric_weights=False, use_threshold=False, num_std=1, use_original=False, weights=None, return_coef=False, conserve_memory=True, delta=None): """ Locally estimated scatterplot smoothing (LOESS). Performs polynomial regression at each data point using the nearest points. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. fraction : float, optional The fraction of N data points to include for the fitting on each point. Default is 0.2. Not used if `total_points` is not None. total_points : int, optional The total number of points to include for the fitting on each point. Default is None, which will use `fraction` * N to determine the number of points. scale : float, optional A scale factor applied to the weighted residuals to control the robustness of the fit. Default is 3.0, as used in [1]_. Note that the original loess procedure for smoothing in [2]_ used a `scale` of ~4.05. poly_order : int, optional The polynomial order for fitting the baseline. Default is 1. tol : float, optional The exit criteria. Default is 1e-3. max_iter : int, optional The maximum number of iterations. Default is 10. symmetric_weights : bool, optional If False (default), will apply weighting asymmetrically, with residuals < 0 having a weight of 1, according to [1]_. If True, will apply weighting the same for both positive and negative residuals, which is regular LOESS. If `use_threshold` is True, this parameter is ignored. use_threshold : bool, optional If False (default), will compute weights each iteration to perform the robust fitting, which is regular LOESS. If True, will apply a threshold on the data being fit each iteration, based on the maximum values of the data and the fit baseline, as proposed by [3]_, similar to the modpoly and imodpoly techniques. num_std : float, optional The number of standard deviations to include when thresholding. Default is 1, which is the value used for the imodpoly technique. Only used if `use_threshold` is True. use_original : bool, optional If False (default), will compare the baseline of each iteration with the y-values of that iteration [4]_ when choosing minimum values for thresholding. If True, will compare the baseline with the original y-values given by `data` [5]_. Only used if `use_threshold` is True. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. conserve_memory : bool, optional If False, will cache the distance-weighted kernels for each value in `x_data` on the first iteration and reuse them on subsequent iterations to save time. The shape of the array of kernels is (len(`x_data`), `total_points`). If True (default), will recalculate the kernels each iteration, which uses very little memory, but is slower. Can usually set to False unless `x_data` and`total_points` are quite large and the function causes memory issues when cacheing the kernels. If numba is installed, there is no significant time difference since the calculations are sped up. delta : float, optional If `delta` is > 0, will skip all but the last x-value in the range `x_last + delta`, where `x_last` is the last x-value to be fit using weighted least squares, and instead use linear interpolation to calculate the fit for those x-values, which can significantly reduce the calculation time (same behavior as in statsmodels [6]_ and Cleveland's original Fortran lowess implementation [7]_). Fits all x-values if `delta` is <= 0. Default is None, which sets `delta` to `0.01 * (max(x_data) - min(x_data))`. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. Does NOT contain the individual distance-weighted kernels for each x-value. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (N, poly_order + 1) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. If `delta` is > 0, the coefficients for any skipped x-value will all be 0. Raises ------ ValueError Raised if the number of points per window for the fitting is less than `poly_order` + 1 or greater than the total number of points, or if the values in `self.x` are not strictly increasing. Notes ----- The iterative, robust, aspect of the fitting can be achieved either through reweighting based on the residuals (the typical usage), or thresholding the fit data based on the residuals, as proposed by [3]_, similar to the modpoly and imodpoly techniques. In baseline literature, this procedure is sometimes called "rbe", meaning "robust baseline estimate". References ---------- .. [1] Ruckstuhl, A.F., et al. Baseline subtraction using robust local regression estimation. J. Quantitative Spectroscopy and Radiative Transfer, 2001, 68, 179-193. .. [2] Cleveland, W. Robust locally weighted regression and smoothing scatterplots. Journal of the American Statistical Association, 1979, 74(368), 829-836. .. [3] Komsta, Ł. Comparison of Several Methods of Chromatographic Baseline Removal with a New Approach Based on Quantile Regression. Chromatographia, 2011, 73, 721-731. .. [4] Gan, F., et al. Baseline correction by improved iterative polynomial fitting with automatic threshold. Chemometrics and Intelligent Laboratory Systems, 2006, 82, 59-65. .. [5] Lieber, C., et al. Automated method for subtraction of fluorescence from biological raman spectra. Applied Spectroscopy, 2003, 57(11), 1363-1367. .. [6] https://github.com/statsmodels/statsmodels. .. [7] https://www.netlib.org/go (lowess.f is the file). """ if total_points is None: total_points = ceil(fraction * self._size) if total_points < poly_order + 1: raise ValueError('total points must be greater than polynomial order + 1') elif total_points > self._size: raise ValueError(( 'points per window is higher than total number of points; lower either ' '"fraction" or "total_points"' )) elif poly_order > 2: warnings.warn( ('polynomial orders greater than 2 can have numerical issues;' ' consider using a polynomial order of 1 or 2 instead'), ParameterWarning, stacklevel=2 ) y, weight_array = self._setup_polynomial(data, weights, poly_order, calc_vander=True) if use_original: y0 = y if delta is None: delta = 0.01 * (self.x_domain[1] - self.x_domain[0]) # x is the scaled version of self.x to fit within the [-1, 1] domain x = np.polynomial.polyutils.mapdomain(self.x, self.x_domain, np.array([-1., 1.])) # find the indices for fitting beforehand so that the fitting can be done # in parallel; cast delta as float so numba does not have to compile for # both int and float windows, fits, skips = _determine_fits(self.x, self._size, total_points, float(delta)) # np.polynomial.polynomial.polyvander returns a Fortran-ordered array, which # is not continguous when indexed (ie. vandermonde[i]) and issues a warning # when using numba, so convert Vandermonde matrix to C-ordering; without Numba, # there is no major slowdown using the non-contiguous array if _HAS_NUMBA: vandermonde = np.ascontiguousarray(self._polynomial.vandermonde) else: vandermonde = self._polynomial.vandermonde baseline = y coefs = np.zeros((self._size, poly_order + 1)) tol_history = np.empty(max_iter + 1) sqrt_w = np.sqrt(weight_array) # do max_iter + 1 since a max_iter of 0 would return y as baseline otherwise for i in range(max_iter + 1): baseline_old = baseline if conserve_memory: baseline = _loess_low_memory( x, y, sqrt_w, coefs, vandermonde, self._size, windows, fits ) elif i == 0: kernels, baseline = _loess_first_loop( x, y, sqrt_w, coefs, vandermonde, total_points, self._size, windows, fits ) else: baseline = _loess_nonfirst_loops( y, sqrt_w, coefs, vandermonde, kernels, windows, self._size, fits ) _fill_skips(x, baseline, skips) calc_difference = relative_difference(baseline_old, baseline) tol_history[i] = calc_difference if calc_difference < tol: break if use_threshold: y = np.minimum( y0 if use_original else y, baseline + num_std * np.std(y - baseline) ) else: residual = y - baseline # TODO median_absolute_value can be 0 if more than half of residuals are # 0 (perfect fit); can that ever really happen? if so, should prevent dividing by 0 sqrt_w = _tukey_square( residual / _median_absolute_value(residual), scale, symmetric_weights ) params = {'weights': sqrt_w**2, 'tol_history': tol_history[:i + 1]} if return_coef: # TODO maybe leave out the coefficients from the rest of the calculations # since they are otherwise unused, and just fit x vs baseline here; would # save a little memory; is providing coefficients for loess even useful? params['coef'] = np.array([_convert_coef(coef, self.x_domain) for coef in coefs]) return baseline, params
[docs] @_Algorithm._register(sort_keys=('weights',)) def quant_reg(self, data, poly_order=2, quantile=0.05, tol=1e-6, max_iter=250, weights=None, eps=None, return_coef=False): """ Approximates the baseline of the data using quantile regression. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. quantile : float, optional The quantile at which to fit the baseline. Default is 0.05. tol : float, optional The exit criteria. Default is 1e-6. For extreme quantiles (`quantile` < 0.01 or `quantile` > 0.99), may need to use a lower value to get a good fit. max_iter : int, optional The maximum number of iterations. Default is 250. For extreme quantiles (`quantile` < 0.01 or `quantile` > 0.99), may need to use a higher value to ensure convergence. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. eps : float, optional A small value added to the square of the residual to prevent dividing by 0. Default is None, which uses the square of the maximum-absolute-value of the fit each iteration multiplied by 1e-6. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input `x_data` and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Raises ------ ValueError Raised if `quantile` is not between 0 and 1. Notes ----- Application of quantile regression for baseline fitting ss described in [1]_. Performs quantile regression using iteratively reweighted least squares (IRLS) as described in [2]_. References ---------- .. [1] Komsta, Ł. Comparison of Several Methods of Chromatographic Baseline Removal with a New Approach Based on Quantile Regression. Chromatographia, 2011, 73, 721-731. .. [2] Schnabel, S., et al. Simultaneous estimation of quantile curves using quantile sheets. AStA Advances in Statistical Analysis, 2013, 97, 77-87. """ # TODO provide a way to estimate best poly_order based on AIC like in Komsta? could be # useful for all polynomial methods; maybe could be an optimizer function if not 0 < quantile < 1: raise ValueError('quantile must be between 0 and 1.') y, weight_array = self._setup_polynomial(data, weights, poly_order, calc_vander=True) # estimate first iteration using least squares sqrt_w = np.sqrt(weight_array) coef = np.linalg.lstsq(self._polynomial.vandermonde * sqrt_w[:, None], y * sqrt_w, None)[0] baseline = self._polynomial.vandermonde @ coef tol_history = np.empty(max_iter) for i in range(max_iter): baseline_old = baseline sqrt_w = np.sqrt(_weighting._quantile(y, baseline, quantile, eps)) coef = np.linalg.lstsq( self._polynomial.vandermonde * sqrt_w[:, None], y * sqrt_w, None )[0] baseline = self._polynomial.vandermonde @ coef # relative_difference(baseline_old, baseline, 1) gives nearly same result and # the l2 norm is faster to calculate, so use that instead of l1 norm calc_difference = relative_difference(baseline_old, baseline) tol_history[i] = calc_difference if calc_difference < tol: break params = {'weights': sqrt_w**2, 'tol_history': tol_history[:i + 1]} if return_coef: params['coef'] = _convert_coef(coef, self.x_domain) return baseline, params
[docs] @_Algorithm._register(sort_keys=('weights',)) def goldindec(self, data, poly_order=2, tol=1e-3, max_iter=250, weights=None, cost_function='asymmetric_indec', peak_ratio=0.5, alpha_factor=0.99, tol_2=1e-3, tol_3=1e-6, max_iter_2=100, return_coef=False): """ Fits a polynomial baseline using a non-quadratic cost function. The non-quadratic cost functions penalize residuals with larger values, giving a more robust fit compared to normal least-squares. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. tol : float, optional The exit criteria for the fitting with a given threshold value. Default is 1e-3. max_iter : int, optional The maximum number of iterations for fitting a threshold value. Default is 250. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. cost_function : str, optional The non-quadratic cost function to minimize. Unlike :meth:`~.Baseline.penalized_poly`, this function only works with asymmetric cost functions, so the symmetry prefix ('a' or 'asymmetric') is optional (eg. 'indec' and 'a_indec' are the same). Default is 'asymmetric_indec'. Available methods, and their associated reference, are: * 'asymmetric_indec'[1]_ * 'asymmetric_truncated_quadratic'[2]_ * 'asymmetric_huber'[2]_ peak_ratio : float, optional A value between 0 and 1 that designates how many points in the data belong to peaks. Values are valid within ~10% of the actual peak ratio. Default is 0.5. alpha_factor : float, optional A value between 0 and 1 that controls the value of the penalty. Default is 0.99. Typically should not need to change this value. tol_2 : float, optional The exit criteria for the difference between the optimal up-down ratio (number of points above 0 in the residual compared to number of points below 0) and the up-down ratio for a given threshold value. Default is 1e-3. tol_3 : float, optional The exit criteria for the relative change in the threshold value. Default is 1e-6. max_iter_2 : float, optional The number of iterations for iterating between different threshold values. Default is 100. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray, shape (J, K) An array containing the calculated tolerance values for each iteration of both threshold values and fit values. Index 0 are the tolerence values for the difference in up-down ratios, index 1 are the tolerance values for the relative change in the threshold, and indices >= 2 are the tolerance values for each fit. All values that were not used in fitting have values of 0. Shape J is 2 plus the number of iterations for the threshold to converge (related to `max_iter_2`, `tol_2`, `tol_3`), and shape K is the maximum of the number of iterations for the threshold and the maximum number of iterations for all of the fits of the various threshold values (related to `max_iter` and `tol`). * 'threshold' : float The optimal threshold value. Could be used in :meth:`~.Baseline.penalized_poly` for fitting other similar data. