├── .github └── workflows │ └── svo_filters_workflow.yml ├── .gitignore ├── .rtd-environment.yml ├── LICENSE ├── MANIFEST.in ├── README.md ├── ci ├── install_conda.sh └── setup_conda_env.sh ├── docs ├── Makefile ├── _build │ ├── doctrees │ │ ├── README.doctree │ │ ├── environment.pickle │ │ ├── index.doctree │ │ └── svo.doctree │ └── html │ │ ├── .buildinfo │ │ ├── .nojekyll │ │ ├── _images │ │ ├── G141.png │ │ ├── H.png │ │ └── filtered.png │ │ ├── _modules │ │ ├── index.html │ │ ├── svo.html │ │ └── svo_filters │ │ │ └── svo.html │ │ ├── _sources │ │ ├── README.rst.txt │ │ ├── index.rst.txt │ │ └── svo.rst.txt │ │ ├── _static │ │ ├── ajax-loader.gif │ │ ├── alabaster.css │ │ ├── basic.css │ │ ├── comment-bright.png │ │ ├── comment-close.png │ │ ├── comment.png │ │ ├── css │ │ │ ├── badge_only.css │ │ │ └── theme.css │ │ ├── custom.css │ │ ├── doctools.js │ │ ├── documentation_options.js │ │ ├── down-pressed.png │ │ ├── down.png │ │ ├── file.png │ │ ├── fonts │ │ │ ├── Inconsolata-Bold.ttf │ │ │ ├── Inconsolata-Regular.ttf │ │ │ ├── Inconsolata.ttf │ │ │ ├── Lato-Bold.ttf │ │ │ ├── Lato-Regular.ttf │ │ │ ├── Lato │ │ │ │ ├── lato-bold.eot │ │ │ │ ├── lato-bold.ttf │ │ │ │ ├── lato-bold.woff │ │ │ │ ├── lato-bold.woff2 │ │ │ │ ├── lato-bolditalic.eot │ │ │ │ ├── lato-bolditalic.ttf │ │ │ │ ├── lato-bolditalic.woff │ │ │ │ ├── lato-bolditalic.woff2 │ │ │ │ ├── lato-italic.eot │ │ │ │ ├── lato-italic.ttf │ │ │ │ ├── lato-italic.woff │ │ │ │ ├── lato-italic.woff2 │ │ │ │ ├── lato-regular.eot │ │ │ │ ├── lato-regular.ttf │ │ │ │ ├── lato-regular.woff │ │ │ │ └── lato-regular.woff2 │ │ │ ├── RobotoSlab-Bold.ttf │ │ │ ├── RobotoSlab-Regular.ttf │ │ │ ├── RobotoSlab │ │ │ │ ├── roboto-slab-v7-bold.eot │ │ │ │ ├── roboto-slab-v7-bold.ttf │ │ │ │ ├── roboto-slab-v7-bold.woff │ │ │ │ ├── roboto-slab-v7-bold.woff2 │ │ │ │ ├── roboto-slab-v7-regular.eot │ │ │ │ ├── roboto-slab-v7-regular.ttf │ │ │ │ ├── roboto-slab-v7-regular.woff │ │ │ │ └── roboto-slab-v7-regular.woff2 │ │ │ ├── fontawesome-webfont.eot │ │ │ ├── fontawesome-webfont.svg │ │ │ ├── fontawesome-webfont.ttf │ │ │ ├── fontawesome-webfont.woff │ │ │ └── fontawesome-webfont.woff2 │ │ ├── jquery-3.2.1.js │ │ ├── jquery.js │ │ ├── js │ │ │ ├── modernizr.min.js │ │ │ └── theme.js │ │ ├── minus.png │ │ ├── plus.png │ │ ├── pygments.css │ │ ├── searchtools.js │ │ ├── underscore-1.3.1.js │ │ ├── underscore.js │ │ ├── up-pressed.png │ │ ├── up.png │ │ └── websupport.js │ │ ├── genindex.html │ │ ├── index.html │ │ ├── objects.inv │ │ ├── py-modindex.html │ │ ├── search.html │ │ ├── searchindex.js │ │ └── svo.html ├── conf.py ├── index.rst ├── make.bat └── svo.rst ├── env ├── environment-3.10.yml └── environment-3.11.yml ├── setup.py ├── svo_demo.ipynb └── svo_filters ├── __init__.py ├── data ├── filters │ ├── .gitkeep │ ├── 2MASS.H │ ├── 2MASS.J │ ├── 2MASS.Ks │ ├── ACS_HRC.F435W │ ├── ACS_HRC.F555W │ ├── ACS_HRC.F658N │ ├── ACS_HRC.F775W │ ├── ACS_HRC.F850LP │ ├── Cousins.I │ ├── Cousins.R │ ├── FourStar.J │ ├── FourStar.J1 │ ├── FourStar.J2 │ ├── FourStar.J3 │ ├── GALEX.FUV │ ├── GALEX.NUV │ ├── Gaia.G │ ├── Gaia.bp │ ├── Gaia.rp │ ├── HAWK_I.H.txt │ ├── HAWK_I.J.txt │ ├── HAWK_I.Ks.txt │ ├── IRAC.I1 │ ├── IRAC.I2 │ ├── IRAC.I3 │ ├── IRAC.I4 │ ├── Johnson.V │ ├── Kepler.K │ ├── MIRI.F1000W │ ├── MIRI.F1130W │ ├── MIRI.F1280W │ ├── MIRI.F1500W │ ├── MIRI.F1800W │ ├── MIRI.F2100W │ ├── MIRI.F2550W │ ├── MIRI.F560W │ ├── MIRI.F770W │ ├── NICMOS3.F110W │ ├── NICMOS3.F160W │ ├── NIRCam.F070W │ ├── NIRCam.F090W │ ├── NIRCam.F115W │ ├── NIRCam.F140M │ ├── NIRCam.F150W │ ├── NIRCam.F150W2 │ ├── NIRCam.F162M │ ├── NIRCam.F164N │ ├── NIRCam.F182M │ ├── NIRCam.F187N │ ├── NIRCam.F200W │ ├── NIRCam.F210M │ ├── NIRCam.F212N │ ├── NIRCam.F250M │ ├── NIRCam.F277W │ ├── NIRCam.F300M │ ├── NIRCam.F322W2 │ ├── NIRCam.F323N │ ├── NIRCam.F335M │ ├── NIRCam.F356W │ ├── NIRCam.F360M │ ├── NIRCam.F405N │ ├── NIRCam.F410M │ ├── NIRCam.F430M │ ├── NIRCam.F444W │ ├── NIRCam.F460M │ ├── NIRCam.F466N │ ├── NIRCam.F470N │ ├── NIRCam.F480M │ ├── NIRISS.F090W │ ├── NIRISS.F115W │ ├── NIRISS.F140M │ ├── NIRISS.F150W │ ├── NIRISS.F158M │ ├── NIRISS.F200W │ ├── NIRISS.F277W │ ├── NIRISS.F356W │ ├── NIRISS.F380M │ ├── NIRISS.F430M │ ├── NIRISS.F444W │ ├── NIRISS.F480M │ ├── NIRISS.GR700XD.1.txt │ ├── NIRISS.GR700XD.2.txt │ ├── NIRISS.GR700XD.3.txt │ ├── NSFCam.H │ ├── NSFCam.J │ ├── NSFCam.K │ ├── NSFCam.Lp │ ├── NSFCam.Mp │ ├── PS1.g │ ├── PS1.i │ ├── PS1.r │ ├── PS1.y │ ├── PS1.z │ ├── SDSS.g │ ├── SDSS.i │ ├── SDSS.r │ ├── SDSS.u │ ├── SDSS.z │ ├── STIS.G430L.txt │ ├── STIS.G750L.txt │ ├── WFC3_IR.F125W │ ├── WFC3_IR.G102 │ ├── WFC3_IR.G141 │ ├── WFC3_UVIS2.F814W │ ├── WFC3_UVIS2.F850LP │ ├── WFPC2.f336w │ ├── WFPC2.f439w │ ├── WFPC2.f656n │ ├── WFPC2.f814w │ ├── WISE.W1 │ ├── WISE.W2 │ ├── WISE.W3 │ ├── WISE.W4 │ └── Wircam.Y ├── plots │ ├── G141.png │ ├── H.png │ └── filtered.png └── spectra │ └── vega.txt ├── setup_package.py ├── svo.py ├── test_svo.py └── utils.py /.github/workflows/svo_filters_workflow.yml: -------------------------------------------------------------------------------- 1 | name: svo_filters Workflow 2 | 3 | on: [push] 4 | 5 | jobs: 6 | build-linux: 7 | name: Python - ${{ matrix.python-version }} 8 | runs-on: ${{ matrix.os }} 9 | strategy: 10 | max-parallel: 5 11 | matrix: 12 | os: [ubuntu-latest] 13 | python-version: ['3.10', '3.11'] 14 | steps: 15 | - uses: actions/checkout@v2 16 | - name: Set up Python 17 | uses: actions/setup-python@v2 18 | with: 19 | python-version: ${{ matrix.python-version }} 20 | - name: Add conda to system path 21 | run: | 22 | # $CONDA is an environment variable pointing to the root of the miniconda directory 23 | echo $CONDA/bin >> $GITHUB_PATH 24 | - name: Install dependencies 25 | run: | 26 | conda env update --file env/environment-${{ matrix.python-version }}.yml --name svo_filters-${{ matrix.python-version }} 27 | env: 28 | PYTHONVERSION: ${{ matrix.python-version }} 29 | - name: Test with pytest 30 | run: | 31 | conda run -n svo_filters-${{ matrix.python-version }} pytest 32 | -------------------------------------------------------------------------------- /.gitignore: -------------------------------------------------------------------------------- 