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chore(deps): update dependency scipy to v1.14.0 #11950

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merged 3 commits into from
Jun 27, 2024

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This PR contains the following updates:

Package Change Age Adoption Passing Confidence
scipy (source) ==1.10.0 -> ==1.14.0 age adoption passing confidence
scipy (source) ==1.11.1 -> ==1.14.0 age adoption passing confidence
scipy (source) ==1.13.1 -> ==1.14.0 age adoption passing confidence
scipy (source) ==1.10.1 -> ==1.14.0 age adoption passing confidence

Release Notes

scipy/scipy (scipy)

v1.14.0: SciPy 1.14.0

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SciPy 1.14.0 Release Notes

SciPy 1.14.0 is the culmination of 3 months of hard work. It contains
many new features, numerous bug-fixes, improved test coverage and better
documentation. There have been a number of deprecations and API changes
in this release, which are documented below. All users are encouraged to
upgrade to this release, as there are a large number of bug-fixes and
optimizations. Before upgrading, we recommend that users check that
their own code does not use deprecated SciPy functionality (to do so,
run your code with python -Wd and check for DeprecationWarning s).
Our development attention will now shift to bug-fix releases on the
1.14.x branch, and on adding new features on the main branch.

This release requires Python 3.10+ and NumPy 1.23.5 or greater.

For running on PyPy, PyPy3 6.0+ is required.

Highlights of this release

  • SciPy now supports the new Accelerate library introduced in macOS 13.3, and
    has wheels built against Accelerate for macOS >=14 resulting in significant
    performance improvements for many linear algebra operations.
  • A new method, cobyqa, has been added to scipy.optimize.minimize - this
    is an interface for COBYQA (Constrained Optimization BY Quadratic
    Approximations), a derivative-free optimization solver, designed to
    supersede COBYLA, developed by the Department of Applied Mathematics, The
    Hong Kong Polytechnic University.
  • scipy.sparse.linalg.spsolve_triangular is now more than an order of
    magnitude faster in many cases.

New features

scipy.fft improvements

  • A new function, scipy.fft.prev_fast_len, has been added. This function
    finds the largest composite of FFT radices that is less than the target
    length. It is useful for discarding a minimal number of samples before FFT.

scipy.io improvements

  • wavfile now supports reading and writing of wav files in the RF64
    format, allowing files greater than 4 GB in size to be handled.

scipy.constants improvements

  • Experimental support for the array API standard has been added.

scipy.interpolate improvements

  • scipy.interpolate.Akima1DInterpolator now supports extrapolation via the
    extrapolate argument.

scipy.optimize improvements

  • scipy.optimize.HessianUpdateStrategy now also accepts square arrays for
    init_scale.
  • A new method, cobyqa, has been added to scipy.optimize.minimize - this
    is an interface for COBYQA (Constrained Optimization BY Quadratic
    Approximations), a derivative-free optimization solver, designed to
    supersede COBYLA, developed by the Department of Applied Mathematics, The
    Hong Kong Polytechnic University.
  • There are some performance improvements in
    scipy.optimize.differential_evolution.
  • scipy.optimize.approx_fprime now has linear space complexity.

scipy.signal improvements

  • scipy.signal.minimum_phase has a new argument half, allowing the
    provision of a filter of the same length as the linear-phase FIR filter
    coefficients and with the same magnitude spectrum.

scipy.sparse improvements

  • Sparse arrays now support 1D shapes in COO, DOK and CSR formats.
    These are all the formats we currently intend to support 1D shapes.
    Other sparse array formats raise an exception for 1D input.
  • Sparse array methods min/nanmin/argmin and max analogs now return 1D arrays.
    Results are still COO format sparse arrays for min/nanmin and
    dense np.ndarray for argmin.
  • Sparse matrix and array objects improve their repr and str output.
  • A special case has been added to handle multiplying a dia_array by a
    scalar, which avoids a potentially costly conversion to CSR format.
  • scipy.sparse.csgraph.yen has been added, allowing usage of Yen's K-Shortest
    Paths algorithm on a directed on undirected graph.
  • Addition between DIA-format sparse arrays and matrices is now faster.
  • scipy.sparse.linalg.spsolve_triangular is now more than an order of
    magnitude faster in many cases.

scipy.spatial improvements

  • Rotation supports an alternative "scalar-first" convention of quaternion
    component ordering. It is available via the keyword argument scalar_first
    of from_quat and as_quat methods.
  • Some minor performance improvements for inverting of Rotation objects.

scipy.special improvements

  • Added scipy.special.log_wright_bessel, for calculation of the logarithm of
    Wright's Bessel function.
  • The relative error in scipy.special.hyp2f1 calculations has improved
    substantially.
  • Improved behavior of boxcox, inv_boxcox, boxcox1p, and
    inv_boxcox1p by preventing premature overflow.

scipy.stats improvements

  • A new function scipy.stats.power can be used for simulating the power
    of a hypothesis test with respect to a specified alternative.
  • The Irwin-Hall (AKA Uniform Sum) distribution has been added as
    scipy.stats.irwinhall.
  • Exact p-value calculations of scipy.stats.mannwhitneyu are much faster
    and use less memory.
  • scipy.stats.pearsonr now accepts n-D arrays and computes the statistic
    along a specified axis.
  • scipy.stats.kstat, scipy.stats.kstatvar, and scipy.stats.bartlett
    are faster at performing calculations along an axis of a large n-D array.

Array API Standard Support

Experimental support for array libraries other than NumPy has been added to
existing sub-packages in recent versions of SciPy. Please consider testing
these features by setting an environment variable SCIPY_ARRAY_API=1 and
providing PyTorch, JAX, or CuPy arrays as array arguments.