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Raises ------ ValueError Raised if `alpha_factor` or `peak_ratio` are not between 0 and 1, or if the specified cost function is symmetric. References ---------- .. [1] Liu, J., et al. Goldindec: A Novel Algorithm for Raman Spectrum Baseline Correction. Applied Spectroscopy, 2015, 69(7), 834-842. .. [2] Mazet, V., et al. Background removal from spectra by designing and minimising a non-quadratic cost function. Chemometrics and Intelligent Laboratory Systems, 2005, 76(2), 121-133. """ if not 0 < alpha_factor <= 1: raise ValueError('alpha_factor must be between 0 and 1') elif not 0 < peak_ratio < 1: raise ValueError('peak_ratio must be between 0 and 1') try: symmetric_loss, method = _identify_loss_method(cost_function) except ValueError: # do not require a prefix since cost must be asymmetric symmetric_loss, method = _identify_loss_method('a_' + cost_function) if symmetric_loss: # symmetric cost functions don't work due to how the up-down ratio vs # peak_ratio function was created in the reference; in theory, could simulate # spectra with both positive and negative peaks following the reference # and build another empirical function, but would likely need to also # add other parameters detailing the percent of positive vs negative peaks, # etc., so it's not worth the effort raise ValueError('goldindec only works for asymmetric cost functions') loss_function = { 'huber': _huber_loss, 'truncated_quadratic': _truncated_quadratic_loss, 'indec': _indec_loss }[method] y, weight_array, pseudo_inverse = self._setup_polynomial( data, weights, poly_order, calc_vander=True, calc_pinv=True ) up_down_ratio_goal = ( 0.7679 + 11.2358 * peak_ratio - 39.7064 * peak_ratio**2 + 92.3583 * peak_ratio**3 ) # TODO reference states threshold must be <= 2 for half-quadratic minimization to # be valid for indec cost function, and normalized y so that threshold is always <= 2; # however, it seems to work fine without normalization; just be aware in case errors # occur, may have to normalize y in both this function and penalized_poly sqrt_w = np.sqrt(weight_array) y_fit = sqrt_w * y coef = pseudo_inverse @ y_fit initial_baseline = self._polynomial.vandermonde @ coef a = 0 # reference used b=1, but normalized y before fitting; instead, set b as max of # initial residual b = abs((y - initial_baseline).max()) threshold = a + 0.618 * (b - a) loss_kwargs = { 'threshold': threshold, 'alpha_factor': alpha_factor, 'symmetric': symmetric_loss } # have to use zeros rather than empty for tol_history since each inner fit may # have a different number of iterations tol_history = np.zeros((max_iter_2 + 2, max(max_iter, max_iter_2))) j_max = 0 for i in range(max_iter_2): baseline = initial_baseline for j in range(max_iter): baseline_old = baseline coef = pseudo_inverse @ ( y_fit + loss_function(y_fit - sqrt_w * baseline, **loss_kwargs) ) baseline = self._polynomial.vandermonde @ coef calc_difference = relative_difference(baseline_old, baseline) tol_history[i + 2, j] = calc_difference if calc_difference < tol: break j_max = max(j, j_max) up_count = (y > baseline).sum() up_down_ratio = up_count / max(1, self._size - up_count) calc_difference = up_down_ratio - up_down_ratio_goal tol_history[0, i] = calc_difference if calc_difference > tol_2: a = threshold elif calc_difference < -tol_2: b = threshold else: break threshold = a + 0.618 * (b - a) # this exit criteria was not stated in the reference, but the change in threshold # becomes zero fairly quickly, so need to also exit rather than needlessly # continuing to calculate with the same threshold value calc_difference = relative_difference(loss_kwargs['threshold'], threshold) tol_history[1, i] = calc_difference if calc_difference < tol_3: break loss_kwargs['threshold'] = threshold params = { 'weights': weight_array, 'tol_history': tol_history[:i + 3, :max(i, j_max) + 1], 'threshold': loss_kwargs['threshold'] } if return_coef: params['coef'] = _convert_coef(coef, self.x_domain) return baseline, params
_polynomial_wrapper = _class_wrapper(_Polynomial) @_polynomial_wrapper def poly(data, x_data=None, poly_order=2, weights=None, return_coef=False): """ Computes a polynomial that fits the baseline of the data. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. x_data : array-like, shape (N,), optional The x-values of the measured data. Default is None, which will create an array from -1 to 1 with N points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'coef': numpy.ndarray, shape (poly_order,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Notes ----- To only fit regions without peaks, supply a weight array with zero values at the indices where peaks are located. """ @_polynomial_wrapper def modpoly(data, x_data=None, poly_order=2, tol=1e-3, max_iter=250, weights=None, use_original=False, mask_initial_peaks=False, return_coef=False): """ The modified polynomial (ModPoly) baseline algorithm. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. x_data : array-like, shape (N,), optional The x-values of the measured data. Default is None, which will create an array from -1 to 1 with N points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. tol : float, optional The exit criteria. Default is 1e-3. max_iter : int, optional The maximum number of iterations. Default is 250. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. use_original : bool, optional If False (default), will compare the baseline of each iteration with the y-values of that iteration [1]_ when choosing minimum values. If True, will compare the baseline with the original y-values given by `data` [2]_. mask_initial_peaks : bool, optional If True, will mask any data where the initial baseline fit + the standard deviation of the residual is less than measured data [3]_. Default is False. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Notes ----- Algorithm originally developed in [2]_ and then slightly modified in [1]_. References ---------- .. [1] Gan, F., et al. Baseline correction by improved iterative polynomial fitting with automatic threshold. Chemometrics and Intelligent Laboratory Systems, 2006, 82, 59-65. .. [2] Lieber, C., et al. Automated method for subtraction of fluorescence from biological raman spectra. Applied Spectroscopy, 2003, 57(11), 1363-1367. .. [3] Zhao, J., et al. Automated Autofluorescence Background Subtraction Algorithm for Biomedical Raman Spectroscopy, Applied Spectroscopy, 2007, 61(11), 1225-1232. """ @_polynomial_wrapper def imodpoly(data, x_data=None, poly_order=2, tol=1e-3, max_iter=250, weights=None, use_original=False, mask_initial_peaks=True, return_coef=False, num_std=1): """ The improved modofied polynomial (IModPoly) baseline algorithm. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. x_data : array-like, shape (N,), optional The x-values of the measured data. Default is None, which will create an array from -1 to 1 with N points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. tol : float, optional The exit criteria. Default is 1e-3. max_iter : int, optional The maximum number of iterations. Default is 250. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. use_original : bool, optional If False (default), will compare the baseline of each iteration with the y-values of that iteration [4]_ when choosing minimum values. If True, will compare the baseline with the original y-values given by `data` [5]_. mask_initial_peaks : bool, optional If True (default), will mask any data where the initial baseline fit + the standard deviation of the residual is less than measured data [6]_. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. num_std : float, optional The number of standard deviations to include when thresholding. Default is 1. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Notes ----- Algorithm originally developed in [6]_. References ---------- .. [4] Gan, F., et al. Baseline correction by improved iterative polynomial fitting with automatic threshold. Chemometrics and Intelligent Laboratory Systems, 2006, 82, 59-65. .. [5] Lieber, C., et al. Automated method for subtraction of fluorescence from biological raman spectra. Applied Spectroscopy, 2003, 57(11), 1363-1367. .. [6] Zhao, J., et al. Automated Autofluorescence Background Subtraction Algorithm for Biomedical Raman Spectroscopy, Applied Spectroscopy, 2007, 61(11), 1225-1232. """ # adapted from (https://www.mathworks.com/matlabcentral/fileexchange/27429-background-correction); # see license above def _huber_loss(residual, threshold=1.0, alpha_factor=0.99, symmetric=True): """ The Huber non-quadratic cost function. Parameters ---------- residual : numpy.ndarray, shape (N,) The residual array. threshold : float, optional Any residual values below the threshold are given quadratic loss. Default is 1.0. alpha_factor : float, optional The scale between 0 and 1 to multiply the cost function's alpha_max value (see Notes below). Default is 0.99. symmetric : bool, optional If True (default), the cost function is symmetric and applies the same weighting for positive and negative values. If False, will apply weights asymmetrically so that only positive weights are given the non-quadratic weigting and negative weights have normal, quadratic weighting. Returns ------- weights : numpy.ndarray, shape (N,) The weight array. Notes ----- The returned result is -residual + alpha_factor * alpha_max * phi'(residual) where phi'(x) is the derivative of the huber loss function, phi(x). References ---------- Mazet, V., et al. Background removal from spectra by designing and minimising a non-quadratic cost function. Chemometrics and Intelligent Laboratory Systems, 2005, 76(2), 121-133. """ alpha = alpha_factor * 0.5 # alpha_max for huber is 0.5 if symmetric: mask = (np.abs(residual) < threshold) weights = ( mask * residual * (2 * alpha - 1) + (~mask) * 2 * alpha * threshold * np.sign(residual) ) else: mask = (residual < threshold) weights = ( mask * residual * (2 * alpha - 1) + (~mask) * (2 * alpha * threshold - residual) ) return weights # adapted from (https://www.mathworks.com/matlabcentral/fileexchange/27429-background-correction); # see license above def _truncated_quadratic_loss(residual, threshold=1.0, alpha_factor=0.99, symmetric=True): """ The Truncated-Quadratic non-quadratic cost function. Parameters ---------- residual : numpy.ndarray, shape (N,) The residual array. threshold : float, optional Any residual values below the threshold are given quadratic loss. Default is 1.0. alpha_factor : float, optional The scale between 0 and 1 to multiply the cost function's alpha_max value (see Notes below). Default is 0.99. symmetric : bool, optional If True (default), the cost function is symmetric and applies the same weighting for positive and negative values. If False, will apply weights asymmetrically so that only positive weights are given the non-quadratic weigting and negative weights have normal, quadratic weighting. Returns ------- weights : numpy.ndarray, shape (N,) The weight array. Notes ----- The returned result is -residual + alpha_factor * alpha_max * phi'(residual) where phi'(x) is the derivative of the truncated quadratic function, phi(x). References ---------- Mazet, V., et al. Background removal from spectra by designing and minimising a non-quadratic cost function. Chemometrics and Intelligent Laboratory Systems, 2005, 76(2), 121-133. """ alpha = alpha_factor * 0.5 # alpha_max for truncated quadratic is 0.5 if symmetric: mask = (np.abs(residual) < threshold) else: mask = (residual < threshold) return mask * residual * (2 * alpha - 1) - (~mask) * residual def _indec_loss(residual, threshold=1.0, alpha_factor=0.99, symmetric=True): """ The Indec non-quadratic cost function. Parameters ---------- residual : numpy.ndarray, shape (N,) The residual array. threshold : float, optional Any residual values below the threshold are given quadratic loss. Default is 1.0. alpha_factor : float, optional The scale between 0 and 1 to multiply the cost function's alpha_max value (see Notes below). Default is 0.99. symmetric : bool, optional If True (default), the cost function is symmetric and applies the same weighting for positive and negative values. If False, will apply weights asymmetrically so that only positive weights are given the non-quadratic weigting and negative weights have normal, quadratic weighting. Returns ------- weights : numpy.ndarray, shape (N,) The weight array. Notes ----- The returned result is -residual + alpha_factor * alpha_max * phi'(residual) where phi'(x) is the derivative of the Indec function, phi(x). References ---------- Liu, J., et al. Goldindec: A Novel Algorithm for Raman Spectrum Baseline Correction. Applied Spectroscopy, 2015, 69(7), 834-842. Mazet, V., et al. Background removal from spectra by designing and minimising a non-quadratic cost function. Chemometrics and Intelligent Laboratory Systems, 2005, 76(2), 121-133. """ alpha = alpha_factor * 0.5 # alpha_max for indec is 0.5 if symmetric: mask = (np.abs(residual) < threshold) multiple = np.sign(residual) else: mask = (residual < threshold) # multiple=1 is same as sign(residual) since residual is always > 0 # for asymmetric case, but this allows not doing the sign calculation multiple = 1 weights = ( mask * residual * (2 * alpha - 1) - (~mask) * ( residual + alpha * multiple * threshold**3 / np.maximum(2 * residual**2, _MIN_FLOAT) ) ) return weights def _identify_loss_method(loss_method): """ Identifies the symmetry for the given loss method. Parameters ---------- loss_method : str The loss method to use. Should have the symmetry identifier as the prefix. Returns ------- symmetric : bool True if `loss_method` had 's_' or 'symmetric_' as the prefix, else False. str The input `loss_method` value without the first section that indicated the symmetry. Raises ------ ValueError Raised if the loss method does not have the correct form. """ prefix, *split_method = loss_method.lower().split('_') if prefix not in ('a', 's', 'asymmetric', 'symmetric') or not split_method: raise ValueError('must specify loss function symmetry by appending "a_" or "s_"') if prefix in ('a', 'asymmetric'): symmetric = False else: symmetric = True return symmetric, '_'.join(split_method) # adapted from (https://www.mathworks.com/matlabcentral/fileexchange/27429-background-correction); # see license above @_polynomial_wrapper def penalized_poly(data, x_data=None, poly_order=2, tol=1e-3, max_iter=250, weights=None, cost_function='asymmetric_truncated_quadratic', threshold=None, alpha_factor=0.99, return_coef=False): """ Fits a polynomial baseline using a non-quadratic cost function. The non-quadratic cost functions penalize residuals with larger values, giving a more robust fit compared to normal least-squares. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. x_data : array-like, shape (N,), optional The x-values of the measured data. Default is None, which will create an array from -1 to 1 with N points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. tol : float, optional The exit criteria. Default is 1e-3. max_iter : int, optional The maximum number of iterations. Default is 250. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. cost_function : str, optional The non-quadratic cost function to minimize. Must indicate symmetry of the method by appending 'a' or 'asymmetric' for asymmetric loss, and 's' or 'symmetric' for symmetric loss. Default is 'asymmetric_truncated_quadratic'. Available methods, and their associated reference, are: * 'asymmetric_truncated_quadratic'[7]_ * 'symmetric_truncated_quadratic'[7]_ * 'asymmetric_huber'[7]_ * 'symmetric_huber'[7]_ * 'asymmetric_indec'[8]_ * 'symmetric_indec'[8]_ threshold : float, optional The threshold value for the loss method, where the function goes from quadratic loss (such as used for least squares) to non-quadratic. For symmetric loss methods, residual values with absolute value less than threshold will have quadratic loss. For asymmetric loss methods, residual values less than the threshold will have quadratic loss. Default is None, which sets `threshold` to one-tenth of the standard deviation of the input data. alpha_factor : float, optional A value between 0 and 1 that controls the value of the penalty. Default is 0.99. Typically should not need to change this value. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Raises ------ ValueError Raised if `alpha_factor` is not between 0 and 1. Notes ----- In baseline literature, this procedure is sometimes called "backcor". References ---------- .. [7] Mazet, V., et al. Background removal from spectra by designing and minimising a non-quadratic cost function. Chemometrics and Intelligent Laboratory Systems, 2005, 76(2), 121-133. .. [8] Liu, J., et al. Goldindec: A Novel Algorithm for Raman Spectrum Baseline Correction. Applied Spectroscopy, 2015, 69(7), 834-842. """ def _tukey_square(residual, scale=3, symmetric=False): """ The square root of Tukey's bisquare function. Parameters ---------- residual : numpy.ndarray, shape (N,) The residual array of the fit. scale : float, optional A scale factor applied to the weighted residuals to control the robustness of the fit. Default is 3.0. symmetric : bool, optional If False (default), will apply weighting asymmetrically, with residuals < 0 having full weight. If True, will apply weighting the same for both positive and negative residuals, which is regular LOESS. Returns ------- weights : numpy.ndarray, shape (N,) The weighting array. Notes ----- The function is technically sqrt(Tukey's bisquare) since the outer power of 2 is not performed. This is intentional, so that the square root for weighting in least squares does not need to be done, speeding up the calculation. References ---------- Ruckstuhl, A.F., et al., Baseline subtraction using robust local regression estimation. J. Quantitative Spectroscopy and Radiative Transfer, 2001, 68, 179-193. """ if symmetric: inner = residual / scale weights = np.maximum(0, 1 - inner * inner) else: weights = np.ones_like(residual) mask = residual > 0 inner = residual[mask] / scale weights[mask] = np.maximum(0, 1 - inner * inner) return weights def _median_absolute_value(values): """ Computes the median absolute value (MAV) of an array. Parameters ---------- values : array-like The array of values to use for the calculation. Returns ------- float The scaled median absolute value for the input array. Notes ----- The 1/0.6744897501960817 scale factor is to make the result comparable to the standard deviation of a Gaussian distribution. The divisor is obtained by calculating the value at which the cumulative distribution function of a Gaussian distribution is 0.75 (see https://en.wikipedia.org/wiki/Median_absolute_deviation), which can be obtained by:: from scipy.special import ndtri ndtri(0.75) # equals 0.6744897501960817 To calculate the median absolute difference (MAD) using this function, simply do:: _median_absolute_value(values - np.median(values)) References ---------- Ruckstuhl, A.F., et al., Baseline subtraction using robust local regression estimation. J. Quantitative Spectroscopy and Radiative Transfer, 2001, 68, 179-193. https://en.wikipedia.org/wiki/Median_absolute_deviation. """ return np.median(np.abs(values)) / 0.6744897501960817 @jit(nopython=True, cache=True) def _loess_solver(AT, b): """ Solves the equation `A x = b` given `A.T` and `b`. Parameters ---------- AT : numpy.ndarray, shape (M, N) The transposed `A` matrix. b : numpy.ndarray, shape (N,) The `b` array. Returns ------- numpy.ndarray, shape (N,) The solution to the normal equation. Notes ----- Uses np.linalg.solve (which uses LU decomposition) rather than np.linalg.lstsq (which uses SVD) since solve is ~30-60% faster. np.linalg.solve requires ``A.T * A``, which squares the condition number of ``A``, but on tested datasets the relative difference when using solve vs lstsq (using np.allclose) is ~1e-10 to 1e-13 for poly_orders of 1 or 2, which seems fine; the relative differences increase to ~1e-6 to 1e-9 for a poly_order of 3, and ~1e-4 to 1e-6 for a poly_order of 4, but loess should use a poly_order <= 2, so that should not be a problem. """ return np.linalg.solve(AT.dot(AT.T), AT.dot(b)) @jit(nopython=True, cache=True) def _fill_skips(x, baseline, skips): """ Fills in the skipped baseline points using linear interpolation. Parameters ---------- x : numpy.ndarray The array of x-values. baseline : numpy.ndarray The array of baseline values with all fit points allocated. All skipped points will be filled in using interpolation. skips : numpy.ndarray, shape (G, 2) The array of left and right indices that define the windows for interpolation, with length G being the number of interpolation segments. Indices are set such that `baseline[skips[i][0]:skips[i][1]]` will have fitted values at the first and last indices and all other values (the slice [1:-1]) will be calculated by interpolation. Notes ----- All changes to `baseline` are done inplace. """ for i in range(skips.shape[0]): window = skips[i] left = window[0] right = window[1] _interp_inplace(x[left:right], baseline[left:right], baseline[left], baseline[right - 1]) # adapted from (https://gist.github.com/agramfort/850437); see license above @jit(nopython=True, cache=True) def _loess_low_memory(x, y, weights, coefs, vander, num_x, windows, fits): """ A version of loess that uses near constant memory. The distance-weighted kernel for each x-value is computed each loop, rather than cached, so memory usage is low but the calculation is slightly slower. Parameters ---------- x : numpy.ndarray, shape (N,) The x-values of the measured data, with N data points. y : numpy.ndarray, shape (N,) The y-values of the measured data, with N points. weights : numpy.ndarray, shape (N,) The array of weights. coefs : numpy.ndarray, shape (N, ``poly_order + 1``) The array of polynomial coefficients (with polynomial order poly_order), for each value in `x`. vander : numpy.ndarray, shape (N, ``poly_order + 1``) The Vandermonde matrix for the `x` array. num_x : int The number of data points in `x`, also known as N. windows : numpy.ndarray, shape (F, 2) An array of left and right indices that define the fitting window for each fit x-value. The length is F, which is the total number of fit points. If `fit_dx` is <= 0, F is equal to N, the total number of x-values. fits : numpy.ndarray, shape (F,) The array of indices indicating which x-values to fit. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. Notes ----- The coefficient array, `coefs`, is modified inplace. """ baseline = np.empty(num_x) y_fit = y * weights vander_fit = vander.T * weights for idx in range(fits.shape[0]): i = fits[idx] window = windows[idx] left = window[0] right = window[1] difference = np.abs(x[left:right] - x[i]) difference = difference / max(difference[0], difference[-1]) difference = difference * difference * difference difference = 1 - difference kernel = np.sqrt(difference * difference * difference) coef = _loess_solver( kernel * vander_fit[:, left:right], kernel * y_fit[left:right] ) baseline[i] = vander[i].dot(coef) coefs[i] = coef return baseline # adapted from (https://gist.github.com/agramfort/850437); see license above @jit(nopython=True, cache=True) def _loess_first_loop(x, y, weights, coefs, vander, total_points, num_x, windows, fits): """ The initial fit for loess that also caches the window values for each x-value. Parameters ---------- x : numpy.ndarray, shape (N,) The x-values of the measured data, with N data points. y : numpy.ndarray, shape (N,) The y-values of the measured data, with N points. weights : numpy.ndarray, shape (N,) The array of weights. coefs : numpy.ndarray, shape (N, ``poly_order + 1``) The array of polynomial coefficients (with polynomial order poly_order), for each value in `x`. vander : numpy.ndarray, shape (N, ``poly_order + 1``) The Vandermonde matrix for the `x` array. total_points : int The number of points to include when fitting each x-value. num_x : int The number of data points in `x`, also known as N. windows : numpy.ndarray, shape (F, 2) An array of left and right indices that define the fitting window for each fit x-value. The length is F, which is the total number of fit points. If `fit_dx` is <= 0, F is equal to N, the total number of x-values. fits : numpy.ndarray, shape (F,) The array of indices indicating which x-values to fit. Returns ------- kernels : numpy.ndarray, shape (N, total_points) The array containing the distance-weighted kernel for each x-value. baseline : numpy.ndarray, shape (N,) The calculated baseline. Notes ----- The coefficient array, `coefs`, is modified inplace. """ kernels = np.empty((num_x, total_points)) baseline = np.empty(num_x) y_fit = y * weights vander_fit = vander.T * weights for idx in range(fits.shape[0]): i = fits[idx] window = windows[idx] left = window[0] right = window[1] difference = np.abs(x[left:right] - x[i]) difference = difference / max(difference[0], difference[-1]) difference = difference * difference * difference difference = 1 - difference kernel = np.sqrt(difference * difference * difference) kernels[i] = kernel coef = _loess_solver( kernel * vander_fit[:, left:right], kernel * y_fit[left:right] ) baseline[i] = vander[i].dot(coef) coefs[i] = coef return kernels, baseline @jit(nopython=True, cache=True) def _loess_nonfirst_loops(y, weights, coefs, vander, kernels, windows, num_x, fits): """ The loess fit to use after the first loop that uses the cached window values. Parameters ---------- y : numpy.ndarray, shape (N,) The y-values of the measured data, with N points. weights : numpy.ndarray, shape (N,) The array of weights. coefs : numpy.ndarray, shape (N, ``poly_order + 1``) The array of polynomial coefficients (with polynomial order poly_order), for each value in `x`. vander : numpy.ndarray, shape (N, ``poly_order + 1``) The Vandermonde matrix for the `x` array. kernels : numpy.ndarray, shape (N, total_points) The array containing the distance-weighted kernel for each x-value. Each kernel has a length of total_points. windows : numpy.ndarray, shape (F, 2) An array of left and right indices that define the fitting window for each fit x-value. The length is F, which is the total number of fit points. If `fit_dx` is <= 0, F is equal to N, the total number of x-values. num_x : int The total number of values, N. fits : numpy.ndarray, shape (F,) The array of indices indicating which x-values to fit. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. Notes ----- The coefficient array, `coefs`, is modified inplace. """ baseline = np.empty(num_x) y_fit = y * weights vander_fit = vander.T * weights for idx in range(fits.shape[0]): i = fits[idx] window = windows[idx] left = window[0] right = window[1] kernel = kernels[i] coef = _loess_solver( kernel * vander_fit[:, left:right], kernel * y_fit[left:right] ) baseline[i] = vander[i].dot(coef) coefs[i] = coef return baseline @jit(nopython=True, cache=True) def _determine_fits(x, num_x, total_points, delta): """ Determines the x-values to fit and the left and right indices for each fit x-value. The windows are set before fitting so that fitting can be done in parallel when numba is installed, since the left and right indices would otherwise need to be determined in order. Similarly, determining which x-values to fit would not be able to be done in parallel since it requires knowledge of the last x-value fit. Parameters ---------- x : numpy.ndarray, shape (N,) The array of x-values. num_x : int The total number of x-values, N. total_points : int The number of values to include in each fitting window. delta : float If `delta` is > 0, will skip all but the last x-value in the range x_last + `delta`, where x_last is the last x-value to be fit. Fits all x-values if `delta` is <= 0. Returns ------- windows : numpy.ndarray, shape (F, 2) An array of left and right indices that define the fitting window for each fit x-value. The length is F, which is the total number of fit points. If `fit_dx` is <= 0, F is equal to N, the total number of x-values. Indices are set such that the number of values in `x[windows[i][0]:windows[i][1]] is equal to `total_points`. fits : numpy.ndarray, shape (F,) The array of indices indicating which x-values to fit. skips : numpy.ndarray, shape (G, 2) The array of left and right indices that define the windows for interpolation, with length G being the number of interpolation segments. G is 0 if `fit_dx` is <= 0. Indices are set such that `baseline[skips[i][0]:skips[i][1]]` will have fitted values at the first and last indices and all other values (the slice [1:-1]) will be calculated by interpolation. Notes ----- The dtype `np.intp` is used for `fits`, `skips`, and `windows` to be consistent with numpy since numpy internally uses that type