1 | # Compiled files 2 | *.py[cod] 3 | __pycache__ 4 | .DS_Store 5 | 6 | # Other generated files 7 | htmlcov 8 | .coverage 9 | MANIFEST 10 | .ipynb_checkpoints 11 | 12 | build 13 | dist/* 14 | *.egg-info* 15 | .idea 16 | -------------------------------------------------------------------------------- /.rtd-environment.yml: -------------------------------------------------------------------------------- 1 | name: svo_filters 2 | 3 | channels: 4 | - astropy 5 | 6 | dependencies: 7 | - astropy 8 | - bokeh 9 | - numpy 10 | -------------------------------------------------------------------------------- /LICENSE: -------------------------------------------------------------------------------- 1 | MIT License 2 | 3 | Copyright (c) 2017 Joe Filippazzo 4 | 5 | Permission is hereby granted, free of charge, to any person obtaining a copy 6 | of this software and associated documentation files (the "Software"), to deal 7 | in the Software without restriction, including without limitation the rights 8 | to use, copy, modify, merge, publish, distribute, sublicense, and/or sell 9 | copies of the Software, and to permit persons to whom the Software is 10 | furnished to do so, subject to the following conditions: 11 | 12 | The above copyright notice and this permission notice shall be included in all 13 | copies or substantial portions of the Software. 14 | 15 | THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR 16 | IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY, 17 | FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE 18 | AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER 19 | LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM, 20 | OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE 21 | SOFTWARE. 22 | -------------------------------------------------------------------------------- /MANIFEST.in: -------------------------------------------------------------------------------- 1 | include README.md 2 | 3 | graft svo_filters/data/filters * 4 | graft svo_filters/data/plots * 5 | graft svo_filters/data/spectra * 6 | 7 | global-exclude *.pyc 8 | global-exclude *.idea 9 | -------------------------------------------------------------------------------- /ci/install_conda.sh: -------------------------------------------------------------------------------- 1 | #!/bin/bash 2 | 3 | if [ -d "$HOME/miniconda3" ] && [ -e "$HOME/miniconda3/bin/conda" ]; then 4 | echo "Miniconda install already present from cache: $HOME/miniconda3" 5 | rm -rf $HOME/miniconda3/envs/hosts # Just in case... 6 | else 7 | echo "Installing Miniconda..." 8 | rm -rf $HOME/miniconda3 # Just in case... 9 | 10 | if [ "${TRAVIS_OS_NAME}" == "osx" ]; then 11 | wget http://repo.continuum.io/miniconda/Miniconda3-latest-MacOSX-x86_64.sh -O miniconda.sh || exit 1 12 | else 13 | wget http://repo.continuum.io/miniconda/Miniconda3-latest-Linux-x86_64.sh -O miniconda.sh || exit 1 14 | fi 15 | 16 | bash miniconda.sh -b -p "$HOME/miniconda3" || exit 1 17 | fi 18 | 19 | echo "Configuring Miniconda..." 20 | conda config --set ssl_verify false || exit 1 21 | conda config --set always_yes true --set changeps1 false || exit 1 22 | 23 | echo "Updating Miniconda" 24 | conda update conda 25 | conda update --all 26 | conda info -a || exit 1 27 | 28 | echo "Installing numpy" 29 | conda install numpy -------------------------------------------------------------------------------- /ci/setup_conda_env.sh: -------------------------------------------------------------------------------- 1 | #!/bin/bash 2 | echo "Creating conda environment for Python $PYTHON_VERSION" 3 | conda env create -f "env/environment-${PYTHON_VERSION}.yml" || exit 1 4 | export CONDA_ENV=svo-filters-$PYTHON_VERSION 5 | source activate $CONDA_ENV 6 | pip install pytest pytest-cov coveralls 7 | -------------------------------------------------------------------------------- /docs/Makefile: -------------------------------------------------------------------------------- 1 | # Minimal makefile for Sphinx documentation 2 | # 3 | 4 | # You can set these variables from the command line. 5 | SPHINXOPTS = 6 | SPHINXBUILD = sphinx-build 7 | SOURCEDIR = . 8 | BUILDDIR = _build 9 | 10 | # Put it first so that "make" without argument is like "make help". 11 | help: 12 | @$(SPHINXBUILD) -M help "$(SOURCEDIR)" "$(BUILDDIR)" $(SPHINXOPTS) $(O) 13 | 14 | .PHONY: help Makefile 15 | 16 | # Catch-all target: route all unknown targets to Sphinx using the new 17 | # "make mode" option. $(O) is meant as a shortcut for $(SPHINXOPTS). 18 | %: Makefile 19 | @$(SPHINXBUILD) -M $@ "$(SOURCEDIR)" "$(BUILDDIR)" $(SPHINXOPTS) $(O) -------------------------------------------------------------------------------- /docs/_build/doctrees/README.doctree: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/doctrees/README.doctree -------------------------------------------------------------------------------- /docs/_build/doctrees/environment.pickle: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/doctrees/environment.pickle -------------------------------------------------------------------------------- /docs/_build/doctrees/index.doctree: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/doctrees/index.doctree -------------------------------------------------------------------------------- /docs/_build/doctrees/svo.doctree: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/doctrees/svo.doctree -------------------------------------------------------------------------------- /docs/_build/html/.buildinfo: -------------------------------------------------------------------------------- 1 | # Sphinx build info version 1 2 | # This file hashes the configuration used when building these files. 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174 | 175 | 176 | 177 | 178 | 179 | 180 | 181 | 182 | 183 | 184 | 185 | 186 | 187 | 188 | 189 | 190 | 191 | 196 | 197 | 198 | -------------------------------------------------------------------------------- /docs/_build/html/_sources/README.rst.txt: -------------------------------------------------------------------------------- 1 | svo_filters 2 | =========== 3 | 4 | The `Spanish Virtual Observatory (SVO) Filter Profile Service `_ is a great resource for homogenized photometric filter curves and metadata. With `svo_filters`, I tried to create a lightweight and flexible package to incorporate these filters into Python applications. 