As of 1.14.0, there is support for

  • scipy.cluster

  • scipy.fft

  • scipy.constants

  • scipy.special: (select functions)

    • scipy.special.log_ndtr
    • scipy.special.ndtr
    • scipy.special.ndtri
    • scipy.special.erf
    • scipy.special.erfc
    • scipy.special.i0
    • scipy.special.i0e
    • scipy.special.i1
    • scipy.special.i1e
    • scipy.special.gammaln
    • scipy.special.gammainc
    • scipy.special.gammaincc
    • scipy.special.logit
    • scipy.special.expit
    • scipy.special.entr
    • scipy.special.rel_entr
    • scipy.special.xlogy
    • scipy.special.chdtrc
  • scipy.stats: (select functions)

    • scipy.stats.describe
    • scipy.stats.moment
    • scipy.stats.skew
    • scipy.stats.kurtosis
    • scipy.stats.kstat
    • scipy.stats.kstatvar
    • scipy.stats.circmean
    • scipy.stats.circvar
    • scipy.stats.circstd
    • scipy.stats.entropy
    • scipy.stats.variation
    • scipy.stats.sem
    • scipy.stats.ttest_1samp
    • scipy.stats.pearsonr
    • scipy.stats.chisquare
    • scipy.stats.skewtest
    • scipy.stats.kurtosistest
    • scipy.stats.normaltest
    • scipy.stats.jarque_bera
    • scipy.stats.bartlett
    • scipy.stats.power_divergence
    • scipy.stats.monte_carlo_test

Deprecated features

  • scipy.stats.gstd, scipy.stats.chisquare, and
    scipy.stats.power_divergence have deprecated support for masked array
    input.
  • scipy.stats.linregress has deprecated support for specifying both samples
    in one argument; x and y are to be provided as separate arguments.
  • The conjtransp method for scipy.sparse.dok_array and
    scipy.sparse.dok_matrix has been deprecated and will be removed in SciPy
    1.16.0.
  • The option quadrature="trapz" in scipy.integrate.quad_vec has been
    deprecated in favour of quadrature="trapezoid" and will be removed in
    SciPy 1.16.0.
  • scipy.special.{comb,perm} have deprecated support for use of exact=True in
    conjunction with non-integral N and/or k.

Backwards incompatible changes

  • Many scipy.stats functions now produce a standardized warning message when
    an input sample is too small (e.g. zero size). Previously, these functions
    may have raised an error, emitted one or more less informative warnings, or
    emitted no warnings. In most cases, returned results are unchanged; in almost
    all cases the correct result is NaN.

Expired deprecations

There is an ongoing effort to follow through on long-standing deprecations.
The following previously deprecated features are affected:

  • Several previously deprecated methods for sparse arrays were removed:
    asfptype, getrow, getcol, get_shape, getmaxprint,
    set_shape, getnnz, and getformat. Additionally, the .A and
    .H attributes were removed.

  • scipy.integrate.{simps,trapz,cumtrapz} have been removed in favour of
    simpson, trapezoid, and cumulative_trapezoid.

  • The tol argument of scipy.sparse.linalg.{bcg,bicstab,cg,cgs,gcrotmk, mres,lgmres,minres,qmr,tfqmr} has been removed in favour of rtol.
    Furthermore, the default value of atol for these functions has changed
    to 0.0.

  • The restrt argument of scipy.sparse.linalg.gmres has been removed in
    favour of restart.

  • The initial_lexsort argument of scipy.stats.kendalltau has been
    removed.

  • The cond and rcond arguments of scipy.linalg.pinv have been
    removed.

  • The even argument of scipy.integrate.simpson has been removed.

  • The turbo and eigvals arguments from scipy.linalg.{eigh,eigvalsh}
    have been removed.

  • The legacy argument of scipy.special.comb has been removed.

  • The hz/nyq argument of signal.{firls, firwin, firwin2, remez} has
    been removed.

  • Objects that weren't part of the public interface but were accessible through
    deprecated submodules have been removed.

  • float128, float96, and object arrays now raise an error in
    scipy.signal.medfilt and scipy.signal.order_filter.

  • scipy.interpolate.interp2d has been replaced by an empty stub (to be
    removed completely in the future).

  • Coinciding with changes to function signatures (e.g. removal of a deprecated
    keyword), we had deprecated positional use of keyword arguments for the
    affected functions, which will now raise an error. Affected functions are:

    • sparse.linalg.{bicg, bicgstab, cg, cgs, gcrotmk, gmres, lgmres, minres, qmr, tfqmr}
    • stats.kendalltau
    • linalg.pinv
    • integrate.simpson
    • linalg.{eigh,eigvalsh}
    • special.comb
    • signal.{firls, firwin, firwin2, remez}

Other changes

  • SciPy now uses C17 as the C standard to build with, instead of C99. The C++
    standard remains C++17.
  • macOS Accelerate, which got a major upgrade in macOS 13.3, is now supported.
    This results in significant performance improvements for linear algebra
    operations, as well as smaller binary wheels.
  • Cross-compilation should be smoother and QEMU or similar is no longer needed
    to run the cross interpreter.
  • Experimental array API support for the JAX backend has been added to several
    parts of SciPy.

