Developing Open Source is great fun! Join us on the scikit-image developer forum.
If you're looking for something to implement or to fix, you can browse the open issues on GitHub.
Warning
Given the uncertainty around licensing of AI-generated code, we require that you not make use of these tools during the development of any contributions to scikit-image.
The following is a brief overview about how changes to source code and documentation can be contributed to scikit-image.
If you are a first-time contributor:
Go to https://github.com/scikit-image/scikit-image and click the "fork" button to create your own copy of the project.
Clone (download) the repository with the project source on your local computer:
git clone https://github.com/your-username/scikit-image.git
Change into the root directory of the cloned repository:
cd scikit-image
Add the upstream repository:
git remote add upstream https://github.com/scikit-image/scikit-image.git
Now, you have remote repositories named:
upstream
, which refers to thescikit-image
repository, andorigin
, which refers to your personal fork.
Next, :ref:`set up your build environment <build-env-setup>`.
Finally, we recommend that you use a pre-commit hook, which runs code checkers and formatters each time you do a
git commit
:pip install pre-commit pre-commit install
Develop your contribution:
Pull the latest changes from upstream:
git checkout main git pull upstream main
Create a branch for the feature you want to work on. Use a sensible name, such as 'transform-speedups':
git checkout -b transform-speedups
Commit locally as you progress (with
git add
andgit commit
). Please write good commit messages.
To submit your contribution:
Push your changes back to your fork on GitHub:
git push origin transform-speedups
Enter your GitHub username and password (repeat contributors or advanced users can remove this step by connecting to GitHub with SSH).
Go to GitHub. The new branch will show up with a green "pull request" button -- click it.
If you want, post on the developer forum to explain your changes or to ask for review.
For a more detailed discussion, read these :doc:`detailed documents
<../gitwash/index>` on how to use Git with scikit-image
(:ref:`using-git`).
Review process:
- Reviewers (the other developers and interested community members) will write inline and/or general comments on your pull request (PR) to help you improve its implementation, documentation, and style. Every single developer working on the project has their code reviewed, and we've come to see it as a friendly conversation from which we all learn and the overall code quality benefits. Therefore, please don't let the review discourage you from contributing: its only aim is to improve the quality of the project, not to criticize (we are, after all, very grateful for the time you're donating!).
- To update your pull request, make your changes on your local repository and commit. As soon as those changes are pushed up (to the same branch as before) the pull request will update automatically.
- Continuous integration (CI) services are triggered after each pull request submission to build the package, run unit tests, measure code coverage, and check the coding style (PEP8) of your branch. The tests must pass before your PR can be merged. If CI fails, you can find out why by clicking on the "failed" icon (red cross) and inspecting the build and test logs.
- A pull request must be approved by two core team members before merging.
Document changes
If your change introduces any API modifications, please update
doc/release/release_dev.rst
.If your change introduces a deprecation, add a reminder to
TODO.txt
for the team to remove the deprecated functionality in the future.
Note
To reviewers: if it is not obvious from the PR description, add a short explanation of what a branch did to the merge message and, if closing a bug, also add "Closes #123" where 123 is the issue number.
If GitHub indicates that the branch of your PR can no longer be merged automatically, merge the main branch into yours:
git fetch upstream main git merge upstream/main
If any conflicts occur, they need to be fixed before continuing. See which files are in conflict using:
git status
Which displays a message like:
Unmerged paths: (use "git add <file>..." to mark resolution) both modified: file_with_conflict.txt
Inside the conflicted file, you'll find sections like these:
The way the text looks in your branch
Choose one version of the text that should be kept, and delete the rest:
The way the text looks in your branch
Now, add the fixed file:
git add file_with_conflict.txt
Once you've fixed all merge conflicts, do:
git commit
Note
Advanced Git users are encouraged to rebase instead of merge, but we squash and merge most PRs either way.
- All code should have tests (see test coverage below for more details).
- All code should be documented, to the same standard as NumPy and SciPy.
- For new functionality, always add an example to the gallery (see Gallery below for more details).
- No changes are ever merged without review and approval by two core team members. There are two exceptions to this rule. First, pull requests which affect only the documentation require review and approval by only one core team member in most cases. If the maintainer feels the changes are large or likely to be controversial, two reviews should still be encouraged. The second case is that of minor fixes which restore CI to a working state, because these should be merged fairly quickly. Reach out on the developer forum if you get no response to your pull request. Never merge your own pull request.
Set up your editor to remove trailing whitespace. Follow PEP08.
Use numpy data types instead of strings (
np.uint8
instead of"uint8"
).Use the following import conventions:
import numpy as np import matplotlib.pyplot as plt import scipy as sp import skimage as ski sp.ndimage.label(...) ski.measure.label(...) # only in Cython code cimport numpy as cnp cnp.import_array()
When documenting array parameters, use
image : (M, N) ndarray
and then refer toM
andN
in the docstring, if necessary.Refer to array dimensions as (plane), row, column, not as x, y, z. See :ref:`Coordinate conventions <numpy-images-coordinate-conventions>` in the user guide for more information.