5 | 6 | Installation 7 | ------------ 8 | 9 | To install **svo_filters**, do:: 10 | 11 | pip install svo_filters 12 | 13 | Alternatively, you can clone from Github with:: 14 | 15 | git clone https://github.com/hover2pi/svo_filters.git 16 | python svo_filters/setup.py install 17 | 18 | Load a Photometric Filter 19 | ---------------------------- 20 | 21 | The actual filters are stored locally as XML files and can be viewed with:: 22 | 23 | from svo_filters import svo 24 | svo.filters() 25 | 26 | To create a filter object, pass a bandpass name to the :py:class:`svo.Filter()` class:: 27 | 28 | H_band = svo.Filter('2MASS.H') 29 | 30 | You can see someinformation about the filter with:: 31 | 32 | H_band.info() 33 | 34 | And you can plot the bandpass like so:: 35 | 36 | H_band.plot() 37 | 38 | .. image:: ../svo_filters/data/plots/H.png 39 | :align: center 40 | :height: 300px 41 | :alt: Filter bandpass 42 | 43 | Load a Grism 44 | ------------ 45 | 46 | Filters can also be binned arbitrarily, for use with grisms. We can pass integers to the ``n_bins`` or ``pixels_per_bin`` arguments to specify the number of wavelength bins or pixels per bin, respectively:: 47 | 48 | G141 = svo.Filter('WFC3_IR.G141', n_bins=15) 49 | 50 | .. image:: ../svo_filters/data/plots/G141.png 51 | :align: center 52 | :height: 300px 53 | :alt: Filter bandpass 54 | 55 | Apply a Filter to a Spectrum 56 | ---------------------------- 57 | 58 | Filters can be applied to a spectrum by passing a sequence of [W, F] or [W, F, E] with astropy units to the :py:meth:`~svo.Filter.apply` method:: 59 | 60 | filtered = G141.apply(spec, plot=True) 61 | 62 | .. image:: ../svo_filters/data/plots/filtered.png 63 | :align: center 64 | :height: 300px 65 | :alt: Filter bandpass 66 | 67 | Contents 68 | ======== 69 | 70 | .. toctree:: 71 | :maxdepth: 2 72 | 73 | svo 74 | 75 | -------------------------------------------------------------------------------- /docs/_build/html/_sources/index.rst.txt: -------------------------------------------------------------------------------- 1 | svo_filters 2 | =========== 3 | 4 | The `Spanish Virtual Observatory (SVO) Filter Profile Service `_ is a great resource for homogenized photometric filter curves and metadata. With `svo_filters`, I tried to create a lightweight and flexible package to incorporate these filters into Python applications. 5 | 6 | Installation 7 | ------------ 8 | 9 | To install **svo_filters**, do:: 10 | 11 | pip install svo_filters 12 | 13 | Alternatively, you can clone from Github with:: 14 | 15 | git clone https://github.com/hover2pi/svo_filters.git 16 | python svo_filters/setup.py install 17 | 18 | Load a Photometric Filter 19 | ---------------------------- 20 | 21 | The actual filters are stored locally as XML files and can be viewed with:: 22 | 23 | from svo_filters import svo 24 | svo.filters() 25 | 26 | To create a filter object, pass a bandpass name to the :py:class:`svo.Filter()` class:: 27 | 28 | H_band = svo.Filter('2MASS.H') 29 | 30 | You can see some information about the filter with:: 31 | 32 | H_band.info() 33 | 34 | And you can plot the bandpass like so:: 35 | 36 | H_band.plot() 37 | 38 | .. image:: ../svo_filters/data/plots/H.png 39 | :align: center 40 | :height: 300px 41 | :alt: Filter bandpass 42 | 43 | Load a Grism 44 | ------------ 45 | 46 | Filters can also be binned arbitrarily, for use with grisms. We can pass integers to the ``n_bins`` or ``pixels_per_bin`` arguments to specify the number of wavelength bins or pixels per bin, respectively:: 47 | 48 | G141 = svo.Filter('WFC3_IR.G141', n_bins=15) 49 | 50 | .. image:: ../svo_filters/data/plots/G141.png 51 | :align: center 52 | :height: 300px 53 | :alt: Filter bandpass 54 | 55 | Apply a Filter to a Spectrum 56 | ---------------------------- 57 | 58 | Filters can be applied to a spectrum by passing a sequence of [W, F] or [W, F, E] with astropy units to the :py:meth:`~svo.Filter.apply` method:: 59 | 60 | filtered = G141.apply(spec, plot=True) 61 | 62 | .. image:: ../svo_filters/data/plots/filtered.png 63 | :align: center 64 | :height: 300px 65 | :alt: Filter bandpass 66 | 67 | Contents 68 | ======== 69 | 70 | .. toctree:: 71 | :maxdepth: 2 72 | 73 | svo 74 | 75 | .. automodule:: svo 76 | -------------------------------------------------------------------------------- /docs/_build/html/_sources/svo.rst.txt: -------------------------------------------------------------------------------- 1 | svo module 2 | ========== 3 | 4 | This is the main module for `svo_filters`. 5 | 6 | .. automodule:: svo 7 | :members: 8 | :undoc-members: 9 | :show-inheritance: -------------------------------------------------------------------------------- /docs/_build/html/_static/ajax-loader.gif: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/html/_static/ajax-loader.gif -------------------------------------------------------------------------------- /docs/_build/html/_static/comment-bright.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/html/_static/comment-bright.png 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* :copyright: Copyright 2007-2018 by the Sphinx team, see AUTHORS. 8 | * :license: BSD, see LICENSE for details. 9 | * 10 | */ 11 | 12 | /** 13 | * select a different prefix for underscore 14 | */ 15 | $u = _.noConflict(); 16 | 17 | /** 18 | * make the code below compatible with browsers without 19 | * an installed firebug like debugger 20 | if (!window.console || !console.firebug) { 21 | var names = ["log", "debug", "info", "warn", "error", "assert", "dir", 22 | "dirxml", "group", "groupEnd", "time", "timeEnd", "count", "trace", 23 | "profile", "profileEnd"]; 24 | window.console = {}; 25 | for (var i = 0; i < names.length; ++i) 26 | window.console[names[i]] = function() {}; 27 | } 28 | */ 29 | 30 | /** 31 | * small helper function to urldecode strings 32 | */ 33 | jQuery.urldecode = function(x) { 34 | return decodeURIComponent(x).replace(/\+/g, ' '); 35 | }; 36 | 37 | /** 38 | * small helper function to urlencode strings 39 | */ 40 | jQuery.urlencode = encodeURIComponent; 41 | 42 | /** 43 | * This function returns the parsed url parameters of the 44 | * current request. Multiple values per key are supported, 45 | * it will always return arrays of strings for the value parts. 