Authors

  • Name (commits)
  • h-vetinari (34)
  • Steven Adams (1) +
  • Max Aehle (1) +
  • Ataf Fazledin Ahamed (2) +
  • Luiz Eduardo Amaral (1) +
  • Trinh Quoc Anh (1) +
  • Miguel A. Batalla (7) +
  • Tim Beyer (1) +
  • Andrea Blengino (1) +
  • boatwrong (1)
  • Jake Bowhay (51)
  • Dietrich Brunn (2)
  • Evgeni Burovski (177)
  • Tim Butters (7) +
  • CJ Carey (5)
  • Sean Cheah (46)
  • Lucas Colley (73)
  • Giuseppe "Peppe" Dilillo (1) +
  • DWesl (2)
  • Pieter Eendebak (5)
  • Kenji S Emerson (1) +
  • Jonas Eschle (1)
  • fancidev (2)
  • Anthony Frazier (1) +
  • Ilan Gold (1) +
  • Ralf Gommers (125)
  • Rohit Goswami (28)
  • Ben Greiner (1) +
  • Lorenzo Gualniera (1) +
  • Matt Haberland (260)
  • Shawn Hsu (1) +
  • Budjen Jovan (3) +
  • Jozsef Kutas (1)
  • Eric Larson (3)
  • Gregory R. Lee (4)
  • Philip Loche (1) +
  • Christian Lorentzen (5)
  • Sijo Valayakkad Manikandan (2) +
  • marinelay (2) +
  • Nikolay Mayorov (1)
  • Nicholas McKibben (2)
  • Melissa Weber Mendonça (7)
  • João Mendes (1) +
  • Samuel Le Meur-Diebolt (1) +
  • Tomiță Militaru (2) +
  • Andrew Nelson (35)
  • Lysandros Nikolaou (1)
  • Nick ODell (5) +
  • Jacob Ogle (1) +
  • Pearu Peterson (1)
  • Matti Picus (5)
  • Ilhan Polat (9)
  • pwcnorthrop (3) +
  • Bharat Raghunathan (1)
  • Tom M. Ragonneau (2) +
  • Tyler Reddy (101)
  • Pamphile Roy (18)
  • Atsushi Sakai (9)
  • Daniel Schmitz (5)
  • Julien Schueller (2) +
  • Dan Schult (13)
  • Tomer Sery (7)
  • Scott Shambaugh (4)
  • Tuhin Sharma (1) +
  • Sheila-nk (4)
  • Skylake (1) +
  • Albert Steppi (215)
  • Kai Striega (6)
  • Zhibing Sun (2) +
  • Nimish Telang (1) +
  • toofooboo (1) +
  • tpl2go (1) +
  • Edgar Andrés Margffoy Tuay (44)
  • Andrew Valentine (1)
  • Valerix (1) +
  • Christian Veenhuis (1)
  • void (2) +
  • Warren Weckesser (3)
  • Xuefeng Xu (1)
  • Rory Yorke (1)
  • Xiao Yuan (1)
  • Irwin Zaid (35)
  • Elmar Zander (1) +
  • Zaikun ZHANG (1)
  • ਗਗਨਦੀਪ ਸਿੰਘ (Gagandeep Singh) (4) +

A total of 85 people contributed to this release.
People with a "+" by their names contributed a patch for the first time.
This list of names is automatically generated, and may not be fully complete.

v1.13.1: SciPy 1.13.1

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SciPy 1.13.1 Release Notes

SciPy 1.13.1 is a bug-fix release with no new features
compared to 1.13.0. The version of OpenBLAS shipped with
the PyPI binaries has been increased to 0.3.27.

Authors

  • Name (commits)
  • h-vetinari (1)
  • Jake Bowhay (2)
  • Evgeni Burovski (6)
  • Sean Cheah (2)
  • Lucas Colley (2)
  • DWesl (2)
  • Ralf Gommers (7)
  • Ben Greiner (1) +
  • Matt Haberland (2)
  • Gregory R. Lee (1)
  • Philip Loche (1) +
  • Sijo Valayakkad Manikandan (1) +
  • Matti Picus (1)
  • Tyler Reddy (62)
  • Atsushi Sakai (1)
  • Daniel Schmitz (2)
  • Dan Schult (3)
  • Scott Shambaugh (2)
  • Edgar Andrés Margffoy Tuay (1)

A total of 19 people contributed to this release.
People with a "+" by their names contributed a patch for the first time.
This list of names is automatically generated, and may not be fully complete.

v1.13.0: SciPy 1.13.0

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SciPy 1.13.0 Release Notes

SciPy 1.13.0 is the culmination of 3 months of hard work. This
out-of-band release aims to support NumPy 2.0.0, and is backwards
compatible to NumPy 1.22.4. The version of OpenBLAS used to build
the PyPI wheels has been increased to 0.3.26.dev.

This release requires Python 3.9+ and NumPy 1.22.4 or greater.

For running on PyPy, PyPy3 6.0+ is required.

Highlights of this release

  • Support for NumPy 2.0.0.
  • Interactive examples have been added to the documentation, allowing users
    to run the examples locally on embedded Jupyterlite notebooks in their
    browser.
  • Preliminary 1D array support for the COO and DOK sparse formats.
  • Several scipy.stats functions have gained support for additional
    axis, nan_policy, and keepdims arguments. scipy.stats also
    has several performance and accuracy improvements.

New features

scipy.integrate improvements

  • The terminal attribute of scipy.integrate.solve_ivp events
    callables now additionally accepts integer values to specify a number
    of occurrences required for termination, rather than the previous restriction
    of only accepting a bool value to terminate on the first registered
    event.

scipy.io improvements

  • scipy.io.wavfile.write has improved dtype input validation.

scipy.interpolate improvements

  • The Modified Akima Interpolation has been added to
    interpolate.Akima1DInterpolator, available via the new method
    argument.
  • New method BSpline.insert_knot inserts a knot into a BSpline instance.
    This routine is similar to the module-level scipy.interpolate.insert
    function, and works with the BSpline objects instead of tck tuples.
  • RegularGridInterpolator gained the functionality to compute derivatives
    in place. For instance, RegularGridInterolator((x, y), values, method="cubic")(xi, nu=(1, 1)) evaluates the mixed second derivative,
    :math:\partial^2 / \partial x \partial y at xi.
  • Performance characteristics of tensor-product spline methods of
    RegularGridInterpolator have been changed: evaluations should be
    significantly faster, while construction might be slower. If you experience
    issues with construction times, you may need to experiment with optional
    keyword arguments solver and solver_args. Previous behavior (fast
    construction, slow evaluations) can be obtained via "*_legacy" methods:
    method="cubic_legacy" is exactly equivalent to method="cubic" in
    previous releases. See gh-19633 for details.

scipy.signal improvements

  • Many filter design functions now have improved input validation for the
    sampling frequency (fs).

