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https://github.com/slsdetectorgroup/aare.git
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merge from latest developer
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@ -12,33 +12,6 @@ set(SPHINX_BUILD ${CMAKE_CURRENT_BINARY_DIR})
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file(GLOB SPHINX_SOURCE_FILES CONFIGURE_DEPENDS "src/*.rst")
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# set(SPHINX_SOURCE_FILES
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# src/index.rst
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# src/Installation.rst
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# src/Requirements.rst
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# src/NDArray.rst
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# src/NDView.rst
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# src/File.rst
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# src/Frame.rst
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# src/Dtype.rst
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# src/ClusterFinder.rst
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# src/ClusterFile.rst
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# src/Pedestal.rst
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# src/RawFile.rst
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# src/RawSubFile.rst
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# src/RawMasterFile.rst
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# src/Hdf5File.rst
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# src/Hdf5SubFile.rst
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# src/Hdf5MasterFile.rst
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# src/VarClusterFinder.rst
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# src/pyVarClusterFinder.rst
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# src/pyFile.rst
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# src/pyCtbRawFile.rst
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# src/pyRawFile.rst
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# src/pyRawMasterFile.rst
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# src/pyHdf5File.rst
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# src/pyHdf5MasterFile.rst
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# )
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foreach(filename ${SPHINX_SOURCE_FILES})
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@ -29,7 +29,6 @@ version = '@PROJECT_VERSION@'
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# extensions coming with Sphinx (named 'sphinx.ext.*') or your custom
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# ones.
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extensions = ['breathe',
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'sphinx_rtd_theme',
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'sphinx.ext.autodoc',
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'sphinx.ext.napoleon',
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]
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7
docs/src/ClusterFinderMT.rst
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7
docs/src/ClusterFinderMT.rst
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@ -0,0 +1,7 @@
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ClusterFinderMT
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==================
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.. doxygenclass:: aare::ClusterFinderMT
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:members:
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:undoc-members:
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6
docs/src/ClusterVector.rst
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6
docs/src/ClusterVector.rst
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@ -0,0 +1,6 @@
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ClusterVector
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=============
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.. doxygenclass:: aare::ClusterVector
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:members:
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:undoc-members:
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25
docs/src/JungfrauDataFile.rst
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25
docs/src/JungfrauDataFile.rst
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@ -0,0 +1,25 @@
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JungfrauDataFile
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==================
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JungfrauDataFile is a class to read the .dat files that are produced by Aldo's receiver.
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It is mostly used for calibration.
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The structure of the file is:
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* JungfrauDataHeader
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* Binary data (256x256, 256x1024 or 512x1024)
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* JungfrauDataHeader
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* ...
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There is no metadata indicating number of frames or the size of the image, but this
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will be infered by this reader.
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.. doxygenstruct:: aare::JungfrauDataHeader
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:members:
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:undoc-members:
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:private-members:
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.. doxygenclass:: aare::JungfrauDataFile
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:members:
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:undoc-members:
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:private-members:
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47
docs/src/Tests.rst
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47
docs/src/Tests.rst
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@ -0,0 +1,47 @@
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****************
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Tests
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****************
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We test the code both from the C++ and Python API. By default only tests that does not require image data is run.
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C++
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~~~~~~~~~~~~~~~~~~
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.. code-block:: bash
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mkdir build
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cd build
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cmake .. -DAARE_TESTS=ON
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make -j 4
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export AARE_TEST_DATA=/path/to/test/data
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./run_test [.files] #or using ctest, [.files] is the option to include tests needing data
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Python
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~~~~~~~~~~~~~~~~~~
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.. code-block:: bash
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#From the root dir of the library
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python -m pytest python/tests --files # passing --files will run the tests needing data
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Getting the test data
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~~~~~~~~~~~~~~~~~~~~~~~~
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.. attention ::
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The tests needing the test data are not run by default. To make the data available, you need to set the environment variable
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AARE_TEST_DATA to the path of the test data directory. Then pass either [.files] for the C++ tests or --files for Python
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The image files needed for the test are large and are not included in the repository. They are stored
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using GIT LFS in a separate repository. To get the test data, you need to clone the repository.
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To do this, you need to have GIT LFS installed. You can find instructions on how to install it here: https://git-lfs.github.com/
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Once you have GIT LFS installed, you can clone the repository like any normal repo using:
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.. code-block:: bash
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git clone https://gitea.psi.ch/detectors/aare-test-data.git
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docs/src/algorithm.rst
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5
docs/src/algorithm.rst
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algorithm
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=============
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.. doxygenfile:: algorithm.hpp
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@ -20,9 +20,6 @@ AARE
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Requirements
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Consume
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.. toctree::
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:caption: Python API
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:maxdepth: 1
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@ -30,24 +27,32 @@ AARE
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pyFile
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pyCtbRawFile
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pyClusterFile
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pyClusterVector
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pyJungfrauDataFile
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pyRawFile
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pyRawMasterFile
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pyHdf5File
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pyHdf5MasterFile
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pyVarClusterFinder
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pyFit
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.. toctree::
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:caption: C++ API
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:maxdepth: 1
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algorithm
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NDArray
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NDView
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Frame
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File
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Dtype
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ClusterFinder
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ClusterFinderMT
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ClusterFile
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ClusterVector
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JungfrauDataFile
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Pedestal
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RawFile
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RawSubFile
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@ -58,4 +63,8 @@ AARE
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.. toctree::
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:caption: Developer
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:maxdepth: 3
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Tests
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33
docs/src/pyClusterVector.rst
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33
docs/src/pyClusterVector.rst
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@ -0,0 +1,33 @@
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ClusterVector
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================
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The ClusterVector, holds clusters from the ClusterFinder. Since it is templated
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in C++ we use a suffix indicating the data type in python. The suffix is
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``_i`` for integer, ``_f`` for float, and ``_d`` for double.
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At the moment the functionality from python is limited and it is not supported
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to push_back clusters to the vector. The intended use case is to pass it to
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C++ functions that support the ClusterVector or to view it as a numpy array.
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**View ClusterVector as numpy array**
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.. code:: python
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from aare import ClusterFile
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with ClusterFile("path/to/file") as f:
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cluster_vector = f.read_frame()
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# Create a copy of the cluster data in a numpy array
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clusters = np.array(cluster_vector)
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# Avoid copying the data by passing copy=False
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clusters = np.array(cluster_vector, copy = False)
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.. py:currentmodule:: aare
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.. autoclass:: ClusterVector_i
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:members:
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:undoc-members:
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:show-inheritance:
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:inherited-members:
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19
docs/src/pyFit.rst
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19
docs/src/pyFit.rst
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@ -0,0 +1,19 @@
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Fit
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========
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.. py:currentmodule:: aare
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**Functions**
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.. autofunction:: gaus
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.. autofunction:: pol1
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**Fitting**
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.. autofunction:: fit_gaus
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.. autofunction:: fit_pol1
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docs/src/pyJungfrauDataFile.rst
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10
docs/src/pyJungfrauDataFile.rst
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JungfrauDataFile
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===================
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.. py:currentmodule:: aare
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.. autoclass:: JungfrauDataFile
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:members:
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:undoc-members:
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:show-inheritance:
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:inherited-members:
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