46 | */ 47 | jQuery.getQueryParameters = function(s) { 48 | if (typeof s === 'undefined') 49 | s = document.location.search; 50 | var parts = s.substr(s.indexOf('?') + 1).split('&'); 51 | var result = {}; 52 | for (var i = 0; i < parts.length; i++) { 53 | var tmp = parts[i].split('=', 2); 54 | var key = jQuery.urldecode(tmp[0]); 55 | var value = jQuery.urldecode(tmp[1]); 56 | if (key in result) 57 | result[key].push(value); 58 | else 59 | result[key] = [value]; 60 | } 61 | return result; 62 | }; 63 | 64 | /** 65 | * highlight a given string on a jquery object by wrapping it in 66 | * span elements with the given class name. 67 | */ 68 | jQuery.fn.highlightText = function(text, className) { 69 | function highlight(node, addItems) { 70 | if (node.nodeType === 3) { 71 | var val = node.nodeValue; 72 | var pos = val.toLowerCase().indexOf(text); 73 | if (pos >= 0 && 74 | !jQuery(node.parentNode).hasClass(className) && 75 | !jQuery(node.parentNode).hasClass("nohighlight")) { 76 | var span; 77 | var isInSVG = jQuery(node).closest("body, svg, foreignObject").is("svg"); 78 | if (isInSVG) { 79 | span = document.createElementNS("http://www.w3.org/2000/svg", "tspan"); 80 | } else { 81 | span = document.createElement("span"); 82 | span.className = className; 83 | } 84 | span.appendChild(document.createTextNode(val.substr(pos, text.length))); 85 | node.parentNode.insertBefore(span, node.parentNode.insertBefore( 86 | document.createTextNode(val.substr(pos + text.length)), 87 | node.nextSibling)); 88 | node.nodeValue = val.substr(0, pos); 89 | if (isInSVG) { 90 | var bbox = span.getBBox(); 91 | var rect = document.createElementNS("http://www.w3.org/2000/svg", "rect"); 92 | rect.x.baseVal.value = bbox.x; 93 | rect.y.baseVal.value = bbox.y; 94 | rect.width.baseVal.value = bbox.width; 95 | rect.height.baseVal.value = bbox.height; 96 | rect.setAttribute('class', className); 97 | var parentOfText = node.parentNode.parentNode; 98 | addItems.push({ 99 | "parent": node.parentNode, 100 | "target": rect}); 101 | } 102 | } 103 | } 104 | else if (!jQuery(node).is("button, select, textarea")) { 105 | jQuery.each(node.childNodes, function() { 106 | highlight(this, addItems); 107 | }); 108 | } 109 | } 110 | var addItems = []; 111 | var result = this.each(function() { 112 | highlight(this, addItems); 113 | }); 114 | for (var i = 0; i < addItems.length; ++i) { 115 | jQuery(addItems[i].parent).before(addItems[i].target); 116 | } 117 | return result; 118 | }; 119 | 120 | /* 121 | * backward compatibility for jQuery.browser 122 | * This will be supported until firefox bug is fixed. 123 | */ 124 | if (!jQuery.browser) { 125 | jQuery.uaMatch = function(ua) { 126 | ua = ua.toLowerCase(); 127 | 128 | var match = /(chrome)[ \/]([\w.]+)/.exec(ua) || 129 | /(webkit)[ \/]([\w.]+)/.exec(ua) || 130 | /(opera)(?:.*version|)[ \/]([\w.]+)/.exec(ua) || 131 | /(msie) ([\w.]+)/.exec(ua) || 132 | ua.indexOf("compatible") < 0 && /(mozilla)(?:.*? rv:([\w.]+)|)/.exec(ua) || 133 | []; 134 | 135 | return { 136 | browser: match[ 1 ] || "", 137 | version: match[ 2 ] || "0" 138 | }; 139 | }; 140 | jQuery.browser = {}; 141 | jQuery.browser[jQuery.uaMatch(navigator.userAgent).browser] = true; 142 | } 143 | 144 | /** 145 | * Small JavaScript module for the documentation. 146 | */ 147 | var Documentation = { 148 | 149 | init : function() { 150 | this.fixFirefoxAnchorBug(); 151 | this.highlightSearchWords(); 152 | this.initIndexTable(); 153 | if (DOCUMENTATION_OPTIONS.NAVIGATION_WITH_KEYS) { 154 | this.initOnKeyListeners(); 155 | } 156 | }, 157 | 158 | /** 159 | * i18n support 160 | */ 161 | TRANSLATIONS : {}, 162 | PLURAL_EXPR : function(n) { return n === 1 ? 0 : 1; }, 163 | LOCALE : 'unknown', 164 | 165 | // gettext and ngettext don't access this so that the functions 166 | // can safely bound to a different name (_ = Documentation.gettext) 167 | gettext : function(string) { 168 | var translated = Documentation.TRANSLATIONS[string]; 169 | if (typeof translated === 'undefined') 170 | return string; 171 | return (typeof translated === 'string') ? translated : translated[0]; 172 | }, 173 | 174 | ngettext : function(singular, plural, n) { 175 | var translated = Documentation.TRANSLATIONS[singular]; 176 | if (typeof translated === 'undefined') 177 | return (n == 1) ? singular : plural; 178 | return translated[Documentation.PLURALEXPR(n)]; 179 | }, 180 | 181 | addTranslations : function(catalog) { 182 | for (var key in catalog.messages) 183 | this.TRANSLATIONS[key] = catalog.messages[key]; 184 | this.PLURAL_EXPR = new Function('n', 'return +(' + catalog.plural_expr + ')'); 185 | this.LOCALE = catalog.locale; 186 | }, 187 | 188 | /** 189 | * add context elements like header anchor links 190 | */ 191 | addContextElements : function() { 192 | $('div[id] > :header:first').each(function() { 193 | $('\u00B6'). 194 | attr('href', '#' + this.id). 195 | attr('title', _('Permalink to this headline')). 196 | appendTo(this); 197 | }); 198 | $('dt[id]').each(function() { 199 | $('\u00B6'). 200 | attr('href', '#' + this.id). 201 | attr('title', _('Permalink to this definition')). 202 | appendTo(this); 203 | }); 204 | }, 205 | 206 | /** 207 | * workaround a firefox stupidity 208 | * see: https://bugzilla.mozilla.org/show_bug.cgi?id=645075 209 | */ 210 | fixFirefoxAnchorBug : function() { 211 | if (document.location.hash && $.browser.mozilla) 212 | window.setTimeout(function() { 213 | document.location.href += ''; 214 | }, 10); 215 | }, 216 | 217 | /** 218 | * highlight the search words provided in the url in the text 219 | */ 220 | highlightSearchWords : function() { 221 | var params = $.getQueryParameters(); 222 | var terms = (params.highlight) ? params.highlight[0].split(/\s+/) : []; 223 | if (terms.length) { 224 | var body = $('div.body'); 225 | if (!body.length) { 226 | body = $('body'); 227 | } 228 | window.setTimeout(function() { 229 | $.each(terms, function() { 230 | body.highlightText(this.toLowerCase(), 'highlighted'); 231 | }); 232 | }, 10); 233 | $('

