GCXS
Bases: SparseArray
, NDArrayOperatorsMixin
A sparse multidimensional array.
This is stored in GCXS format, a generalization of the GCRS/GCCS formats from Efficient storage scheme for n-dimensional sparse array: GCRS/GCCS. GCXS generalizes the CRS/CCS sparse matrix formats.
For arrays with ndim == 2, GCXS is the same CSR/CSC. For arrays with ndim >2, any combination of axes can be compressed, significantly reducing storage.
GCXS consists of 3 arrays. Let the 3 arrays be RO, CO and VL. The first element of array RO is the integer 0 and later elements are the number of cumulative non-zero elements in each row for GCRS, column for GCCS. CO stores column indexes of non-zero elements at each row for GCRS, column for GCCS. VL stores the values of the non-zero array elements.
The superiority of the GCRS/GCCS over traditional (CRS/CCS) is shown by both theoretical analysis and experimental results, outlined in the linked research paper.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
arg
|
tuple(data, indices, indptr)
|
A tuple of arrays holding the data, indices, and index pointers for the nonzero values of the array. |
required |
shape
|
tuple[int](ndim)
|
The shape of the array. |
None
|
compressed_axes
|
Iterable[int]
|
The axes to compress. |
None
|
prune
|
bool_
|
A flag indicating whether or not we should prune any fill-values present in the data array. |
False
|
fill_value
|
The fill value for this array. |
None
|
Attributes:
Name | Type | Description |
---|---|---|
data |
ndarray(nnz)
|
An array holding the nonzero values corresponding to |
indices |
ndarray(nnz)
|
An array holding the coordinates of every nonzero element along uncompressed dimensions. |
indptr |
ndarray
|
An array holding the cumulative sums of the nonzeros along the compressed dimensions. |
shape |
tuple[int](ndim)
|
The dimensions of this array. |
See Also
sparse.DOK
: A mostly write-only sparse array.
Source code in sparse/numba_backend/_compressed/compressed.py
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|
Attributes
device
property
ndim
property
The number of dimensions of this array.
Returns:
Type | Description |
---|---|
int
|
The number of dimensions of this array. |
See Also
sparse.DOK.ndim
: Equivalent property forsparse.DOK
arrays.numpy.ndarray.ndim
: Numpy equivalent property.
Examples:
>>> from sparse import COO
>>> import numpy as np
>>> x = np.random.rand(1, 2, 3, 1, 2)
>>> s = COO.from_numpy(x)
>>> s.ndim
5
>>> s.ndim == x.ndim
True
size
property
The number of all elements (including zeros) in this array.
Returns:
Type | Description |
---|---|
int
|
The number of elements. |
See Also
numpy.ndarray.size
: Numpy equivalent property.
Examples:
>>> from sparse import COO
>>> import numpy as np
>>> x = np.zeros((10, 10))
>>> s = COO.from_numpy(x)
>>> s.size
100
density
property
The ratio of nonzero to all elements in this array.
Returns:
Type | Description |
---|---|
float
|
The ratio of nonzero to all elements. |
See Also
sparse.COO.size
: Number of elements.sparse.COO.nnz
: Number of nonzero elements.
Examples:
>>> import numpy as np
>>> from sparse import COO
>>> x = np.zeros((8, 8))
>>> x[0, :] = 1
>>> s = COO.from_numpy(x)
>>> s.density
0.125
amax = max
class-attribute
instance-attribute
amin = min
class-attribute
instance-attribute
round_ = round
class-attribute
instance-attribute
real
property
The real part of the array.
Examples:
>>> from sparse import COO
>>> x = COO.from_numpy([1 + 0j, 0 + 1j])
>>> x.real.todense()
array([1., 0.])
>>> x.real.dtype
dtype('float64')
Returns:
Name | Type | Description |
---|---|---|
out |
SparseArray
|
The real component of the array elements. If the array dtype is real, the dtype of the array is used for the output. If the array is complex, the output dtype is float. |
See Also
numpy.ndarray.real
: NumPy equivalent attribute.numpy.real
: NumPy equivalent function.
imag
property
The imaginary part of the array.
Examples:
>>> from sparse import COO
>>> x = COO.from_numpy([1 + 0j, 0 + 1j])
>>> x.imag.todense()
array([0., 1.])