scipy.sparse improvements

  • coo_array now supports 1D shapes, and has additional 1D support for
    min, max, argmin, and argmax. The DOK format now has
    preliminary 1D support as well, though only supports simple integer indices
    at the time of writing.
  • Experimental support has been added for pydata/sparse array inputs to
    scipy.sparse.csgraph.
  • dok_array and dok_matrix now have proper implementations of
    fromkeys.
  • csr and csc formats now have improved setdiag performance.

scipy.spatial improvements

  • voronoi_plot_2d now draws Voronoi edges to infinity more clearly
    when the aspect ratio is skewed.

scipy.special improvements

  • All Fortran code, namely, AMOS, specfun, and cdflib libraries
    that the majority of special functions depend on, is ported to Cython/C.
  • The function factorialk now also supports faster, approximate
    calculation using exact=False.

scipy.stats improvements

  • scipy.stats.rankdata and scipy.stats.wilcoxon have been vectorized,
    improving their performance and the performance of hypothesis tests that
    depend on them.
  • stats.mannwhitneyu should now be faster due to a vectorized statistic
    calculation, improved caching, improved exploitation of symmetry, and a
    memory reduction. PermutationMethod support was also added.
  • scipy.stats.mood now has nan_policy and keepdims support.
  • scipy.stats.brunnermunzel now has axis and keepdims support.
  • scipy.stats.friedmanchisquare, scipy.stats.shapiro,
    scipy.stats.normaltest, scipy.stats.skewtest,
    scipy.stats.kurtosistest, scipy.stats.f_oneway,
    scipy.stats.alexandergovern, scipy.stats.combine_pvalues, and
    scipy.stats.kstest have gained axis, nan_policy and
    keepdims support.
  • scipy.stats.boxcox_normmax has gained a ymax parameter to allow user
    specification of the maximum value of the transformed data.
  • scipy.stats.vonmises pdf method has been extended to support
    kappa=0. The fit method is also more performant due to the use of
    non-trivial bounds to solve for kappa.
  • High order moment calculations for scipy.stats.powerlaw are now more
    accurate.
  • The fit methods of scipy.stats.gamma (with method='mm') and
    scipy.stats.loglaplace are faster and more reliable.
  • scipy.stats.goodness_of_fit now supports the use of a custom statistic
    provided by the user.
  • scipy.stats.wilcoxon now supports PermutationMethod, enabling
    calculation of accurate p-values in the presence of ties and zeros.
  • scipy.stats.monte_carlo_test now has improved robustness in the face of
    numerical noise.
  • scipy.stats.wasserstein_distance_nd was introduced to compute the
    Wasserstein-1 distance between two N-D discrete distributions.

Deprecated features

  • Complex dtypes in PchipInterpolator and Akima1DInterpolator have
    been deprecated and will raise an error in SciPy 1.15.0. If you are trying
    to use the real components of the passed array, use np.real on y.

Backwards incompatible changes

Other changes

  • The second argument of scipy.stats.moment has been renamed to order
    while maintaining backward compatibility.

Authors

  • Name (commits)
  • h-vetinari (50)
  • acceptacross (1) +
  • Petteri Aimonen (1) +
  • Francis Allanah (2) +
  • Jonas Kock am Brink (1) +
  • anupriyakkumari (12) +
  • Aman Atman (2) +
  • Aaditya Bansal (1) +
  • Christoph Baumgarten (2)
  • Sebastian Berg (4)
  • Nicolas Bloyet (2) +
  • Matt Borland (1)
  • Jonas Bosse (1) +
  • Jake Bowhay (25)
  • Matthew Brett (1)
  • Dietrich Brunn (7)
  • Evgeni Burovski (65)
  • Matthias Bussonnier (4)
  • Tim Butters (1) +
  • Cale (1) +
  • CJ Carey (5)
  • Thomas A Caswell (1)
  • Sean Cheah (44) +
  • Lucas Colley (97)
  • com3dian (1)
  • Gianluca Detommaso (1) +
  • Thomas Duvernay (1)
  • DWesl (2)
  • f380cedric (1) +
  • fancidev (13) +
  • Daniel Garcia (1) +
  • Lukas Geiger (3)
  • Ralf Gommers (147)
  • Matt Haberland (81)
  • Tessa van der Heiden (2) +
  • Shawn Hsu (1) +
  • inky (3) +
  • Jannes Münchmeyer (2) +
  • Aditya Vidyadhar Kamath (2) +
  • Agriya Khetarpal (1) +
  • Andrew Landau (1) +
  • Eric Larson (7)
  • Zhen-Qi Liu (1) +
  • Christian Lorentzen (2)
  • Adam Lugowski (4)
  • m-maggi (6) +
  • Chethin Manage (1) +
  • Ben Mares (1)
  • Chris Markiewicz (1) +
  • Mateusz Sokół (3)
  • Daniel McCloy (1) +
  • Melissa Weber Mendonça (6)
  • Josue Melka (1)
  • Michał Górny (4)
  • Juan Montesinos (1) +
  • Juan F. Montesinos (1) +
  • Takumasa Nakamura (1)
  • Andrew Nelson (27)
  • Praveer Nidamaluri (1)
  • Yagiz Olmez (5) +
  • Dimitri Papadopoulos Orfanos (1)
  • Drew Parsons (1) +
  • Tirth Patel (7)
  • Pearu Peterson (1)
  • Matti Picus (3)
  • Rambaud Pierrick (1) +
  • Ilhan Polat (30)
  • Quentin Barthélemy (1)
  • Tyler Reddy (117)
  • Pamphile Roy (10)
  • Atsushi Sakai (8)
  • Daniel Schmitz (10)
  • Dan Schult (17)
  • Eli Schwartz (4)
  • Stefanie Senger (1) +
  • Scott Shambaugh (2)
  • Kevin Sheppard (2)
  • sidsrinivasan (4) +
  • Samuel St-Jean (1)
  • Albert Steppi (31)
  • Adam J. Stewart (4)
  • Kai Striega (3)
  • Ruikang Sun (1) +
  • Mike Taves (1)
  • Nicolas Tessore (3)
  • Benedict T Thekkel (1) +
  • Will Tirone (4)
  • Jacob Vanderplas (2)
  • Christian Veenhuis (1)
  • Isaac Virshup (2)
  • Ben Wallace (1) +
  • Xuefeng Xu (3)
  • Xiao Yuan (5)
  • Irwin Zaid (8)
  • Elmar Zander (1) +
  • Mathias Zechmeister (1) +

