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/dports/devel/py-dask/dask-2021.11.2/docs/source/
H A Ddelayed-best-practices.rst31 then call ``dask.compute`` only at the end. It is ok to call ``dask.compute``
40 | # Avoid calling compute repeatedly | # Collect many calls for one compute …
61 | .. code-block:: python | .. code-block:: python |
73 .. code-block:: python
110 to pass the output to something that eventually calls compute.
115 | .. code-block:: python | .. code-block:: python |
138 | .. code-block:: python | .. code-block:: python |
164 | dask.compute(f(filenames)) | dask.compute(f(filenames)) |
194 .. code-block:: python
265 .. code-block:: python
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H A Darray-assignment.rst34 .. code-block:: python
41 >>> x.compute()
45 >>> x.compute()
57 .. code-block:: python
62 >>> print(x.compute())
66 >>> print(x.compute())
70 >>> print(x.compute())
78 .. code-block:: python
82 >>> print(x.compute())
90 .. code-block:: python
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H A Duser-interfaces.rst37 .. code-block:: python
73 .. code-block:: python
96 .. code-block:: python
109 results = dask.compute(*lazy_results) # compute all in parallel
122 .. code-block:: python
139 .. code-block:: python
145 y = y.compute()
151 .. code-block:: python
153 # compute multiple results at the same time with the compute function
162 .. code-block:: python
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/dports/net/google-cloud-sdk/google-cloud-sdk/lib/googlecloudsdk/command_lib/meta/test_templates/
H A Dscenario_unit_test_template.tpl1 title: compute images get-iam-policy scenario test
6 - command: compute images get-iam-policy my-image
10 - command: compute images get-iam-policy my-image
40 command: compute images get-iam-policy my-image
44 …uri: https://compute.googleapis.com/compute/$$api-version$$/projects/fake-project/global/images/my…
58 code: 0
61 command: compute images get-iam-policy my-image
65 …uri: https://compute.googleapis.com/compute/$$api-version$$/projects/fake-project/global/images/my…
99 code: 0
107 …uri: https://compute.googleapis.com/compute/$$api-version$$/projects/fake-project/global/images/my…
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/dports/astro/py-skyfield/skyfield-1.41/skyfield/
H A Declipselib.py51 e = earth.compute(jd, fr)
52 m = moon.compute(jd, fr)
53 s = sun.compute(jd, fr)
74 b = earth_barycenter.compute(jd, fr)
75 e = earth.compute(jd, fr)
76 m = moon.compute(jd, fr)
77 s = sun.compute(jd, fr)
114 code = partial.astype(byte)
115 code += total
124 return t, code, details
/dports/math/R-cran-NMF/NMF/man/
H A Dalgorithmic.Rd125 that describes the algorithm used to compute another
136 iterations performed to compute an object. The function
142 been run to compute an object. Usually this will be 1,
148 methods for \code{objective} may also compute the
152 \code{runtime} returns the CPU time required to compute
157 compute a collection of objects, e.g. a sequence of
194 compute all fits stored in \code{object}
320 Returns the CPU time required to compute a single NMF
337 Returns the CPU time required to compute all the NMF
367 sequentially compute all NMF fits stored in
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H A DNMFList-class.Rd8 \code{\link{nmf}}, using different parameters, methods,
18 \item{algorithm}{\code{signature(object = "NMFList")}:
19 Returns the method names used to compute the NMF fits in
20 the list. It returns \code{NULL} if the list is empty. }
22 \item{runtime}{\code{signature(object = "NMFList")}:
23 Returns the CPU time required to compute all NMF fits in
28 \item{seqtime}{\code{signature(object = "NMFList")}:
30 sequentially compute all NMF fits stored in
31 \code{object}.
34 and sum up the results. It returns \code{NULL} on an
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/dports/graphics/piglit/piglit-136a7f5fa0703603be1ffb338abe4865e76a8058/tests/glslparsertest/glsl2/
H A Dxreal-lighting-dbs-omni.frag11 This file is part of XreaL source code.
13 XreaL source code is free software; you can redistribute it
18 XreaL source code is distributed in the hope that it will be
24 along with XreaL source code; if not, write to the Free Software
49 // compute view direction in tangent space
52 // compute light direction in tangent space
55 // compute half angle in tangent space
62 // compute the diffuse term
66 // compute the specular term
69 // compute attenuation
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/dports/devel/py-joblib/joblib-1.1.0/doc/auto_examples/