when referring to indices. """ # faster to allocate array and return only filled in sections # rather than constanly appending to a list if delta > 0: check_fits = True fits = np.empty(num_x, dtype=np.intp) fits[0] = 0 # always fit first item skips = np.empty((num_x, 2), dtype=np.intp) else: # TODO maybe use another function when fitting all points in order # to skip the if check_fits check for every x-value; does it affect # calculation time that much? check_fits = False # TODO once numba minimum version is >= 0.47, can use dtype kwarg in np.arange fits = np.arange(num_x).astype(np.intp) # numba cannot compile in nopython mode when directly creating # np.array([], dtype=np.intp), so work-around by creating np.array([[0, 0]]) # and then index with [:total_skips], which becomes np.array([]) # since total_skips is 0 when delta is <= 0. skips = np.array([[0, 0]], dtype=np.intp) windows = np.empty((num_x, 2), dtype=np.intp) windows[0] = (0, total_points) total_fits = 1 total_skips = 0 skip_start = 0 skip_range = x[0] + delta left = 0 right = total_points for i in range(1, num_x - 1): x_val = x[i] if check_fits: # use x[i+1] rather than x[i] since it ensures that the last value within # the range x_last_fit + delta is used; x[i+1] is also guranteed to be >= x[i] if x[i + 1] < skip_range: if not skip_start: skip_start = i continue else: skip_range = x_val + delta fits[total_fits] = i if skip_start: skips[total_skips] = (skip_start - 1, i + 1) total_skips += 1 skip_start = 0 while right < num_x and x_val - x[left] > x[right] - x_val: left += 1 right += 1 window = windows[total_fits] window[0] = left window[1] = right total_fits += 1 if skip_start: # fit second to last x-value fits[total_fits] = num_x - 2 if x[-1] - x[-2] < x[-2] - x[num_x - total_points]: windows[total_fits] = (num_x - total_points, num_x) else: windows[total_fits] = (num_x - total_points - 1, num_x - 1) total_fits += 1 skips[total_skips] = (skip_start - 1, num_x - 1) total_skips += 1 # always fit last item fits[total_fits] = num_x - 1 windows[total_fits] = (num_x - total_points, num_x) total_fits += 1 return windows[:total_fits], fits[:total_fits], skips[:total_skips] @_polynomial_wrapper def loess(data, x_data=None, fraction=0.2, total_points=None, poly_order=1, scale=3.0, tol=1e-3, max_iter=10, symmetric_weights=False, use_threshold=False, num_std=1, use_original=False, weights=None, return_coef=False, conserve_memory=True, delta=None): """ Locally estimated scatterplot smoothing (LOESS). Performs polynomial regression at each data point using the nearest points. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. x_data : array-like, shape (N,), optional The x-values of the measured data. Default is None, which will create an array from -1 to 1 with N points. fraction : float, optional The fraction of N data points to include for the fitting on each point. Default is 0.2. Not used if `total_points` is not None. total_points : int, optional The total number of points to include for the fitting on each point. Default is None, which will use `fraction` * N to determine the number of points. scale : float, optional A scale factor applied to the weighted residuals to control the robustness of the fit. Default is 3.0, as used in [9]_. Note that the original loess procedure in [10]_ used a `scale` of ~4.05. poly_order : int, optional The polynomial order for fitting the baseline. Default is 1. tol : float, optional The exit criteria. Default is 1e-3. max_iter : int, optional The maximum number of iterations. Default is 10. symmetric_weights : bool, optional If False (default), will apply weighting asymmetrically, with residuals < 0 having a weight of 1, according to [9]_. If True, will apply weighting the same for both positive and negative residuals, which is regular LOESS. If `use_threshold` is True, this parameter is ignored. use_threshold : bool, optional If False (default), will compute weights each iteration to perform the robust fitting, which is regular LOESS. If True, will apply a threshold on the data being fit each iteration, based on the maximum values of the data and the fit baseline, as proposed by [11]_, similar to the modpoly and imodpoly techniques. num_std : float, optional The number of standard deviations to include when thresholding. Default is 1, which is the value used for the imodpoly technique. Only used if `use_threshold` is True. use_original : bool, optional If False (default), will compare the baseline of each iteration with the y-values of that iteration [12]_ when choosing minimum values for thresholding. If True, will compare the baseline with the original y-values given by `data` [13]_. Only used if `use_threshold` is True. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. conserve_memory : bool, optional If False, will cache the distance-weighted kernels for each value in `x_data` on the first iteration and reuse them on subsequent iterations to save time. The shape of the array of kernels is (len(`x_data`), `total_points`). If True (default), will recalculate the kernels each iteration, which uses very little memory, but is slower. Can usually set to False unless `x_data` and`total_points` are quite large and the function causes memory issues when cacheing the kernels. If numba is installed, there is no significant time difference since the calculations are sped up. delta : float, optional If `delta` is > 0, will skip all but the last x-value in the range `x_last + delta`, where `x_last` is the last x-value to be fit using weighted least squares, and instead use linear interpolation to calculate the fit for those x-values, which can significantly reduce the calculation time (same behavior as in statsmodels [14]_ and Cleveland's original Fortran lowess implementation [15]_). Fits all x-values if `delta` is <= 0. Default is None, which sets `delta` to `0.01 * (max(x_data) - min(x_data))`. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. Does NOT contain the individual distance-weighted kernels for each x-value. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (N, poly_order + 1) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. If `delta` is > 0, the coefficients for any skipped x-value will all be 0. Raises ------ ValueError Raised if the number of points per window for the fitting is less than `poly_order` + 1 or greater than the total number of points. Notes ----- The iterative, robust, aspect of the fitting can be achieved either through reweighting based on the residuals (the typical usage), or thresholding the fit data based on the residuals, as proposed by [11]_, similar to the modpoly and imodpoly techniques. In baseline literature, this procedure is sometimes called "rbe", meaning "robust baseline estimate". References ---------- .. [9] Ruckstuhl, A.F., et al. Baseline subtraction using robust local regression estimation. J. Quantitative Spectroscopy and Radiative Transfer, 2001, 68, 179-193. .. [10] Cleveland, W. Robust locally weighted regression and smoothing scatterplots. Journal of the American Statistical Association, 1979, 74(368), 829-836. .. [11] Komsta, Ł. Comparison of Several Methods of Chromatographic Baseline Removal with a New Approach Based on Quantile Regression. Chromatographia, 2011, 73, 721-731. .. [12] Gan, F., et al. Baseline correction by improved iterative polynomial fitting with automatic threshold. Chemometrics and Intelligent Laboratory Systems, 2006, 82, 59-65. .. [13] Lieber, C., et al. Automated method for subtraction of fluorescence from biological raman spectra. Applied Spectroscopy, 2003, 57(11), 1363-1367. .. [14] https://github.com/statsmodels/statsmodels. .. [15] https://www.netlib.org/go (lowess.f is the file). """ @_polynomial_wrapper def quant_reg(data, x_data=None, poly_order=2, quantile=0.05, tol=1e-6, max_iter=250, weights=None, eps=None, return_coef=False): """ Approximates the baseline of the data using quantile regression. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. x_data : array-like, shape (N,), optional The x-values of the measured data. Default is None, which will create an array from -1 to 1 with N points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. quantile : float, optional The quantile at which to fit the baseline. Default is 0.05. tol : float, optional The exit criteria. Default is 1e-6. For extreme quantiles (`quantile` < 0.01 or `quantile` > 0.99), may need to use a lower value to get a good fit. max_iter : int, optional The maximum number of iterations. Default is 250. For extreme quantiles (`quantile` < 0.01 or `quantile` > 0.99), may need to use a higher value to ensure convergence. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. eps : float, optional A small value added to the square of the residual to prevent dividing by 0. Default is None, which uses the square of the maximum-absolute-value of the fit each iteration multiplied by 1e-6. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input `x_data` and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray An array containing the calculated tolerance values for each iteration. The length of the array is the number of iterations completed. If the last value in the array is greater than the input `tol` value, then the function did not converge. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Raises ------ ValueError Raised if `quantile` is not between 0 and 1. Notes ----- Application of quantile regression for baseline fitting as described in [16]_. Performs quantile regression using iteratively reweighted least squares (IRLS) as described in [17]_. References ---------- .. [16] Komsta, Ł. Comparison of Several Methods of Chromatographic Baseline Removal with a New Approach Based on Quantile Regression. Chromatographia, 2011, 73, 721-731. .. [17] Schnabel, S., et al. Simultaneous estimation of quantile curves using quantile sheets. AStA Advances in Statistical Analysis, 2013, 97, 77-87. """ @_polynomial_wrapper def goldindec(data, x_data=None, poly_order=2, tol=1e-3, max_iter=250, weights=None, cost_function='asymmetric_indec', peak_ratio=0.5, alpha_factor=0.99, tol_2=1e-3, tol_3=1e-6, max_iter_2=100, return_coef=False): """ Fits a polynomial baseline using a non-quadratic cost function. The non-quadratic cost functions penalize residuals with larger values, giving a more robust fit compared to normal least-squares. Parameters ---------- data : array-like, shape (N,) The y-values of the measured data, with N data points. x_data : array-like, shape (N,), optional The x-values of the measured data. Default is None, which will create an array from -1 to 1 with N points. poly_order : int, optional The polynomial order for fitting the baseline. Default is 2. tol : float, optional The exit criteria for the fitting with a given threshold value. Default is 1e-3. max_iter : int, optional The maximum number of iterations for fitting a threshold value. Default is 250. weights : array-like, shape (N,), optional The weighting array. If None (default), then will be an array with size equal to N and all values set to 1. cost_function : str, optional The non-quadratic cost function to minimize. Unlike :meth:`~.Baseline.penalized_poly`, this function only works with asymmetric cost functions, so the symmetry prefix ('a' or 'asymmetric') is optional (eg. 'indec' and 'a_indec' are the same). Default is 'asymmetric_indec'. Available methods, and their associated reference, are: * 'asymmetric_indec'[18]_ * 'asymmetric_truncated_quadratic'[19]_ * 'asymmetric_huber'[19]_ peak_ratio : float, optional A value between 0 and 1 that designates how many points in the data belong to peaks. Values are valid within ~10% of the actual peak ratio. Default is 0.5. alpha_factor : float, optional A value between 0 and 1 that controls the value of the penalty. Default is 0.99. Typically should not need to change this value. tol_2 : float, optional The exit criteria for the difference between the optimal up-down ratio (number of points above 0 in the residual compared to number of points below 0) and the up-down ratio for a given threshold value. Default is 1e-3. tol_3 : float, optional The exit criteria for the relative change in the threshold value. Default is 1e-6. max_iter_2 : float, optional The number of iterations for iterating between different threshold values. Default is 100. return_coef : bool, optional If True, will convert the polynomial coefficients for the fit baseline to a form that fits the input x_data and return them in the params dictionary. Default is False, since the conversion takes time. Returns ------- baseline : numpy.ndarray, shape (N,) The calculated baseline. params : dict A dictionary with the following items: * 'weights': numpy.ndarray, shape (N,) The weight array used for fitting the data. * 'tol_history': numpy.ndarray, shape (J, K) An array containing the calculated tolerance values for each iteration of both threshold values and fit values. Index 0 are the tolerence values for the difference in up-down ratios, index 1 are the tolerance values for the relative change in the threshold, and indices >= 2 are the tolerance values for each fit. All values that were not used in fitting have values of 0. Shape J is 2 plus the number of iterations for the threshold to converge (related to `max_iter_2`, `tol_2`, `tol_3`), and shape K is the maximum of the number of iterations for the threshold and the maximum number of iterations for all of the fits of the various threshold values (related to `max_iter` and `tol`). * 'threshold' : float The optimal threshold value. Could be used in :meth:`~.Baseline.penalized_poly` for fitting other similar data. * 'coef': numpy.ndarray, shape (poly_order + 1,) Only if `return_coef` is True. The array of polynomial parameters for the baseline, in increasing order. Can be used to create a polynomial using :class:`numpy.polynomial.polynomial.Polynomial`. Raises ------ ValueError Raised if `alpha_factor` or `peak_ratio` are not between 0 and 1, or if the specified cost function is symmetric. References ---------- .. [18] Liu, J., et al. Goldindec: A Novel Algorithm for Raman Spectrum Baseline Correction. Applied Spectroscopy, 2015, 69(7), 834-842. .. [19] Mazet, V., et al. Background removal from spectra by designing and minimising a non-quadratic cost function. Chemometrics and Intelligent Laboratory Systems, 2005, 76(2), 121-133. """