' + _('Hide Search Matches') + '

') 235 | .appendTo($('#searchbox')); 236 | } 237 | }, 238 | 239 | /** 240 | * init the domain index toggle buttons 241 | */ 242 | initIndexTable : function() { 243 | var togglers = $('img.toggler').click(function() { 244 | var src = $(this).attr('src'); 245 | var idnum = $(this).attr('id').substr(7); 246 | $('tr.cg-' + idnum).toggle(); 247 | if (src.substr(-9) === 'minus.png') 248 | $(this).attr('src', src.substr(0, src.length-9) + 'plus.png'); 249 | else 250 | $(this).attr('src', src.substr(0, src.length-8) + 'minus.png'); 251 | }).css('display', ''); 252 | if (DOCUMENTATION_OPTIONS.COLLAPSE_INDEX) { 253 | togglers.click(); 254 | } 255 | }, 256 | 257 | /** 258 | * helper function to hide the search marks again 259 | */ 260 | hideSearchWords : function() { 261 | $('#searchbox .highlight-link').fadeOut(300); 262 | $('span.highlighted').removeClass('highlighted'); 263 | }, 264 | 265 | /** 266 | * make the url absolute 267 | */ 268 | makeURL : function(relativeURL) { 269 | return DOCUMENTATION_OPTIONS.URL_ROOT + '/' + relativeURL; 270 | }, 271 | 272 | /** 273 | * get the current relative url 274 | */ 275 | getCurrentURL : function() { 276 | var path = document.location.pathname; 277 | var parts = path.split(/\//); 278 | $.each(DOCUMENTATION_OPTIONS.URL_ROOT.split(/\//), function() { 279 | if (this === '..') 280 | parts.pop(); 281 | }); 282 | var url = parts.join('/'); 283 | return path.substring(url.lastIndexOf('/') + 1, path.length - 1); 284 | }, 285 | 286 | initOnKeyListeners: function() { 287 | $(document).keyup(function(event) { 288 | var activeElementType = document.activeElement.tagName; 289 | // don't navigate when in search box or textarea 290 | if (activeElementType !== 'TEXTAREA' && activeElementType !== 'INPUT' && activeElementType !== 'SELECT') { 291 | switch (event.keyCode) { 292 | case 37: // left 293 | var prevHref = $('link[rel="prev"]').prop('href'); 294 | if (prevHref) { 295 | window.location.href = prevHref; 296 | return false; 297 | } 298 | case 39: // right 299 | var nextHref = $('link[rel="next"]').prop('href'); 300 | if (nextHref) { 301 | window.location.href = nextHref; 302 | return false; 303 | } 304 | } 305 | } 306 | }); 307 | } 308 | }; 309 | 310 | // quick alias for translations 311 | _ = Documentation.gettext; 312 | 313 | $(document).ready(function() { 314 | Documentation.init(); 315 | }); 316 | -------------------------------------------------------------------------------- /docs/_build/html/_static/documentation_options.js: -------------------------------------------------------------------------------- 1 | var DOCUMENTATION_OPTIONS = { 2 | URL_ROOT: document.getElementById("documentation_options").getAttribute('data-url_root'), 3 | VERSION: '0.2.16', 4 | LANGUAGE: 'None', 5 | COLLAPSE_INDEX: false, 6 | FILE_SUFFIX: '.html', 7 | HAS_SOURCE: true, 8 | SOURCELINK_SUFFIX: '.txt', 9 | NAVIGATION_WITH_KEYS: false, 10 | SEARCH_LANGUAGE_STOP_WORDS: ["a","and","are","as","at","be","but","by","for","if","in","into","is","it","near","no","not","of","on","or","such","that","the","their","then","there","these","they","this","to","was","will","with"] 11 | }; 12 | 13 | 14 | 15 | /* Non-minified version JS is _stemmer.js if file is provided */ 16 | /** 17 | * Porter Stemmer 18 | */ 19 | var Stemmer = function() { 20 | 21 | var step2list = { 22 | ational: 'ate', 23 | tional: 'tion', 24 | enci: 'ence', 25 | anci: 'ance', 26 | izer: 'ize', 27 | bli: 'ble', 28 | alli: 'al', 29 | entli: 'ent', 30 | eli: 'e', 31 | ousli: 'ous', 32 | ization: 'ize', 33 | ation: 'ate', 34 | ator: 'ate', 35 | alism: 'al', 36 | iveness: 'ive', 37 | fulness: 'ful', 38 | ousness: 'ous', 39 | aliti: 'al', 40 | iviti: 'ive', 41 | biliti: 'ble', 42 | logi: 'log' 43 | }; 44 | 45 | var step3list = { 46 | icate: 'ic', 47 | ative: '', 48 | alize: 'al', 49 | iciti: 'ic', 50 | ical: 'ic', 51 | ful: '', 52 | ness: '' 53 | }; 54 | 55 | var c = "[^aeiou]"; // consonant 56 | var v = "[aeiouy]"; // vowel 57 | var C = c + "[^aeiouy]*"; // consonant sequence 58 | var V = v + "[aeiou]*"; // vowel sequence 59 | 60 | var mgr0 = "^(" + C + ")?" + V + C; // [C]VC... is m>0 61 | var meq1 = "^(" + C + ")?" + V + C + "(" + V + ")?