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author | astroteam |
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date | Fri, 18 Jul 2025 14:23:35 +0000 |
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<tool id="source_extractor_astro_tool" name="source-extractor" version="0.0.1+galaxy0" profile="24.0"> <requirements> <requirement type="package" version="6.1.4">astropy</requirement> <requirement type="package" version="3.10.3">matplotlib</requirement> <requirement type="package" version="1.21.4">wget</requirement> <requirement type="package" version="1.4.1">sep</requirement> <requirement type="package" version="1.2.33">oda-api</requirement> <requirement type="package" version="2025.6.11">tifffile</requirement> <requirement type="package" version="9.4.0">ipython</requirement> <!--Requirements string 'nb2workflow>=1.3.30' can't be converted automatically. Please add the galaxy/conda requirement manually or modify the requirements file!--> </requirements> <command detect_errors="exit_code">ipython '$__tool_directory__/source_extraction.py'</command> <environment_variables> <environment_variable name="BASEDIR">$__tool_directory__</environment_variable> <environment_variable name="GALAXY_TOOL_DIR">$__tool_directory__</environment_variable> </environment_variables> <configfiles> <inputs name="inputs" filename="inputs.json" data_style="paths" /> </configfiles> <inputs> <param name="input_file" type="data" label="Input file" format="data" optional="false" /> <param name="mask_file" type="data" label="Mask file" format="data" optional="true" /> <param name="thresh" type="float" value="1.5" label="thresh" optional="false" /> <param name="err_option" type="select" label="err_option" optional="false"> <option value="array_rms">array_rms</option> <option value="float_globalrms" selected="true">float_globalrms</option> <option value="none">none</option> </param> <param name="maskthresh" type="float" value="0.0" label="maskthresh" optional="false" /> <param name="minarea" type="integer" value="5" label="minarea" optional="false" /> <param name="filter_case" type="select" label="Filter Case" optional="false"> <option value="default" selected="true">default</option> <option value="file">file</option> <option value="none">none</option> </param> <param name="filter_file" type="data" label="Filter file" format="data" optional="true" /> <param name="filter_type" type="select" label="filter_type" optional="false"> <option value="conv">conv</option> <option value="matched" selected="true">matched</option> </param> <param name="deblend_nthresh" type="integer" value="32" label="deblend_nthresh" optional="false" /> <param name="deblend_cont" type="float" value="0.005" label="deblend_cont" optional="false" /> <param name="clean" type="boolean" checked="true" label="clean" optional="false" /> <param name="clean_param" type="float" value="1.0" label="clean_param" optional="false" /> <param name="bw" type="integer" value="64" label="bw" optional="false" /> <param name="bh" type="integer" value="64" label="bh" optional="false" /> <param name="fw" type="integer" value="3" label="fw" optional="false" /> <param name="fh" type="integer" value="3" label="fh" optional="false" /> <param name="fthresh" type="float" value="0.0" label="fthresh" optional="false" /> </inputs> <outputs> <data label="${tool.name} -> source_extraction bkg_picture" name="out_source_extraction_bkg_picture" format="auto" from_work_dir="bkg_picture_galaxy.output" /> <data label="${tool.name} -> source_extraction rms_picture" name="out_source_extraction_rms_picture" format="auto" from_work_dir="rms_picture_galaxy.output" /> <data label="${tool.name} -> source_extraction data_picture" name="out_source_extraction_data_picture" format="auto" from_work_dir="data_picture_galaxy.output" /> <data label="${tool.name} -> source_extraction sources_picture" name="out_source_extraction_sources_picture" format="auto" from_work_dir="sources_picture_galaxy.output" /> <data label="${tool.name} -> source_extraction segmentation_map_picture" name="out_source_extraction_segmentation_map_picture" format="auto" from_work_dir="segmentation_map_picture_galaxy.output" /> <data label="${tool.name} -> source_extraction