A total of 96 people contributed to this release.
People with a "+" by their names contributed a patch for the first time.
This list of names is automatically generated, and may not be fully complete.

v1.12.0: SciPy 1.12.0

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SciPy 1.12.0 Release Notes

SciPy 1.12.0 is the culmination of 6 months of hard work. It contains
many new features, numerous bug-fixes, improved test coverage and better
documentation. There have been a number of deprecations and API changes
in this release, which are documented below. All users are encouraged to
upgrade to this release, as there are a large number of bug-fixes and
optimizations. Before upgrading, we recommend that users check that
their own code does not use deprecated SciPy functionality (to do so,
run your code with python -Wd and check for DeprecationWarning s).
Our development attention will now shift to bug-fix releases on the
1.12.x branch, and on adding new features on the main branch.

This release requires Python 3.9+ and NumPy 1.22.4 or greater.

For running on PyPy, PyPy3 6.0+ is required.

Highlights of this release

  • Experimental support for the array API standard has been added to part of
    scipy.special, and to all of scipy.fft and scipy.cluster. There are
    likely to be bugs and early feedback for usage with CuPy arrays, PyTorch
    tensors, and other array API compatible libraries is appreciated. Use the
    SCIPY_ARRAY_API environment variable for testing.
  • A new class, ShortTimeFFT, provides a more versatile implementation of the
    short-time Fourier transform (STFT), its inverse (ISTFT) as well as the (cross-)
    spectrogram. It utilizes an improved algorithm for calculating the ISTFT.
  • Several new constructors have been added for sparse arrays, and many operations
    now additionally support sparse arrays, further facilitating the migration
    from sparse matrices.
  • A large portion of the scipy.stats API now has improved support for handling
    NaN values, masked arrays, and more fine-grained shape-handling. The
    accuracy and performance of a number of stats methods have been improved,
    and a number of new statistical tests and distributions have been added.

New features

scipy.cluster improvements

  • Experimental support added for the array API standard; PyTorch tensors,
    CuPy arrays and array API compatible array libraries are now accepted
    (GPU support is limited to functions with pure Python implementations).
    CPU arrays which can be converted to and from NumPy are supported
    module-wide and returned arrays will match the input type.
    This behaviour is enabled by setting the SCIPY_ARRAY_API environment
    variable before importing scipy. This experimental support is still
    under development and likely to contain bugs - testing is very welcome.

scipy.fft improvements

  • Experimental support added for the array API standard; functions which are
    part of the fft array API standard extension module, as well as the
    Fast Hankel Transforms and the basic FFTs which are not in the extension
    module, now accept PyTorch tensors, CuPy arrays and array API compatible
    array libraries. CPU arrays which can be converted to and from NumPy arrays
    are supported module-wide and returned arrays will match the input type.
    This behaviour is enabled by setting the SCIPY_ARRAY_API environment
    variable before importing scipy. This experimental support is still under
    development and likely to contain bugs - testing is very welcome.

scipy.integrate improvements

  • Added scipy.integrate.cumulative_simpson for cumulative quadrature
    from sampled data using Simpson's 1/3 rule.

scipy.interpolate improvements

  • New class NdBSpline represents tensor-product splines in N dimensions.
    This class only knows how to evaluate a tensor product given coefficients
    and knot vectors. This way it generalizes BSpline for 1D data to N-D, and
    parallels NdPPoly (which represents N-D tensor product polynomials).
    Evaluations exploit the localized nature of b-splines.
  • NearestNDInterpolator.__call__ accepts **query_options, which are
    passed through to the KDTree.query call to find nearest neighbors. This
    allows, for instance, to limit the neighbor search distance and parallelize
    the query using the workers keyword.
  • BarycentricInterpolator now allows computing the derivatives.
  • It is now possible to change interpolation values in an existing
    CloughTocher2DInterpolator instance, while also saving the barycentric
    coordinates of interpolation points.

scipy.linalg improvements

  • Access to new low-level LAPACK functions is provided via dtgsyl and
    stgsyl.

scipy.optimize improvements

  • scipy.optimize.isotonic_regression has been added to allow nonparametric isotonic
    regression.
  • scipy.optimize.nnls is rewritten in Python and now implements the so-called
    fnnls or fast nnls, making it more efficient for high-dimensional problems.
  • The result object of scipy.optimize.root and scipy.optimize.root_scalar
    now reports the method used.
  • The callback method of scipy.optimize.differential_evolution can now be
    passed more detailed information via the intermediate_results keyword
    parameter. Also, the evolution strategy now accepts a callable for
    additional customization. The performance of differential_evolution has
    also been improved.
  • scipy.optimize.minimize method Newton-CG now supports functions that
    return sparse Hessian matrices/arrays for the hess parameter and is slightly
    more efficient.
  • scipy.optimize.minimize method BFGS now accepts an initial estimate for the
    inverse of the Hessian, which allows for more efficient workflows in some
    circumstances. The new parameter is hess_inv0.
  • scipy.optimize.minimize methods CG, Newton-CG, and BFGS now accept
    parameters c1 and c2, allowing specification of the Armijo and curvature rule
    parameters, respectively.
  • scipy.optimize.curve_fit performance has improved due to more efficient memoization
    of the callable function.

scipy.signal improvements

  • freqz, freqz_zpk, and group_delay are now more accurate
    when fs has a default value.
  • The new class ShortTimeFFT provides a more versatile implementation of the
    short-time Fourier transform (STFT), its inverse (ISTFT) as well as the (cross-)
    spectrogram. It utilizes an improved algorithm for calculating the ISTFT based on
    dual windows and provides more fine-grained control of the parametrization especially
    in regard to scaling and phase-shift. Functionality was implemented to ease
    working with signal and STFT chunks. A section has been added to the "SciPy User Guide"
    providing algorithmic details. The functions stft, istft and spectrogram
    have been marked as legacy.