$"; // [C]VC[V] is m=1 62 | var mgr1 = "^(" + C + ")?" + V + C + V + C; // [C]VCVC... is m>1 63 | var s_v = "^(" + C + ")?" + v; // vowel in stem 64 | 65 | this.stemWord = function (w) { 66 | var stem; 67 | var suffix; 68 | var firstch; 69 | var origword = w; 70 | 71 | if (w.length < 3) 72 | return w; 73 | 74 | var re; 75 | var re2; 76 | var re3; 77 | var re4; 78 | 79 | firstch = w.substr(0,1); 80 | if (firstch == "y") 81 | w = firstch.toUpperCase() + w.substr(1); 82 | 83 | // Step 1a 84 | re = /^(.+?)(ss|i)es$/; 85 | re2 = /^(.+?)([^s])s$/; 86 | 87 | if (re.test(w)) 88 | w = w.replace(re,"$1$2"); 89 | else if (re2.test(w)) 90 | w = w.replace(re2,"$1$2"); 91 | 92 | // Step 1b 93 | re = /^(.+?)eed$/; 94 | re2 = /^(.+?)(ed|ing)$/; 95 | if (re.test(w)) { 96 | var fp = re.exec(w); 97 | re = new RegExp(mgr0); 98 | if (re.test(fp[1])) { 99 | re = /.$/; 100 | w = w.replace(re,""); 101 | } 102 | } 103 | else if (re2.test(w)) { 104 | var fp = re2.exec(w); 105 | stem = fp[1]; 106 | re2 = new RegExp(s_v); 107 | if (re2.test(stem)) { 108 | w = stem; 109 | re2 = /(at|bl|iz)$/; 110 | re3 = new RegExp("([^aeiouylsz])\\1$"); 111 | re4 = new RegExp("^" + C + v + "[^aeiouwxy]$"); 112 | if (re2.test(w)) 113 | w = w + "e"; 114 | else if (re3.test(w)) { 115 | re = /.$/; 116 | w = w.replace(re,""); 117 | } 118 | else if (re4.test(w)) 119 | w = w + "e"; 120 | } 121 | } 122 | 123 | // Step 1c 124 | re = /^(.+?)y$/; 125 | if (re.test(w)) { 126 | var fp = re.exec(w); 127 | stem = fp[1]; 128 | re = new RegExp(s_v); 129 | if (re.test(stem)) 130 | w = stem + "i"; 131 | } 132 | 133 | // Step 2 134 | re = /^(.+?)(ational|tional|enci|anci|izer|bli|alli|entli|eli|ousli|ization|ation|ator|alism|iveness|fulness|ousness|aliti|iviti|biliti|logi)$/; 135 | if (re.test(w)) { 136 | var fp = re.exec(w); 137 | stem = fp[1]; 138 | suffix = fp[2]; 139 | re = new RegExp(mgr0); 140 | if (re.test(stem)) 141 | w = stem + step2list[suffix]; 142 | } 143 | 144 | // Step 3 145 | re = /^(.+?)(icate|ative|alize|iciti|ical|ful|ness)$/; 146 | if (re.test(w)) { 147 | var fp = re.exec(w); 148 | stem = fp[1]; 149 | suffix = fp[2]; 150 | re = new RegExp(mgr0); 151 | if (re.test(stem)) 152 | w = stem + step3list[suffix]; 153 | } 154 | 155 | // Step 4 156 | re = /^(.+?)(al|ance|ence|er|ic|able|ible|ant|ement|ment|ent|ou|ism|ate|iti|ous|ive|ize)$/; 157 | re2 = /^(.+?)(s|t)(ion)$/; 158 | if (re.test(w)) { 159 | var fp = re.exec(w); 160 | stem = fp[1]; 161 | re = new RegExp(mgr1); 162 | if (re.test(stem)) 163 | w = stem; 164 | } 165 | else if (re2.test(w)) { 166 | var fp = re2.exec(w); 167 | stem = fp[1] + fp[2]; 168 | re2 = new RegExp(mgr1); 169 | if (re2.test(stem)) 170 | w = stem; 171 | } 172 | 173 | // Step 5 174 | re = /^(.+?)e$/; 175 | if (re.test(w)) { 176 | var fp = re.exec(w); 177 | stem = fp[1]; 178 | re = new RegExp(mgr1); 179 | re2 = new RegExp(meq1); 180 | re3 = new RegExp("^" + C + v + "[^aeiouwxy]$"); 181 | if (re.test(stem) || (re2.test(stem) && !(re3.test(stem)))) 182 | w = stem; 183 | } 184 | re = /ll$/; 185 | re2 = new RegExp(mgr1); 186 | if (re.test(w) && re2.test(w)) { 187 | re = /.$/; 188 | w = w.replace(re,""); 189 | } 190 | 191 | // and turn initial Y back to y 192 | if (firstch == "y") 193 | w = firstch.toLowerCase() + w.substr(1); 194 | return w; 195 | } 196 | } 197 | 198 | 199 | 200 | 201 | 202 | var splitChars = (function() { 203 | var result = {}; 204 | var singles = [96, 180, 187, 191, 215, 247, 749, 885, 903, 907, 909, 930, 1014, 1648, 205 | 1748, 1809, 2416, 2473, 2481, 2526, 2601, 2609, 2612, 2615, 2653, 2702, 206 | 2706, 2729, 2737, 2740, 2857, 2865, 2868, 2910, 2928, 2948, 2961, 2971, 207 | 2973, 3085, 3089, 3113, 3124, 3213, 3217, 3241, 3252, 3295, 3341, 3345, 208 | 3369, 3506, 3516, 3633, 3715, 3721, 3736, 3744, 3748, 3750, 3756, 3761, 209 | 3781, 3912, 4239, 4347, 4681, 4695, 4697, 4745, 4785, 4799, 4801, 4823, 210 | 4881, 5760, 5901, 5997, 6313, 7405, 8024, 8026, 8028, 8030, 8117, 8125, 211 | 8133, 8181, 8468, 8485, 8487, 8489, 8494, 8527, 11311, 11359, 11687, 11695, 212 | 11703, 11711, 11719, 11727, 11735, 12448, 12539, 43010, 43014, 43019, 43587, 213 | 43696, 43713, 64286, 64297, 64311, 64317, 64319, 64322, 64325, 65141]; 214 | var i, j, start, end; 215 | for (i = 0; i < singles.length; i++) { 216 | result[singles[i]] = true; 217 | } 218 | var ranges = [[0, 47], [58, 