Mercurial > repos > astroteam > cta_astro_tool
diff cta_astro_tool.xml @ 0:2f3e314c3dfa draft default tip
planemo upload for repository https://github.com/esg-epfl-apc/tools-astro/tree/main/tools commit 4543470805fc78f6cf2604b9d55beb6f06359995
author | astroteam |
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date | Fri, 19 Apr 2024 10:06:21 +0000 |
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--- /dev/null Thu Jan 01 00:00:00 1970 +0000 +++ b/cta_astro_tool.xml Fri Apr 19 10:06:21 2024 +0000 @@ -0,0 +1,183 @@ +<tool id="cta_astro_tool" name="CTA" version="0.0.1+galaxy0" profile="23.0"> + <requirements> + <requirement type="package" version="6.0">unzip</requirement> + <requirement type="package" version="2.31.0">requests</requirement> + <requirement type="package" version="1.2">gammapy</requirement> + <requirement type="package" version="5.3">astropy</requirement> + <requirement type="package" version="3.8.4">matplotlib</requirement> + <requirement type="package" version="1.11.4">scipy</requirement> + <requirement type="package" version="1.2.15">oda-api</requirement> + <requirement type="package" version="8.22.2">ipython</requirement> + <!--Requirements string 'nb2workflow[cwl,service,rdf,mmoda]>=1.3.30 +' can't be converted automatically. Please add the galaxy/conda requirement manually or modify the requirements file!--> + <requirement type="package" version="7.16.3">nbconvert</requirement> + </requirements> + <command detect_errors="exit_code">ipython '$__tool_directory__/${_data_product._selector}.py'</command> + <configfiles> + <inputs name="inputs" filename="inputs.json" data_style="paths" /> + </configfiles> + <inputs> + <conditional name="_data_product"> + <param name="_selector" type="select" label="Data Product"> + <option value="pre-defined_model" selected="true">pre-defined_model</option> + <option value="model_cube_file" selected="false">model_cube_file</option> + </param> + <when value="pre-defined_model"> + <param name="RA" type="float" value="166.113809" label="RA (unit: deg)" /> + <param name="DEC" type="float" value="38.208833" label="DEC (unit: deg)" /> + <param name="OffAxis_angle" type="float" value="0.78" label="OffAxis_angle (unit: deg)" /> + <param name="Texp" type="float" value="1.0" label="Texp (unit: hour)" /> + <param name="z" type="float" value="0.03" label="z" /> + <param name="F0" type="float" value="1e-11" label="F0" /> + <param name="E0" type="float" value="1.0" label="E0 (unit: TeV)" /> + <param name="Gamma" type="float" value="2.0" label="Gamma" /> + <param name="Radius_spectal_extraction" type="float" value="0.2" label="Radius_spectal_extraction" /> + <param name="Radius_sky_image" type="float" value="2.5" label="Radius_sky_image (unit: deg)" /> + <param name="Site" type="select" label="Site"> + <option value="North" selected="true">North</option> + <option value="South">South</option> + </param> + <param name="Telescope_LST" type="boolean" checked="true" label="Telescope_LST" /> + <param name="Telescope_MST" type="boolean" checked="true" label="Telescope_MST" /> + <param name="Telescope_SST" type="boolean" label="Telescope_SST" /> + </when> + <when value="model_cube_file"> + <param name="data_cube" type="data" label="data_cube" format="data" /> + <param name="F0" type="float" value="1e-11" label="F0" /> + <param name="E0" type="float" value="1.0" label="E0 (unit: TeV)" /> + <param name="OffAxis_angle" type="float" value="0.4" label="OffAxis_angle (unit: deg)" /> + <param name="Radius_spectal_extraction" type="float" value="0.2" label="Radius_spectal_extraction (unit: deg)" /> + <param name="Radius_sky_image" type="float" value="2.5" label="Radius_sky_image (unit: deg)" /> + <param name="Site" type="select" label="Site"> + <option value="North" selected="true">North</option> + <option value="South">South</option> + </param> + <param name="Telescopes_LST" type="boolean" checked="true" label="Telescopes_LST" /> + <param name="Telescopes_MST" type="boolean" checked="true" label="Telescopes_MST" /> + <param name="Telescopes_SST" type="boolean" label="Telescopes_SST" /> + <param name="Texp" type="float" value="1.0" label="Texp (unit: hour)" /> + </when> + </conditional> + </inputs> + <outputs> + <data label="${tool.name} -> pre-defined_model image_png" name="out_pre_defined_model_image_png" format="auto" from_work_dir="image_png_galaxy.output"> + <filter>_data_product['_selector'] == 'pre-defined_model'</filter> + </data> + <data label="${tool.name} -> pre-defined_model theta2_png" name="out_pre_defined_model_theta2_png" format="auto" from_work_dir="theta2_png_galaxy.output"> + <filter>_data_product['_selector'] == 'pre-defined_model'</filter> + </data> + <data label="${tool.name} -> pre-defined_model spectrum_png" name="out_pre_defined_model_spectrum_png" format="auto" from_work_dir="spectrum_png_galaxy.output"> + <filter>_data_product['_selector'] == 'pre-defined_model'</filter> + </data> + <data label="${tool.name} -> pre-defined_model event_list_fits" name="out_pre_defined_model_event_list_fits" format="auto" from_work_dir="event_list_fits_galaxy.output"> + <filter>_data_product['_selector'] == 'pre-defined_model'</filter> + </data> + <data label="${tool.name} -> model_cube_file spectrum_png" name="out_model_cube_file_spectrum_png" format="auto" from_work_dir="spectrum_png_galaxy.output"> + <filter>_data_product['_selector'] == 