>>> x.imag.dtype
dtype('float64')
Returns:
Name | Type | Description |
---|---|---|
out |
SparseArray
|
The imaginary component of the array elements. If the array dtype is real, the dtype of the array is used for the output. If the array is complex, the output dtype is float. |
See Also
numpy.ndarray.imag
: NumPy equivalent attribute.numpy.imag
: NumPy equivalent function.
shape = shape
instance-attribute
fill_value = self.data.dtype.type(fill_value)
instance-attribute
dtype
property
The datatype of this array.
Returns:
Type | Description |
---|---|
dtype
|
The datatype of this array. |
See Also
numpy.ndarray.dtype
: Numpy equivalent property.scipy.sparse.csr_matrix.dtype
: Scipy equivalent property.
nnz
property
The number of nonzero elements in this array.
Returns:
Type | Description |
---|---|
int
|
The number of nonzero elements in this array. |
See Also
sparse.COO.nnz
: Equivalentsparse.COO
array property.sparse.DOK.nnz
: Equivalentsparse.DOK
array property.numpy.count_nonzero
: A similar Numpy function.scipy.sparse.coo_matrix.nnz
: The Scipy equivalent property.
format
property
The storage format of this array.
Returns:
Type | Description |
---|---|
str
|
The storage format of this array. |
See Also
scipy.sparse.dok_matrix.format
: The Scipy equivalent property.
Examples:
>>> import sparse
>>> s = sparse.random((5, 5), density=0.2, format="dok")
>>> s.format
'dok'
>>> t = sparse.random((5, 5), density=0.2, format="coo")
>>> t.format
'coo'
nbytes
property
The number of bytes taken up by this object. Note that for small arrays, this may undercount the number of bytes due to the large constant overhead.
Returns:
Type | Description |
---|---|
int
|
The approximate bytes of memory taken by this object. |
See Also
numpy.ndarray.nbytes
: The equivalent Numpy property.
T
property
mT
property
compressed_axes
property
Functions
to_device(device, /, *, stream=None)
Source code in sparse/numba_backend/_sparse_array.py
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|
reduce(method, axis=(0,), keepdims=False, **kwargs)
Performs a reduction operation on this array.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
method
|
ufunc
|
The method to use for performing the reduction. |
required |
axis
|
Union[int, Iterable[int]]
|
The axes along which to perform the reduction. Uses all axes by default. |
(0,)
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
**kwargs
|
dict
|
Any extra arguments to pass to the reduction operation. |
{}
|
See Also
numpy.ufunc.reduce
: A similar Numpy method.sparse.COO.reduce
: This method implemented on COO arrays.sparse.GCXS.reduce
: This method implemented on GCXS arrays.
Source code in sparse/numba_backend/_sparse_array.py
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|
sum(axis=None, keepdims=False, dtype=None, out=None)
Performs a sum operation along the given axes. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to sum. Uses all axes by default. |
None
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
dtype
|
dtype
|
The data type of the output array. |
None
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.sum
: Equivalent numpy function.scipy.sparse.coo_matrix.sum
: Equivalent Scipy function.
Source code in sparse/numba_backend/_sparse_array.py
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|
max(axis=None, keepdims=False, out=None)
Maximize along the given axes. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to maximize. Uses all axes by default. |
None
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
out
|
dtype
|
The data type of the output array. |
None
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.max
: Equivalent numpy function.scipy.sparse.coo_matrix.max
: Equivalent Scipy function.
Source code in sparse/numba_backend/_sparse_array.py
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|
any(axis=None, keepdims=False, out=None)
See if any values along array are True
. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to minimize. Uses all axes by default. |
None
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.any
: Equivalent numpy function.
Source code in sparse/numba_backend/_sparse_array.py
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|
all(axis=None, keepdims=False, out=None)
See if all values in an array are True
. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to minimize. Uses all axes by default. |
None
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.all
: Equivalent numpy function.
Source code in sparse/numba_backend/_sparse_array.py
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|
min(axis=None, keepdims=False, out=None)
Minimize along the given axes. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to minimize. Uses all axes by default. |
None
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
out
|
dtype
|
The data type of the output array. |
None
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.min
: Equivalent numpy function.scipy.sparse.coo_matrix.min
: Equivalent Scipy function.