64], [91, 94], [123, 169], [171, 177], [182, 184], [706, 709], 219 | [722, 735], [741, 747], [751, 879], [888, 889], [894, 901], [1154, 1161], 220 | [1318, 1328], [1367, 1368], [1370, 1376], [1416, 1487], [1515, 1519], [1523, 1568], 221 | [1611, 1631], [1642, 1645], [1750, 1764], [1767, 1773], [1789, 1790], [1792, 1807], 222 | [1840, 1868], [1958, 1968], [1970, 1983], [2027, 2035], [2038, 2041], [2043, 2047], 223 | [2070, 2073], [2075, 2083], [2085, 2087], [2089, 2307], [2362, 2364], [2366, 2383], 224 | [2385, 2391], [2402, 2405], [2419, 2424], [2432, 2436], [2445, 2446], [2449, 2450], 225 | [2483, 2485], [2490, 2492], [2494, 2509], [2511, 2523], [2530, 2533], [2546, 2547], 226 | [2554, 2564], [2571, 2574], [2577, 2578], [2618, 2648], [2655, 2661], [2672, 2673], 227 | [2677, 2692], [2746, 2748], [2750, 2767], [2769, 2783], [2786, 2789], [2800, 2820], 228 | [2829, 2830], [2833, 2834], [2874, 2876], [2878, 2907], [2914, 2917], [2930, 2946], 229 | [2955, 2957], [2966, 2968], [2976, 2978], [2981, 2983], [2987, 2989], [3002, 3023], 230 | [3025, 3045], [3059, 3076], [3130, 3132], [3134, 3159], [3162, 3167], [3170, 3173], 231 | [3184, 3191], [3199, 3204], [3258, 3260], [3262, 3293], [3298, 3301], [3312, 3332], 232 | [3386, 3388], [3390, 3423], [3426, 3429], [3446, 3449], [3456, 3460], [3479, 3481], 233 | [3518, 3519], [3527, 3584], [3636, 3647], [3655, 3663], [3674, 3712], [3717, 3718], 234 | [3723, 3724], [3726, 3731], [3752, 3753], [3764, 3772], [3774, 3775], [3783, 3791], 235 | [3802, 3803], [3806, 3839], [3841, 3871], [3892, 3903], [3949, 3975], [3980, 4095], 236 | [4139, 4158], [4170, 4175], [4182, 4185], [4190, 4192], [4194, 4196], [4199, 4205], 237 | [4209, 4212], [4226, 4237], [4250, 4255], [4294, 4303], [4349, 4351], [4686, 4687], 238 | [4702, 4703], [4750, 4751], [4790, 4791], [4806, 4807], [4886, 4887], [4955, 4968], 239 | [4989, 4991], [5008, 5023], [5109, 5120], [5741, 5742], [5787, 5791], [5867, 5869], 240 | [5873, 5887], [5906, 5919], [5938, 5951], [5970, 5983], [6001, 6015], [6068, 6102], 241 | [6104, 6107], [6109, 6111], [6122, 6127], [6138, 6159], [6170, 6175], [6264, 6271], 242 | [6315, 6319], [6390, 6399], [6429, 6469], [6510, 6511], [6517, 6527], [6572, 6592], 243 | [6600, 6607], [6619, 6655], [6679, 6687], [6741, 6783], [6794, 6799], [6810, 6822], 244 | [6824, 6916], [6964, 6980], [6988, 6991], [7002, 7042], [7073, 7085], [7098, 7167], 245 | [7204, 7231], [7242, 7244], [7294, 7400], [7410, 7423], [7616, 7679], [7958, 7959], 246 | [7966, 7967], [8006, 8007], [8014, 8015], [8062, 8063], [8127, 8129], [8141, 8143], 247 | [8148, 8149], [8156, 8159], [8173, 8177], [8189, 8303], [8306, 8307], [8314, 8318], 248 | [8330, 8335], [8341, 8449], [8451, 8454], [8456, 8457], [8470, 8472], [8478, 8483], 249 | [8506, 8507], [8512, 8516], [8522, 8525], [8586, 9311], [9372, 9449], [9472, 10101], 250 | [10132, 11263], [11493, 11498], [11503, 11516], [11518, 11519], [11558, 11567], 251 | [11622, 11630], [11632, 11647], [11671, 11679], [11743, 11822], [11824, 12292], 252 | [12296, 12320], [12330, 12336], [12342, 12343], [12349, 12352], [12439, 12444], 253 | [12544, 12548], [12590, 12592], [12687, 12689], [12694, 12703], [12728, 12783], 254 | [12800, 12831], [12842, 12880], [12896, 12927], [12938, 12976], [12992, 13311], 255 | [19894, 19967], [40908, 40959], [42125, 42191], [42238, 42239], [42509, 42511], 256 | [42540, 42559], [42592, 42593], [42607, 42622], 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32 | -------------------------------------------------------------------------------- /docs/_build/html/_static/up-pressed.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/html/_static/up-pressed.png -------------------------------------------------------------------------------- /docs/_build/html/_static/up.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/html/_static/up.png -------------------------------------------------------------------------------- /docs/_build/html/genindex.html: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | Index — svo_filters 0.2.16 documentation 13 | 14 | 15 | 16 | 17 | 18 | 19 | 20 | 21 | 22 | 23 | 24 | 25 | 26 | 27 | 28 | 29 | 30 | 31 | 32 | 33 | 34 | 35 | 36 | 37 | 38 | 39 | 40 | 41 |
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Index