Functions should support all input image dtypes. Use utility functions such as
img_as_float
to help convert to an appropriate type. The output format can be whatever is most efficient. This allows us to string together several functions into a pipeline, e.g.:hough(canny(my_image))
Use
Py_ssize_t
as data type for all indexing, shape and size variables in C/C++ and Cython code.Use relative module imports, i.e.
from .._shared import xyz
rather thanfrom skimage._shared import xyz
.Wrap Cython code in a pure Python function, which defines the API. This improves compatibility with code introspection tools, which are often not aware of Cython code.
For Cython functions, release the GIL whenever possible, using
with nogil:
.
The test suite must pass before a pull request can be merged, and tests should be added to cover all modifications in behavior.
We use the pytest testing
framework, with tests located in the various
skimage/submodule/tests
folders.
Testing requirements are listed in requirements/test.txt. Run:
- All tests:
spin test
- Tests for a submodule:
spin test skimage/morphology
- Run tests from a specific file:
spin test skimage/morphology/tests/test_gray.py
- Run a test inside a file:
spin test skimage/morphology/tests/test_gray.py::test_3d_fallback_black_tophat
- Run tests with arbitrary ``pytest`` options:
spin test -- any pytest args you want
. - Run all tests and doctests:
spin test -- --doctest-modules skimage
By default, warnings raised by the test suite result in errors.
You can switch that behavior off by setting the environment variable
SKIMAGE_TEST_STRICT_WARNINGS
to 0.
Tests for a module should ideally cover all code in that module, i.e., statement coverage should be at 100%.
To measure test coverage run:
$ spin coverage
This will print a report with one line for each file in skimage, detailing the test coverage:
Name Stmts Exec Cover Missing ------------------------------------------------------------------------------ skimage/color/colorconv 77 77 100% skimage/filter/__init__ 1 1 100% ...
To build the HTML documentation, run:
spin docs
Output is in scikit-image/doc/build/html/
. Add the --clean
flag to build from scratch, deleting any cached output.
The example gallery is built using
Sphinx-Gallery.
Refer to their documentation for complete usage instructions, and also
to existing examples in doc/examples
.
Gallery examples should have a maximum figure width of 8 inches. You can also change a gallery entry's thumbnail.
- "citation not found: R###" There is probably an underscore after a reference in the first line of a docstring (e.g. [1]_). Use this method to find the source file: $ cd doc/build; grep -rin R####
- "Duplicate citation R###, other instance in..."" There is probably a [2] without a [1] in one of the docstrings
- Make sure to use pre-sphinxification paths to images (not the _images directory)
If the way a function is called has to be changed, a deprecation cycle must be followed to warn users.
A deprecation cycle is not necessary when:
- adding a new function, or
- adding a new keyword argument to the end of a function signature, or
- fixing unexpected or incorrect behavior.
A deprecation cycle is necessary when:
- renaming keyword arguments, or
- changing the order of arguments or keywords, or
- adding arguments to a function, or
- changing a function's name or location, or
- changing the default value of function arguments or keywords.
Typically, deprecation warnings are in place for two releases, before a change is made.
For example, consider the modification of a default value in a function signature. In version N, we have:
def some_function(image, rescale=True):
"""Do something.
Parameters
----------
image : ndarray
Input image.
rescale : bool, optional
Rescale the image unless ``False`` is given.
Returns
-------
out : ndarray
The resulting image.
"""
out = do_something(image, rescale=rescale)
return out
In version N+1, we will change this to:
def some_function(image, rescale=None):
"""Do something.
Parameters
----------
image : ndarray
Input image.
rescale : bool, optional
Rescale the image unless ``False`` is given.
.. warning:: The default value will change from ``True`` to
``False`` in skimage N+3.
Returns
-------
out : ndarray
The resulting image.
"""
if rescale is None:
warn('The default value of rescale will change '
'to `False` in version N+3.', stacklevel=2)
rescale = True
out = do_something(image, rescale=rescale)
return out
And, in version N+3:
def some_function(image, rescale=False):
"""Do something.
Parameters
----------
image : ndarray
Input image.
rescale : bool, optional
Rescale the image if ``True`` is given.
Returns
-------
out : ndarray
The resulting image.
"""
out = do_something(image, rescale=rescale)
return out
Here is the process for a 3-release deprecation cycle:
- Set the default to None, and modify the docstring to specify that the default is True.
- In the function, _if_ rescale is None, set it to True and warn that the default will change to False in version N+3.
- In
doc/release/release_dev.rst
, under deprecations, add "In some_function, the rescale argument will default to False in N+3." - In
TODO.txt
, create an item in the section related to version N+3 and write "change rescale default to False in some_function".
Note that the 3-release deprecation cycle is not a strict rule and, in some cases, developers can agree on a different procedure.
skimage
raises FutureWarning
s to highlight changes in its
API, e.g.:
from warnings import warn
warn(
"Automatic detection of the color channel was deprecated in "
"v0.19, and `channel_axis=None` will be the new default in "
"v0.22. Set `channel_axis=-1` explicitly to silence this "
"warning.",
FutureWarning,
stacklevel=2,
)
The stacklevel is a bit of a technicality, but ensures that the warning points to the user-called function, and not to a utility function within.