Source code in sparse/numba_backend/_sparse_array.py
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|
prod(axis=None, keepdims=False, dtype=None, out=None)
Performs a product operation along the given axes. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to multiply. Uses all axes by default. |
None
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
dtype
|
dtype
|
The data type of the output array. |
None
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.prod
: Equivalent numpy function.
Source code in sparse/numba_backend/_sparse_array.py
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round(decimals=0, out=None)
Evenly round to the given number of decimals.
See Also
numpy.round
: NumPy equivalent ufunc.sparse.elemwise
: Apply an arbitrary element-wise function to one or two arguments.
Source code in sparse/numba_backend/_sparse_array.py
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|
clip(min=None, max=None, out=None)
Clip (limit) the values in the array.
Return an array whose values are limited to [min, max]
. One of min
or max must be given.
See Also
- sparse.clip : For full documentation and more details.
numpy.clip
: Equivalent NumPy function.
Source code in sparse/numba_backend/_sparse_array.py
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astype(dtype, casting='unsafe', copy=True)
Copy of the array, cast to a specified type.
See Also
scipy.sparse.coo_matrix.astype
: SciPy sparse equivalent functionnumpy.ndarray.astype
: NumPy equivalent ufunc.sparse.elemwise
: Apply an arbitrary element-wise function to one or two arguments.
Source code in sparse/numba_backend/_sparse_array.py
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|
mean(axis=None, keepdims=False, dtype=None, out=None)
Compute the mean along the given axes. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to compute the mean. Uses all axes by default. |
None
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
dtype
|
dtype
|
The data type of the output array. |
None
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.ndarray.mean
: Equivalent numpy method.scipy.sparse.coo_matrix.mean
: Equivalent Scipy method.
Notes
- The
out
parameter is provided just for compatibility with Numpy and isn't actually supported.
Examples:
You can use sparse.COO.mean
to compute the mean of an array across any
dimension.
>>> from sparse import COO
>>> x = np.array([[1, 2, 0, 0], [0, 1, 0, 0]], dtype="i8")
>>> s = COO.from_numpy(x)
>>> s2 = s.mean(axis=1)
>>> s2.todense()
array([0.5, 1.5, 0., 0.])
You can also use the keepdims
argument to keep the dimensions
after the mean.
>>> s3 = s.mean(axis=0, keepdims=True)
>>> s3.shape
(1, 4)
You can pass in an output datatype, if needed.
>>> s4 = s.mean(axis=0, dtype=np.float16)
>>> s4.dtype
dtype('float16')
By default, this reduces the array down to one number, computing the mean along all axes.
>>> s.mean()
np.float64(0.5)
Source code in sparse/numba_backend/_sparse_array.py
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var(axis=None, dtype=None, out=None, ddof=0, keepdims=False)
Compute the variance along the given axes. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to compute the variance. Uses all axes by default. |
None
|
dtype
|
dtype
|
The output datatype. |
None
|
out
|
SparseArray
|
The array to write the output to. |
None
|
ddof
|
int
|
The degrees of freedom. |
0
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.ndarray.var
: Equivalent numpy method.
Examples:
You can use sparse.COO.var
to compute the variance of an array across any
dimension.
>>> from sparse import COO
>>> x = np.array([[1, 2, 0, 0], [0, 1, 0, 0]], dtype="i8")
>>> s = COO.from_numpy(x)
>>> s2 = s.var(axis=1)
>>> s2.todense()
array([0.6875, 0.1875])
You can also use the keepdims
argument to keep the dimensions
after the variance.
>>> s3 = s.var(axis=0, keepdims=True)
>>> s3.shape
(1, 4)
You can pass in an output datatype, if needed.
>>> s4 = s.var(axis=0, dtype=np.float16)
>>> s4.dtype
dtype('float16')
By default, this reduces the array down to one number, computing the variance along all axes.