scipy.sparse improvements

  • sparse.linalg iterative solvers sparse.linalg.cg,
    sparse.linalg.cgs, sparse.linalg.bicg, sparse.linalg.bicgstab,
    sparse.linalg.gmres, and sparse.linalg.qmr are rewritten in Python.
  • Updated vendored SuperLU version to 6.0.1, along with a few additional
    fixes.
  • Sparse arrays have gained additional constructors: eye_array,
    random_array, block_array, and identity. kron and kronsum
    have been adjusted to additionally support operation on sparse arrays.
  • Sparse matrices now support a transpose with axes=(1, 0), to mirror
    the .T method.
  • LaplacianNd now allows selection of the largest subset of eigenvalues,
    and additionally now supports retrieval of the corresponding eigenvectors.
    The performance of LaplacianNd has also been improved.
  • The performance of dok_matrix and dok_array has been improved,
    and their inheritance behavior should be more robust.
  • hstack, vstack, and block_diag now work with sparse arrays, and
    preserve the input sparse type.
  • A new function, scipy.sparse.linalg.matrix_power, has been added, allowing
    for exponentiation of sparse arrays.

scipy.spatial improvements

  • Two new methods were implemented for spatial.transform.Rotation:
    __pow__ to raise a rotation to integer or fractional power and
    approx_equal to check if two rotations are approximately equal.
  • The method Rotation.align_vectors was extended to solve a constrained
    alignment problem where two vectors are required to be aligned precisely.
    Also when given a single pair of vectors, the algorithm now returns the
    rotation with minimal magnitude, which can be considered as a minor
    backward incompatible change.
  • A new representation for spatial.transform.Rotation called Davenport
    angles is available through from_davenport and as_davenport methods.
  • Performance improvements have been added to distance.hamming and
    distance.correlation.
  • Improved performance of SphericalVoronoi sort_vertices_of_regions
    and two dimensional area calculations.

scipy.special improvements

  • Added scipy.special.stirling2 for computation of Stirling numbers of the
    second kind. Both exact calculation and an asymptotic approximation
    (the default) are supported via exact=True and exact=False (the
    default) respectively.
  • Added scipy.special.betaincc for computation of the complementary
    incomplete Beta function and scipy.special.betainccinv for computation of
    its inverse.
  • Improved precision of scipy.special.betainc and scipy.special.betaincinv.
  • Experimental support added for alternative backends: functions
    scipy.special.log_ndtr, scipy.special.ndtr, scipy.special.ndtri,
    scipy.special.erf, scipy.special.erfc, scipy.special.i0,
    scipy.special.i0e, scipy.special.i1, scipy.special.i1e,
    scipy.special.gammaln, scipy.special.gammainc, scipy.special.gammaincc,
    scipy.special.logit, and scipy.special.expit now accept PyTorch tensors
    and CuPy arrays. These features are still under development and likely to
    contain bugs, so they are disabled by default; enable them by setting a
    SCIPY_ARRAY_API environment variable to 1 before importing scipy.
    Testing is appreciated!

scipy.stats improvements

  • Added scipy.stats.quantile_test, a nonparametric test of whether a
    hypothesized value is the quantile associated with a specified probability.
    The confidence_interval method of the result object gives a confidence
    interval of the quantile.
  • scipy.stats.sampling.FastGeneratorInversion provides a convenient
    interface to fast random sampling via numerical inversion of distribution
    CDFs.
  • scipy.stats.geometric_discrepancy adds geometric/topological discrepancy
    metrics for random samples.
  • scipy.stats.multivariate_normal now has a fit method for fitting
    distribution parameters to data via maximum likelihood estimation.
  • scipy.stats.bws_test performs the Baumgartner-Weiss-Schindler test of
    whether two-samples were drawn from the same distribution.
  • scipy.stats.jf_skew_t implements the Jones and Faddy skew-t distribution.
  • scipy.stats.anderson_ksamp now supports a permutation version of the test
    using the method parameter.
  • The fit methods of scipy.stats.halfcauchy, scipy.stats.halflogistic, and
    scipy.stats.halfnorm are faster and more accurate.
  • scipy.stats.beta entropy accuracy has been improved for extreme values of
    distribution parameters.
  • The accuracy of sf and/or isf methods have been improved for
    several distributions: scipy.stats.burr, scipy.stats.hypsecant,
    scipy.stats.kappa3, scipy.stats.loglaplace, scipy.stats.lognorm,
    scipy.stats.lomax, scipy.stats.pearson3, scipy.stats.rdist, and
    scipy.stats.pareto.
  • The following functions now support parameters axis, nan_policy, and
    keep_dims: scipy.stats.entropy, scipy.stats.differential_entropy,
    scipy.stats.variation, scipy.stats.ansari, scipy.stats.bartlett,
    scipy.stats.levene, scipy.stats.fligner, scipy.stats.circmean,
    scipy.stats.circvar, scipy.stats.circstd, scipy.stats.tmean,
    scipy.stats.tvar, scipy.stats.tstd, scipy.stats.tmin, scipy.stats.tmax,
    and scipy.stats.tsem.
  • The logpdf and fit methods of scipy.stats.skewnorm have been improved.
  • The beta negative binomial distribution is implemented as scipy.stats.betanbinom.
  • Improved performance of scipy.stats.invwishart rvs and logpdf.
  • A source of intermediate overflow in scipy.stats.boxcox_normmax with
    method='mle' has been eliminated, and the returned value of lmbda is
    constrained such that the transformed data will not overflow.
  • scipy.stats.nakagami stats is more accurate and reliable.
  • A source of intermediate overflow in scipy.norminvgauss.pdf has been eliminated.
  • Added support for masked arrays to scipy.stats.circmean, scipy.stats.circvar,
    scipy.stats.circstd, and scipy.stats.entropy.
  • scipy.stats.dirichlet has gained a new covariance (cov) method.
  • Improved accuracy of entropy method of scipy.stats.multivariate_t for large
    degrees of freedom.
  • scipy.stats.loggamma has an improved entropy method.