H A Dmemory_basic_usage.rst23 .. code-block:: python
48 .. code-block:: python
68 The function took 5.00 s to compute.
85 .. code-block:: python
115 The function took 5.07 s to compute.
128 .. code-block:: python
146 The function took 0.02 s to compute.
167 .. code-block:: python
203 The function took 5.07 s to compute.
211 .. code-block:: python
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/dports/misc/mxnet/incubator-mxnet-1.9.0/3rdparty/mkldnn/src/gpu/ocl/
H A Docl_gpu_engine.cpp57 compute::compute_engine_t::init(); in init()
84 cl_uint count_lines(const char **code) { in count_lines() argument
86 while (*code) { in count_lines()
88 code++; in count_lines()
101 std::vector<gpu::compute::scalar_type_t> arg_types; in create_kernel()
106 *kernel = compute::kernel_t( in create_kernel()
114 std::vector<compute::kernel_t> *kernels, in create_kernels()
116 const compute::kernel_ctx_t &kernel_ctx) const { in create_kernels()
119 compute::kernel_list_t kernel_list; in create_kernels()
150 std::vector<compute::kernel_t> *kernels, in create_kernels_from_ocl_source()
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/dports/science/lammps/lammps-stable_29Sep2021/doc/src/
H A Dcompute_smd_ulsph_num_neighs.rst1 .. index:: compute smd/ulsph/num/neighs
3 compute smd/ulsph/num/neighs command
9 .. code-block:: LAMMPS
11 compute ID group-ID smd/ulsph/num/neighs
13 * ID, group-ID are documented in :doc:`compute <compute>` command
14 * smd/ulsph/num/neighs = style name of this compute command
19 .. code-block:: LAMMPS
21 compute 1 all smd/ulsph/num/neighs
36 This compute returns a per-particle vector, which can be accessed by
37 any command that uses per-particle values from a compute as input.
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H A Dcompute_reduce_chunk.rst1 .. index:: compute reduce/chunk
3 compute reduce/chunk command
13 * ID, group-ID are documented in :doc:`compute <compute>` command
31 .. code-block:: LAMMPS
72 result of a :doc:`compute <compute>` or :doc:`fix <fix>` or the evaluation
90 .. code-block:: LAMMPS
114 .. code-block:: LAMMPS
123 .. code-block:: LAMMPS
141 .. code-block:: LAMMPS
151 .. code-block:: LAMMPS
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H A Dcompute_smd_ulsph_stress.rst1 .. index:: compute smd/ulsph/stress
3 compute smd/ulsph/stress command
9 .. code-block:: LAMMPS
11 compute ID group-ID smd/ulsph/stress
13 * ID, group-ID are documented in :doc:`compute <compute>` command
14 * smd/ulsph/stress = style name of this compute command
19 .. code-block:: LAMMPS
21 compute 1 all smd/ulsph/stress
34 This compute calculates a per-particle vector of vectors (tensors),
49 This compute is part of the MACHDYN package. It is only enabled if
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H A Dcompute_smd_ulsph_effm.rst1 .. index:: compute smd/ulsph/effm
3 compute smd/ulsph/effm command
9 .. code-block:: LAMMPS
11 compute ID group-ID smd/ulsph/effm
13 * ID, group-ID are documented in :doc:`compute <compute>` command
14 * smd/ulsph/effm = style name of this compute command
19 .. code-block:: LAMMPS
21 compute 1 all smd/ulsph/effm
35 This compute calculates a per-particle vector, which can be accessed
36 by any command that uses per-particle values from a compute as input.
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H A Dcompute_smd_ulsph_strain.rst1 .. index:: compute smd/ulsph/strain
3 compute smd/ulsph/strain command
9 .. code-block:: LAMMPS
11 compute ID group-ID smd/ulsph/strain
13 * ID, group-ID are documented in :doc:`compute <compute>` command
14 * smd/ulsph/strain = style name of this compute command
19 .. code-block:: LAMMPS
21 compute 1 all smd/ulsph/strain
35 This compute calculates a per-particle tensor, which can be accessed
49 This compute is part of the MACHDYN package. It is only enabled if
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H A Dcompute_smd_ulsph_strain_rate.rst1 .. index:: compute smd/ulsph/strain/rate
3 compute smd/ulsph/strain/rate command
9 .. code-block:: LAMMPS
11 compute ID group-ID smd/ulsph/strain/rate
13 * ID, group-ID are documented in :doc:`compute <compute>` command
14 * smd/ulsph/strain/rate = style name of this compute command
19 .. code-block:: LAMMPS
21 compute 1 all smd/ulsph/strain/rate
36 This compute calculates a per-particle vector of vectors (tensors),
49 This compute is part of the MACHDYN package. It is only enabled if
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/dports/math/R-cran-irlba/irlba/man/
H A Dpartial_eigen.Rd12 \item{n}{number of largest eigenvalues and corresponding eigenvectors to compute.}
14 \item{symmetric}{\code{TRUE} indicates \code{x} is a symmetric matrix (the default);
15 specify \code{symmetric=FALSE} to compute the largest eigenvalues and corresponding
16 eigenvectors of \code{t(x) \%*\% x} instead.}
28 Use \code{partial_eigen} to estimate a subset of the largest (most positive)
33 Specify \code{symmetric=FALSE} to compute the largest \code{n} eigenvalues
35 \code{t(x) \%*\% x}.