>>> s.var()
np.float64(0.5)
Source code in sparse/numba_backend/_sparse_array.py
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std(axis=None, dtype=None, out=None, ddof=0, keepdims=False)
Compute the standard deviation along the given axes. Uses all axes by default.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axis
|
Union[int, Iterable[int]]
|
The axes along which to compute the standard deviation. Uses all axes by default. |
None
|
dtype
|
dtype
|
The output datatype. |
None
|
out
|
SparseArray
|
The array to write the output to. |
None
|
ddof
|
int
|
The degrees of freedom. |
0
|
keepdims
|
bool_
|
Whether or not to keep the dimensions of the original array. |
False
|
Returns:
Type | Description |
---|---|
SparseArray
|
The reduced output sparse array. |
See Also
numpy.ndarray.std
: Equivalent numpy method.
Examples:
You can use sparse.COO.std
to compute the standard deviation of an array
across any dimension.
>>> from sparse import COO
>>> x = np.array([[1, 2, 0, 0], [0, 1, 0, 0]], dtype="i8")
>>> s = COO.from_numpy(x)
>>> s2 = s.std(axis=1)
>>> s2.todense()
array([0.8291562, 0.4330127])
You can also use the keepdims
argument to keep the dimensions
after the standard deviation.
>>> s3 = s.std(axis=0, keepdims=True)
>>> s3.shape
(1, 4)
You can pass in an output datatype, if needed.
>>> s4 = s.std(axis=0, dtype=np.float16)
>>> s4.dtype
dtype('float16')
By default, this reduces the array down to one number, computing the standard deviation along all axes.
>>> s.std()
0.7071067811865476
Source code in sparse/numba_backend/_sparse_array.py
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conj()
Return the complex conjugate, element-wise.
The complex conjugate of a complex number is obtained by changing the sign of its imaginary part.
Examples:
>>> from sparse import COO
>>> x = COO.from_numpy([1 + 2j, 2 - 1j])
>>> res = x.conj()
>>> res.todense()
array([1.-2.j, 2.+1.j])
>>> res.dtype
dtype('complex128')
Returns:
Name | Type | Description |
---|---|---|
out |
SparseArray
|
The complex conjugate, with same dtype as the input. |
See Also
numpy.ndarray.conj
: NumPy equivalent method.numpy.conj
: NumPy equivalent function.
Source code in sparse/numba_backend/_sparse_array.py
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copy(deep=True)
Return a copy of the array.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
deep
|
boolean
|
If True (default), the internal coords and data arrays are also
copied. Set to |
True
|
Source code in sparse/numba_backend/_compressed/compressed.py
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|
from_numpy(x, compressed_axes=None, fill_value=None, idx_dtype=None)
classmethod
Source code in sparse/numba_backend/_compressed/compressed.py
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|
from_coo(x, compressed_axes=None, idx_dtype=None)
classmethod
Source code in sparse/numba_backend/_compressed/compressed.py
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from_scipy_sparse(x, /, *, fill_value=None)
classmethod
Source code in sparse/numba_backend/_compressed/compressed.py
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|
from_iter(x, shape=None, compressed_axes=None, fill_value=None, idx_dtype=None)
classmethod
Source code in sparse/numba_backend/_compressed/compressed.py
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|
change_compressed_axes(new_compressed_axes)
Returns a new array with specified compressed axes. This operation is similar to converting a scipy.sparse.csc_matrix to a scipy.sparse.csr_matrix.
Returns:
Type | Description |
---|---|
GCXS
|
A new instance of the input array with compression along the specified dimensions. |
Source code in sparse/numba_backend/_compressed/compressed.py
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|
tocoo()
Convert this sparse.GCXS
array to a sparse.COO
.
Returns:
Type | Description |
---|---|
COO
|
The converted COO array. |
Source code in sparse/numba_backend/_compressed/compressed.py
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|
todense()
Convert this sparse.GCXS
array to a dense numpy.ndarray
. Note that
this may take a large amount of memory if the sparse.GCXS
object's shape
is large.
Returns:
Type | Description |
---|---|
ndarray
|
The converted dense array. |
See Also
sparse.DOK.todense
: Equivalentsparse.DOK
array method.sparse.COO.todense
: Equivalentsparse.COO
array method.scipy.sparse.coo_matrix.todense
: Equivalent Scipy method.