Deprecated features

  • Error messages have been made clearer for objects that don't exist in the
    public namespace and warnings sharpened for private attributes that are not
    supposed to be imported at all.

  • scipy.signal.cmplx_sort has been deprecated and will be removed in
    SciPy 1.15. A replacement you can use is provided in the deprecation message.

  • Values the the argument initial of scipy.integrate.cumulative_trapezoid
    other than 0 and None are now deprecated.

  • scipy.stats.rvs_ratio_uniforms is deprecated in favour of
    scipy.stats.sampling.RatioUniforms

  • scipy.integrate.quadrature and scipy.integrate.romberg have been
    deprecated due to accuracy issues and interface shortcomings. They will
    be removed in SciPy 1.15. Please use scipy.integrate.quad instead.

  • Coinciding with upcoming changes to function signatures (e.g. removal of a
    deprecated keyword), we are deprecating positional use of keyword arguments
    for the affected functions, which will raise an error starting with
    SciPy 1.14. In some cases, this has delayed the originally announced
    removal date, to give time to respond to the second part of the deprecation.
    Affected functions are:

    • linalg.{eigh, eigvalsh, pinv}
    • integrate.simpson
    • signal.{firls, firwin, firwin2, remez}
    • sparse.linalg.{bicg, bicgstab, cg, cgs, gcrotmk, gmres, lgmres, minres, qmr, tfqmr}
    • special.comb
    • stats.kendalltau
  • All wavelet functions have been deprecated, as PyWavelets provides suitable
    implementations; affected functions are: signal.{daub, qmf, cascade, morlet, morlet2, ricker, cwt}

  • scipy.integrate.trapz, scipy.integrate.cumtrapz, and scipy.integrate.simps have
    been deprecated in favour of scipy.integrate.trapezoid, scipy.integrate.cumulative_trapezoid,
    and scipy.integrate.simpson respectively and will be removed in SciPy 1.14.

  • The tol argument of scipy.sparse.linalg.{bcg,bicstab,cg,cgs,gcrotmk,gmres,lgmres,minres,qmr,tfqmr}
    is now deprecated in favour of rtol and will be removed in SciPy 1.14.
    Furthermore, the default value of atol for these functions is due
    to change to 0.0 in SciPy 1.14.

Expired Deprecations

There is an ongoing effort to follow through on long-standing deprecations.
The following previously deprecated features are affected:

  • The centered keyword of scipy.stats.qmc.LatinHypercube has been removed.
    Use scrambled=False instead of centered=True.
  • scipy.stats.binom_test has been removed in favour of scipy.stats.binomtest.
  • In scipy.stats.iqr, the use of scale='raw' has been removed in favour
    of scale=1.

Backwards incompatible changes

Other changes

  • The arguments used to compile and link SciPy are now available via
    show_config.

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v1.11.4: SciPy 1.11.4

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SciPy 1.11.4 Release Notes

SciPy 1.11.4 is a bug-fix release with no new features
compared to 1.11.3.

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v1.11.3: SciPy 1.11.3

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SciPy 1.11.3 Release Notes

SciPy 1.11.3 is a bug-fix release with no new features
compared to 1.11.2.

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v1.11.2: SciPy 1.11.2

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SciPy 1.11.2 Release Notes

SciPy 1.11.2 is a bug-fix release with no new features
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v1.11.1: SciPy 1.11.1

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SciPy 1.11.1 Release Notes

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v1.11.0: SciPy 1.11.0

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SciPy 1.11.0 Release Notes

SciPy 1.11.0 is the culmination of 6 months of hard work. It contains
many new features, numerous bug-fixes, improved test coverage and better
documentation. There have been a number of deprecations and API changes
in this release, which are documented below. All users are encouraged to
upgrade to this release, as there are a large number of bug-fixes and
optimizations. Before upgrading, we recommend that users check that
their own code does not use deprecated SciPy functionality (to do so,
run your code with python -Wd and check for DeprecationWarning s).
Our development attention will now shift to bug-fix releases on the
1.11.x branch, and on adding new features on the main branch.

This release requires Python 3.9+ and NumPy 1.21.6 or greater.

For running on PyPy, PyPy3 6.0+ is required.

Highlights of this release

  • Several scipy.sparse array API improvements, including sparse.sparray, a new
    public base class distinct from the older sparse.spmatrix class,
    proper 64-bit index support, and numerous deprecations paving the way to a
    modern sparse array experience.
  • scipy.stats added tools for survival analysis, multiple hypothesis testing,
    sensitivity analysis, and working with censored data.
  • A new function was added for quasi-Monte Carlo integration, and linear
    algebra functions det and lu now accept nD-arrays.
  • An axes argument was added broadly to ndimage functions, facilitating
    analysis of stacked image data.

New features

scipy.integrate improvements

  • Added scipy.integrate.qmc_quad for quasi-Monte Carlo integration.
  • For an even number of points, scipy.integrate.simpson now calculates
    a parabolic segment over the last three points which gives improved
    accuracy over the previous implementation.

scipy.cluster improvements

  • disjoint_set has a new method subset_size for providing the size
    of a particular subset.

scipy.constants improvements

  • The quetta, ronna, ronto, and quecto SI prefixes were added.

scipy.linalg improvements

  • scipy.linalg.det is improved and now accepts nD-arrays.
  • scipy.linalg.lu is improved and now accepts nD-arrays. With the new
    p_indices switch the output permutation argument can be 1D (n,)
    permutation index instead of the full (n, n) array.

scipy.ndimage improvements

  • axes argument was added to rank_filter, percentile_filter,
    median_filter, uniform_filter, minimum_filter,
    maximum_filter, and gaussian_filter, which can be useful for
    processing stacks of image data.