In most cases, set the stacklevel
to 2
.
When warnings originate from helper routines internal to the
scikit-image library, set it to 3
.
To test if your warning is being emitted correctly, try calling the function from an IPython console. It should point you to the console input itself instead of being emitted by files in the scikit-image library:
- Good:
ipython:1: UserWarning: ...
- Bad:
scikit-image/skimage/measure/_structural_similarity.py:155: UserWarning:
When removing keywords or entire functions, the
skimage._shared.utils.deprecate_kwarg
and
skimage._shared.utils.deprecate_func
utility functions can be used
to perform the above procedure.
While code is hosted on github, example datasets are on gitlab. These are fetched with pooch when accessing skimage.data.*.
New datasets are submitted on gitlab and, once merged, the data
registry skimage/data/_registry.py
in the main GitHub repository
can be updated.
While not mandatory for most pull requests, we ask that performance related PRs include a benchmark in order to clearly depict the use-case that is being optimized for. A historical view of our snapshots can be found on at the following website.
In this section we will review how to setup the benchmarks,
and three commands spin asv -- dev
, spin asv -- run
and
spin asv -- continuous
.
Begin by installing airspeed velocity
in your development environment. Prior to installation, be sure to activate your
development environment, then if using venv
you may install the requirement with:
source skimage-dev/bin/activate pip install asv
If you are using conda, then the command:
conda activate skimage-dev conda install asv
is more appropriate. Once installed, it is useful to run the command:
spin asv -- machine
To let airspeed velocity know more information about your machine.
To write benchmark, add a file in the benchmarks
directory which contains a
a class with one setup
method and at least one method prefixed with time_
.
The time_
method should only contain code you wish to benchmark.
Therefore it is useful to move everything that prepares the benchmark scenario
into the setup
method. This function is called before calling a time_
method and its execution time is not factored into the benchmarks.
Take for example the TransformSuite
benchmark:
import numpy as np
from skimage import transform
class TransformSuite:
"""Benchmark for transform routines in scikit-image."""
def setup(self):
self.image = np.zeros((2000, 2000))
idx = np.arange(500, 1500)
self.image[idx[::-1], idx] = 255
self.image[idx, idx] = 255
def time_hough_line(self):
result1, result2, result3 = transform.hough_line(self.image)
Here, the creation of the image is completed in the setup
method, and not
included in the reported time of the benchmark.
It is also possible to benchmark features such as peak memory usage. To learn more about the features, please refer to the official airspeed velocity documentation.
Also, the benchmark files need to be importable when benchmarking old versions of scikit-image. So if anything from scikit-image is imported at the top level, it should be done as:
try:
from skimage import metrics
except ImportError:
pass
The benchmarks themselves don't need any guarding against missing features, only the top-level imports.
To allow tests of newer functions to be marked as "n/a" (not available) rather than "failed" for older versions, the setup method itself can raise a NotImplemented error. See the following example for the registration module:
try:
from skimage import registration
except ImportError:
raise NotImplementedError("registration module not available")
Prior to running the true benchmark, it is often worthwhile to test that the code is free of typos. To do so, you may use the command:
spin asv -- dev -b TransformSuite
Where the TransformSuite
above will be run once in your current environment
to test that everything is in order.
The command above is fast, but doesn't test the performance of the code
adequately. To do that you may want to run the benchmark in your current
environment to see the performance of your change as you are developing new
features. The command asv run -E existing
will specify that you wish to run
the benchmark in your existing environment. This will save a significant amount
of time since building scikit-image can be a time consuming task:
spin asv -- run -E existing -b TransformSuite
Often, the goal of a PR is to compare the results of the modifications in terms
speed to a snapshot of the code that is in the main branch of the
scikit-image
repository. The command asv continuous
is of help here:
spin asv -- continuous main -b TransformSuite
This call will build out the environments specified in the asv.conf.json
file and compare the performance of the benchmark between your current commit
and the code in the main branch.
The output may look something like:
$ spin asv -- continuous main -b TransformSuite · Creating environments · Discovering benchmarks ·· Uninstalling from conda-py3.7-cython-numpy1.15-scipy ·· Installing 544c0fe3 <benchmark_docs> into conda-py3.7-cython-numpy1.15-scipy. · Running 4 total benchmarks (2 commits * 2 environments * 1 benchmarks) [ 0.00%] · For scikit-image commit 37c764cb <benchmark_docs~1> (round 1/2): [...] [100.00%] ··· ...ansform.TransformSuite.time_hough_line 33.2±2ms BENCHMARKS NOT SIGNIFICANTLY CHANGED.
In this case, the differences between HEAD and main are not significant enough for airspeed velocity to report.
It is also possible to get a comparison of results for two specific revisions for which benchmark results have previously been run via the asv compare command:
spin asv -- compare v0.14.5 v0.17.2
Finally, one can also run ASV benchmarks only for a specific commit hash or
release tag by appending ^!
to the commit or tag name. For example to run
the skimage.filter module benchmarks on release v0.17.2:
spin asv -- run -b Filter v0.17.2^!