Source code in sparse/numba_backend/_compressed/compressed.py
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|
todok()
Source code in sparse/numba_backend/_compressed/compressed.py
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|
to_scipy_sparse(accept_fv=None)
Converts this sparse.GCXS
object into a scipy.sparse.csr_matrix
or scipy.sparse.csc_matrix
.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
accept_fv
|
scalar or list of scalar
|
The list of accepted fill-values. The default accepts only zero. |
None
|
Returns:
Type | Description |
---|---|
csr_matrix or csc_matrix
|
The converted Scipy sparse matrix. |
Raises:
Type | Description |
---|---|
ValueError
|
If the array is not two-dimensional. |
ValueError
|
If all the array doesn't zero fill-values. |
Source code in sparse/numba_backend/_compressed/compressed.py
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|
asformat(format, **kwargs)
Convert this sparse array to a given format.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
format
|
str
|
A format string. |
required |
Returns:
Name | Type | Description |
---|---|---|
out |
SparseArray
|
The converted array. |
Raises:
Type | Description |
---|---|
NotImplementedError
|
If the format isn't supported. |
Source code in sparse/numba_backend/_compressed/compressed.py
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|
maybe_densify(max_size=1000, min_density=0.25)
Converts this sparse.GCXS
array to a numpy.ndarray
if not too
costly.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
max_size
|
int
|
Maximum number of elements in output |
1000
|
min_density
|
float
|
Minimum density of output |
0.25
|
Returns:
Type | Description |
---|---|
ndarray
|
The dense array. |
See Also
- sparse.GCXS.todense: Converts to Numpy function without checking the cost.
- sparse.COO.maybe_densify: The equivalent COO function.
Raises:
Type | Description |
---|---|
ValueError
|
If the returned array would be too large. |
Source code in sparse/numba_backend/_compressed/compressed.py
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|
flatten(order='C')
Returns a new sparse.GCXS
array that is a flattened version of this array.
Returns:
Type | Description |
---|---|
GCXS
|
The flattened output array. |
Notes
The order
parameter is provided just for compatibility with
Numpy and isn't actually supported.
Source code in sparse/numba_backend/_compressed/compressed.py
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|
reshape(shape, order='C', compressed_axes=None)
Returns a new sparse.GCXS
array that is a reshaped version of this array.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
shape
|
tuple[int]
|
The desired shape of the output array. |
required |
compressed_axes
|
Iterable[int]
|
The axes to compress to store the array. Finds the most efficient storage by default. |
None
|
Returns:
Type | Description |
---|---|
GCXS
|
The reshaped output array. |
See Also
numpy.ndarray.reshape
: The equivalent Numpy function.- sparse.COO.reshape : The equivalent COO function.
Notes
The order
parameter is provided just for compatibility with
Numpy and isn't actually supported.
Source code in sparse/numba_backend/_compressed/compressed.py
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|
transpose(axes=None, compressed_axes=None)
Returns a new array which has the order of the axes switched.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
axes
|
Iterable[int]
|
The new order of the axes compared to the previous one. Reverses the axes by default. |
None
|
compressed_axes
|
Iterable[int]
|
The axes to compress to store the array. Finds the most efficient storage by default. |
None
|
Returns:
Type | Description |
---|---|
GCXS
|
The new array with the axes in the desired order. |
See Also
sparse.GCXS.T
: A quick property to reverse the order of the axes.numpy.ndarray.transpose
: Numpy equivalent function.
Source code in sparse/numba_backend/_compressed/compressed.py
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|
dot(other)
Performs the equivalent of x.dot(y)
for sparse.GCXS
.
Parameters:
Name | Type | Description | Default |
---|---|---|---|
other
|
Union[GCXS, COO, ndarray, spmatrix]
|
The second operand of the dot product operation. |
required |
Returns:
Type | Description |
---|---|
{GCXS, ndarray}
|
The result of the dot product. If the result turns out to be dense, then a dense array is returned, otherwise, a sparse array. |
Raises:
Type | Description |
---|---|
ValueError
|
If all arguments don't have zero fill-values. |
See Also
sparse.dot
: Equivalent function for two arguments.numpy.dot
: Numpy equivalent function.scipy.sparse.coo_matrix.dot
: Scipy equivalent function.
Source code in sparse/numba_backend/_compressed/compressed.py
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|
isinf()
Source code in sparse/numba_backend/_compressed/compressed.py
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|
isnan()
Source code in sparse/numba_backend/_compressed/compressed.py
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|