'model_cube_file'</filter> + </data> + <data label="${tool.name} -> model_cube_file theta2_png" name="out_model_cube_file_theta2_png" format="auto" from_work_dir="theta2_png_galaxy.output"> + <filter>_data_product['_selector'] == 'model_cube_file'</filter> + </data> + <data label="${tool.name} -> model_cube_file image_png" name="out_model_cube_file_image_png" format="auto" from_work_dir="image_png_galaxy.output"> + <filter>_data_product['_selector'] == 'model_cube_file'</filter> + </data> + <data label="${tool.name} -> model_cube_file event_list_fits" name="out_model_cube_file_event_list_fits" format="auto" from_work_dir="event_list_fits_galaxy.output"> + <filter>_data_product['_selector'] == 'model_cube_file'</filter> + </data> + </outputs> + <tests> + <test expect_num_outputs="4"> + <conditional name="_data_product"> + <param name="_selector" value="pre-defined_model" /> + <param name="RA" value="166.113809" /> + <param name="DEC" value="38.208833" /> + <param name="OffAxis_angle" value="0.78" /> + <param name="Texp" value="1.0" /> + <param name="z" value="0.03" /> + <param name="F0" value="1e-11" /> + <param name="E0" value="1.0" /> + <param name="Gamma" value="2.0" /> + <param name="Radius_spectal_extraction" value="0.2" /> + <param name="Radius_sky_image" value="2.5" /> + <param name="Site" value="North" /> + <param name="Telescope_LST" value="True" /> + <param name="Telescope_MST" value="True" /> + <param name="Telescope_SST" value="False" /> + </conditional> + <assert_stdout> + <has_text text="*** Job finished successfully ***" /> + </assert_stdout> + </test> + <test expect_num_outputs="4"> + <conditional name="_data_product"> + <param name="_selector" value="model_cube_file" /> + <param name="data_cube" location="https://gitlab.renkulab.io/astronomy/mmoda/cta/-/raw/b3f69b091ce942c05ad035220501ea078d54de26/3d.fits" /> + <param name="F0" value="1e-11" /> + <param name="E0" value="1.0" /> + <param name="OffAxis_angle" value="0.4" /> + <param name="Radius_spectal_extraction" value="0.2" /> + <param name="Radius_sky_image" value="2.5" /> + <param name="Site" value="North" /> + <param name="Telescopes_LST" value="True" /> + <param name="Telescopes_MST" value="True" /> + <param name="Telescopes_SST" value="False" /> + <param name="Texp" value="1.0" /> + </conditional> + <assert_stdout> + <has_text text="*** Job finished successfully ***" /> + </assert_stdout> + </test> + </tests> + <help>This service provides simulaiton of observations with `Cherenkov +Telescope Array (CTA) <https://www.cta-observatory.org/>`__ observatory +(now in construction), based on the Instrument Response Funcitons (IRF) +from Monte-Carlo Production 5: |DOI|. The simulation is done using +`Gammapy <https://gammapy.org/>`__ package. + +Two possibilities for defining the sky model are available: +``Simulate_pointing_using_pre-defined_model`` and +``Simulate_pointing_using_model_cube_file``. The “pre-defined model” +option provides a possibility to simulate a source at sky position +``RA``, ``DEC``, with a power-law spectrum, +``dN/dE=F0 (E/E0)^{-\Gamma}``, considering also the effect of absorption +on the Extragalactic Backgorund Light (EBL, based on `Franceschini et +al. (2017) <https://arxiv.org/abs/1705.10256>`__ model. In the “model +cube file” approach, the sky model is loaded from a datacube file (to be +uploaded from an URL to be given in the parameter box). The model cube +describes source counts as a function of ``RA``, ``DEC`` and energy +``E``. Hence, both the source position on the sky and the model source +spectrum are encoded directly in the data cube. + +Parameters that can be adjusted are the source position (``RA``, +``DEC``), the off-axis angle in the telescope field-of-view, ``R_s``, +Radius of the sky image around the source position, ``Radius`` (used in +the image preview), the exposure time in hours, ``Texp``, source +redshift ``z``, the powerlaw flux normalisation ``F0`` and the reference +energy of normalisation ``E0`` (in TeV), the slope of the powerlaw +spectrum ``Gamma``, radius of the spectral extraction region ``R_s`` +used in the count-spectrum preview. + +For the sources visible from both South and North CTA sites, it is +possible to choose between ``South`` and ``North`` sites. It is also +possible to simulate observations with different CTA sub-arrays: Large +Size Telescopes (LST), Medium Size Telescopes (MST), Small Size +Telescopes (SST). Note that in the “Production 5” Monte-Carlo +simulations of the telescope responses it was assumed that the Northern +site will host only LST and MST sub-arrays (no SST available), while the +Southern site will have MST and SST sub-arrays (no LST available). + +Four data products are generated: the Data Level 3 (DL3) event list (a +FITS file), a sky image, a “theta-square plot” showsing distribution of +gamma-like events around the the source position, and the count-spectrum +showing the excess counts as a funciton of energy. The image, spectrum +and theta-square plot are for “preview” of the event set, further +analysis of the simulated events can be done with deticated imaging and +spectral analysis tools. + +.. |DOI| image:: https://zenodo.org/badge/DOI/10.5281/zenodo.5499840.svg + :target: https://doi.org/10.5281/zenodo.5499840 +</help> + <citations> + <citation type="doi">10.1007/s10686-011-9247-0</citation> + </citations> +</tool> \ No newline at end of file