scipy.optimize improvements

  • scipy.optimize.linprog now passes unrecognized options directly to HiGHS.
  • scipy.optimize.root_scalar now uses Newton's method to be used without
    providing fprime and the secant method to be used without a second
    guess.
  • scipy.optimize.lsq_linear now accepts bounds arguments of type
    scipy.optimize.Bounds.
  • scipy.optimize.minimize method='cobyla' now supports simple bound
    constraints.
  • Users can opt into a new callback interface for most methods of
    scipy.optimize.minimize: If the provided callback callable accepts
    a single keyword argument, intermediate_result, scipy.optimize.minimize
    now passes both the current solution and the optimal value of the objective
    function to the callback as an instance of scipy.optimize.OptimizeResult.
    It also allows the user to terminate optimization by raising a
    StopIteration exception from the callback function.
    scipy.optimize.minimize will return normally, and the latest solution
    information is provided in the result object.
  • scipy.optimize.curve_fit now supports an optional nan_policy argument.
  • scipy.optimize.shgo now has parallelization with the workers argument,
    symmetry arguments that can improve performance, class-based design to
    improve usability, and generally improved performance.

scipy.signal improvements

  • istft has an improved warning message when the NOLA condition fails.

scipy.sparse improvements

  • A new public base class scipy.sparse.sparray was introduced, allowing further
    extension of the sparse array API (such as the support for 1-dimensional
    sparse arrays) without breaking backwards compatibility.
    isinstance(x, scipy.sparse.sparray) to select the new sparse array classes,
    while isinstance(x, scipy.sparse.spmatrix) selects only the old sparse
    matrix classes.
  • Division of sparse arrays by a dense array now returns sparse arrays.
  • scipy.sparse.isspmatrix now only returns True for the sparse matrices instances.
    scipy.sparse.issparse now has to be used instead to check for instances of sparse
    arrays or instances of sparse matrices.
  • Sparse arrays constructed with int64 indices will no longer automatically
    downcast to int32.
  • The argmin and argmax methods now return the correct result when explicit
    zeros are present.

scipy.sparse.linalg improvements

  • dividing LinearOperator by a number now returns a
    _ScaledLinearOperator
  • LinearOperator now supports right multiplication by arrays
  • lobpcg should be more efficient following removal of an extraneous
    QR decomposition.

scipy.spatial improvements

  • Usage of new C++ backend for additional distance metrics, the majority of
    which will see substantial performance improvements, though a few minor
    regressions are known. These are focused on distances between boolean
    arrays.

scipy.special improvements

  • The factorial functions factorial, factorial2 and factorialk
    were made consistent in their behavior (in terms of dimensionality,
    errors etc.). Additionally, factorial2 can now handle arrays with
    exact=True, and factorialk can handle arrays.

scipy.stats improvements

New Features

  • scipy.stats.sobol_indices, a method to compute Sobol' sensitivity indices.
  • scipy.stats.dunnett, which performs Dunnett's test of the means of multiple
    experimental groups against the mean of a control group.
  • scipy.stats.ecdf for computing the empirical CDF and complementary
    CDF (survival function / SF) from uncensored or right-censored data. This
    function is also useful for survival analysis / Kaplan-Meier estimation.
  • scipy.stats.logrank to compare survival functions underlying samples.
  • scipy.stats.false_discovery_control for adjusting p-values to control the
    false discovery rate of multiple hypothesis tests using the
    Benjamini-Hochberg or Benjamini-Yekutieli procedures.
  • scipy.stats.CensoredData to represent censored data. It can be used as
    input to the fit method of univariate distributions and to the new
    ecdf function.
  • Filliben's goodness of fit test as method='Filliben' of
    scipy.stats.goodness_of_fit.
  • scipy.stats.ttest_ind has a new method, confidence_interval for
    computing a confidence interval of the difference between means.
  • scipy.stats.MonteCarloMethod, scipy.stats.PermutationMethod, and
    scipy.stats.BootstrapMethod are new classes to configure resampling and/or
    Monte Carlo versions of hypothesis tests. They can currently be used with
    scipy.stats.pearsonr.

Statistical Distributions

  • Added the von-Mises Fisher distribution as scipy.stats.vonmises_fisher.
    This distribution is the most common analogue of the normal distribution
    on the unit sphere.

  • Added the relativistic Breit-Wigner distribution as
    scipy.stats.rel_breitwigner.
    It is used in high energy physics to model resonances.

  • Added the Dirichlet multinomial distribution as
    scipy.stats.dirichlet_multinomial.

  • Improved the speed and precision of several univariate statistical
    distributions.

    • scipy.stats.anglit sf
    • scipy.stats.beta entropy
    • scipy.stats.betaprime cdf, sf, ppf
    • scipy.stats.chi entropy
    • scipy.stats.chi2 entropy
    • scipy.stats.dgamma entropy, cdf, sf, ppf, and isf
    • scipy.stats.dweibull entropy, sf, and isf
    • scipy.stats.exponweib sf and isf
    • scipy.stats.f entropy
    • scipy.stats.foldcauchy sf
    • scipy.stats.foldnorm cdf and sf
    • scipy.stats.gamma entropy
    • scipy.stats.genexpon ppf, isf, rvs
    • scipy.stats.gengamma entropy
    • scipy.stats.geom entropy
    • scipy.stats.genlogistic entropy, logcdf, sf, ppf,
      and isf
    • scipy.stats.genhyperbolic cdf and sf
    • scipy.stats.gibrat sf and isf
    • scipy.stats.gompertz entropy, sf. and isf
    • scipy.stats.halflogistic sf, and isf
    • scipy.stats.halfcauchy sf and isf
    • scipy.stats.halfnorm cdf, sf, and isf
    • scipy.stats.invgamma entropy
    • scipy.stats.invgauss entropy
    • scipy.stats.johnsonsb pdf, cdf, sf, ppf, and isf
    • scipy.stats.johnsonsu pdf, sf, isf, and stats

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