segmentation_map" name="out_source_extraction_segmentation_map" format="auto" from_work_dir="segmentation_map_galaxy.output" /> <data label="${tool.name} -> source_extraction bkg_array" name="out_source_extraction_bkg_array" format="auto" from_work_dir="bkg_array_galaxy.output" /> <data label="${tool.name} -> source_extraction rms_array" name="out_source_extraction_rms_array" format="auto" from_work_dir="rms_array_galaxy.output" /> <data label="${tool.name} -> source_extraction catalog_table" name="out_source_extraction_catalog_table" format="auto" from_work_dir="catalog_table_galaxy.output" /> </outputs> <tests> <test expect_num_outputs="9"> <param name="input_file" location="https://gitlab.renkulab.io/astronomy/mmoda/source-extractor/-/raw/5680fc685979c56c69f98eec8153673422abfa72/input.fits" /> <param name="thresh" value="1.5" /> <param name="err_option" value="float_globalrms" /> <param name="maskthresh" value="0.0" /> <param name="minarea" value="5" /> <param name="filter_case" value="default" /> <param name="filter_type" value="matched" /> <param name="deblend_nthresh" value="32" /> <param name="deblend_cont" value="0.005" /> <param name="clean" value="True" /> <param name="clean_param" value="1.0" /> <param name="bw" value="64" /> <param name="bh" value="64" /> <param name="fw" value="3" /> <param name="fh" value="3" /> <param name="fthresh" value="0.0" /> <assert_stdout> <has_text text="*** Job finished successfully ***" /> </assert_stdout> </test> </tests> <help>Source extractor ================ This tool can be used to extract luminous sources from sky images. It is entirely based on the `sep <https://sep.readthedocs.io/en/stable/index.html>`__ package, which is built on `Source Extractor <https://sextractor.readthedocs.io/en/latest/Introduction.html>`__. Input ----- Important input parameters: 1. **Input file** (``.fits`` or ``.tiff``) - A single-channel sky image to analyze. 2. **Mask file** (``.fits`` or ``.tiff``; optional) - A 2D numpy array. True values, or numeric values greater than **maskthresh**, are considered masked. Masking a pixel is equivalent to setting data to zero and noise (if present) to infinity. 3. **thresh** - Threshold pixel value for detection: ``thresh * err[j, i]``, where ``err[j, i]`` is given by the **err_option** parameter; ``j`` and ``i`` represent the pixel indices 4. **err_option** - Sets the error that is taken into account into the detection of sources: - ``none`` - The value of **thresh** is taken as an absolute threshold. - ``array_rms`` - An array of the background RMS, i.e. for each individual pixel. - ``float_globalrms`` - A float value of the global background RMS. The rest of the parameters are described in the documentations of `sep.Background <https://sep.readthedocs.io/en/stable/api/sep.Background.html#sep.Background>`__ and `sep.extract <https://sep.readthedocs.io/en/stable/api/sep.extract.html#sep.extract>`__. Output ------ Source Catalog ~~~~~~~~~~~~~~ The catalogue of sources is explained `here <https://sep.readthedocs.io/en/stable/api/sep.extract.html#sep.extract>`__. Images ~~~~~~ There are 4 images as output: - **Background**: - ``.fits``: The output of ``sep.Background`` function, i.e. the estimated 2D background of the input image. - ``.png``: The gray-scale image of the previously described array - **Background noise**: - ``.fits``: The RMS of the background image. - ``.png``: The gray-scale image of the previously described array - **Input image** - The gray-scale input image. - **Sources** - The sources on the background subtracted input image - **Segmentation map**: - ``.fits``: Each pixel is labeled with 0 or object ID (``0`` = background; ``i+1`` = object ``i``). - ``.png``: Binary mask (``1`` = source, ``0`` = background). Acknowledgement --------------- Bertin, E. & Arnouts, S. 1996: `SExtractor: Software for source extraction <https://ui.adsabs.harvard.edu/abs/1996A%26AS..117..393B/abstract>`__, Astronomy & Astrophysics Supplement 317, 393 Barbary, (2016), SEP: Source Extractor as a library, Journal of Open Source Software, 1(6), 58, doi:10.21105/joss.00058 </help> <citations> <citation type="doi">10.1051/aas:1996164</citation> <citation type="doi">10.21105/joss.00058</citation> </citations> </tool>