37 This function uses the \code{irlba} function under the hood. See \code{?irlba}
38 for description of additional options, especially the \code{tol} parameter.
53 # Use symmetric=FALSE to compute the eigenvalues of t(x) \%*\% x for general
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/dports/lang/racket-minimal/racket-8.3/src/ChezScheme/s/
H A Dinspect.ss2689 (compute-size ($continuation-return-code x))
2690 (compute-size ($closure-code x))
2726 (compute-size ($code-name x))
2727 (compute-size ($code-info x))
2728 (compute-size ($code-pinfo* x)))]
2866 (compute-composition! ($continuation-return-code x))
2867 (compute-composition! ($closure-code x))
2878 (compute-composition! ($closure-code x))
2902 (compute-composition! ($code-name x))
2903 (compute-composition! ($code-info x))
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/dports/lang/racket/racket-8.3/src/ChezScheme/s/
H A Dinspect.ss2689 (compute-size ($continuation-return-code x))
2690 (compute-size ($closure-code x))
2726 (compute-size ($code-name x))
2727 (compute-size ($code-info x))
2728 (compute-size ($code-pinfo* x)))]
2866 (compute-composition! ($continuation-return-code x))
2867 (compute-composition! ($closure-code x))
2878 (compute-composition! ($closure-code x))
2902 (compute-composition! ($code-name x))
2903 (compute-composition! ($code-info x))
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/dports/lang/chez-scheme/ChezScheme-9.5.4/s/
H A Dinspect.ss2508 (compute-size ($continuation-return-code x))
2509 (compute-size ($closure-code x))
2543 (compute-size ($code-name x))
2544 (compute-size ($code-info x))
2545 (compute-size ($code-pinfo* x)))]
2662 (compute-composition! ($continuation-return-code x))
2663 (compute-composition! ($closure-code x))
2673 (compute-composition! ($closure-code x))
2697 (compute-composition! ($code-name x))
2698 (compute-composition! ($code-info x))
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/dports/editors/texmacs/TeXmacs-1.99.4-src/src/Style/Environment/
H A Dstd_environment.cpp146 void compute () { in compute() function in assign_memorizer_rep
188 void compute () { in compute() function in begin_with_memorizer_rep
236 void compute () { in compute() function in end_with_memorizer_rep
280 void compute () { in compute() function in macro_down_memorizer_rep
306 void compute () { in compute() function in macro_redown_memorizer_rep
368 void compute () { in compute() function in macro_up_memorizer_rep
413 int i1= code%8, i2= (3*code)%8; in test_environment()
417 int j1= code % N(s1), j2= code % N(s2); in test_environment()
420 code= code*code % 176246173; in test_environment()
421 if (code < 0) code= -code; in test_environment()
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/dports/textproc/py-agate/agate-1.6.3/docs/cookbook/
H A Dexcel.rst14 .. code::
20 .. code-block:: python
25 new_table = table.compute([
34 .. code-block:: python
45 new_table = table.compute([
52 .. code-block:: python
54 new_table = table.compute([
61 .. code-block:: python
63 new_table = table.compute([
72 new_table = table.compute([
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/dports/devel/py-distributed/distributed-2021.11.2/docs/source/
H A Dmanage-computation.rst21 ``.compute()`` method or ``dask.compute(...)`` function. This function will
30 .. code-block:: python
39 .. code-block:: python
41 >>> df.compute()
56 client.compute
61 .. code-block:: python
75 .. code-block:: python
92 .. code-block:: python
128 .. code-block:: python
150 .. code-block:: python
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/dports/math/R-cran-spdep/spdep/man/
H A Dssw.Rd17 \item{id}{Node index to compute the cost}
19 If \code{method} is character, method must be "mahalanobis" or
22 If \code{method} is one of "euclidean", "maximum",
24 \code{\link{dist}} for details,
25 because this function as used to compute the distance.
26 If \code{method="mahalanobis"}, the mahalanobis distance
28 If \code{method} is a \code{function}, this function is
29 used to compute the distance.}
31 \item{cov}{The covariance matrix used to compute the mahalanobis
39 \code{id} of \code{data} and the mean (scalar of vector) of
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/dports/devel/R-cran-broom/broom/man/
H A Daugment_columns.Rd26 \item{type}{Type of prediction and residuals to compute}
28 \item{type.predict}{Type of prediction to compute; by default
29 same as \code{type}}
31 \item{type.residuals}{Type of residuals to compute; by default
32 same as \code{type}}
34 \item{se.fit}{Value to pass to predict's \code{se.fit}, or NULL for
40 \code{augment_columns} is intended for use in the internals of \code{augment} methods
42 instead use \code{\link[=augment]{augment()}} to appropriately make use of the functionality
43 in \code{augment_columns()}.
46 Note that, in the case that a \code{residuals()} or \code{influence()} generic is
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