150 | 151 |
152 | A 153 | | B 154 | | C 155 | | F 156 | | I 157 | | L 158 | | M 159 | | O 160 | | P 161 | | R 162 | | S 163 | | T 164 | | W 165 | | Z 166 | 167 |
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A

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B

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370 | © Copyright 2018, Joe Filippazzo 371 | 372 |

373 |
374 | Built with Sphinx using a theme provided by Read the Docs. 375 | 376 |
377 | 378 |
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384 | 385 | 386 | 387 | 388 | 389 | 390 | 391 | 392 | 393 | 394 | 395 | 396 | 397 | 398 | 399 | 400 | 401 | 406 | 407 | 408 | -------------------------------------------------------------------------------- /docs/_build/html/index.html: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | svo_filters — svo_filters 0.2.16 documentation 12 | 13 | 14 | 15 | 16 | 17 | 18 | 19 | 20 | 21 | 22 | 23 | 24 | 25 | 26 | 27 | 28 | 29 | 30 | 31 | 32 | 33 | 34 | 35 | 36 | 37 | 38 | 39 | 40 | 41 |
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    • 130 | 131 |
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    • 132 | 133 | 134 |
  • 135 | 136 | 137 | View page source 138 | 139 | 140 |
    • 141 | 142 |
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146 |
147 |
148 |
149 | 150 |
151 |

svo_filters

152 |

The Spanish Virtual Observatory (SVO) Filter Profile Service is a great resource for homogenized photometric filter curves and metadata. With svo_filters, I tried to create a lightweight and flexible package to incorporate these filters into Python applications.

153 |
154 |

Installation

155 |

To install svo_filters, do:

156 | 
pip install svo_filters
157 |
158 |
159 |

Alternatively, you can clone from Github with:

160 | 
git clone https://github.com/hover2pi/svo_filters.git
161 | python svo_filters/setup.py install
162 |
163 |
164 |
165 |
166 |

Load a Photometric Filter

167 |

The actual filters are stored locally as XML files and can be viewed with:

168 | 
from svo_filters import svo
169 | svo.filters()
170 |
171 |
172 |

To create a filter object, pass a bandpass name to the svo.Filter() class:

173 | 
H_band = svo.Filter('2MASS.H')
174 |
175 |
176 |

You can see some information about the filter with:

177 | 
H_band.info()
178 |
179 |
180 |

And you can plot the bandpass like so:

181 | 
H_band.plot()
182 |
183 |
184 | Filter bandpass 185 |
186 |
187 |

Load a Grism

188 |

Filters can also be binned arbitrarily, for use with grisms. We can pass integers to the n_bins or pixels_per_bin arguments to specify the number of wavelength bins or pixels per bin, respectively:

189 | 
G141 = svo.Filter('WFC3_IR.G141', n_bins=15)
190 |
191 |
192 | Filter bandpass 193 |
194 |
195 |

Apply a Filter to a Spectrum

196 |

Filters can be applied to a spectrum by passing a sequence of [W, F] or [W, F, E] with astropy units to the apply() method:

197 | 
filtered = G141.apply(spec, plot=True)
198 |
199 |
200 | Filter bandpass 201 |
202 |
203 |
204 |

Contents

205 |
206 | 209 |
210 |

A Python wrapper for the SVO Filter Profile Service

211 |
212 | 213 | 214 |
215 | 216 |
217 |
218 | 219 | 225 | 226 | 227 |
228 | 229 |
230 |

231 | © Copyright 2018, Joe Filippazzo 232 | 233 |

234 |
235 | Built with Sphinx using a theme provided by Read the Docs. 236 | 237 |
238 | 239 |
240 |
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245 | 246 | 247 | 248 | 249 | 250 | 251 | 252 | 253 | 254 | 255 | 256 | 257 | 258 | 259 | 260 | 261 | 262 | 267 | 268 | 269 | -------------------------------------------------------------------------------- /docs/_build/html/objects.inv: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/docs/_build/html/objects.inv -------------------------------------------------------------------------------- /docs/_build/html/py-modindex.html: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | Python Module Index — svo_filters 0.2.16 documentation 12 | 13 | 14 | 15 | 16 | 17 | 18 | 19 | 20 | 21 | 22 | 23 | 24 | 25 | 26 | 27 | 28 | 29 | 30 | 31 | 32 | 33 | 36 | 37 | 38 | 39 | 40 | 41 | 42 | 43 | 44 | 45 | 46 | 47 |
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Python Module Index

154 | 155 |
156 | s 157 |
158 | 159 | 160 | 161 | 163 | 164 | 165 | 168 |
 
162 | s
166 | svo 167 |
169 | 170 | 171 |
172 | 173 |
174 |
175 | 176 | 177 |
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181 | © Copyright 2018, Joe Filippazzo 182 | 183 |

184 |
185 | Built with Sphinx using a theme provided by Read the Docs. 186 | 187 |
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195 | 196 | 197 | 198 | 199 | 200 | 201 | 202 | 203 | 204 | 205 | 206 | 207 | 208 | 209 | 210 | 211 | 212 | 217 | 218 | 219 | -------------------------------------------------------------------------------- /docs/_build/html/search.html: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | Search — svo_filters 0.2.16 documentation 12 | 13 | 14 | 15 | 16 | 17 | 18 | 19 | 20 | 21 | 22 | 23 | 24 | 25 | 26 | 27 | 28 | 29 | 30 | 31 | 32 | 33 | 34 | 35 | 36 | 37 | 38 | 39 | 40 |
41 | 42 | 43 | 92 | 93 |
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171 | © Copyright 2018, Joe Filippazzo 172 | 173 |

174 |
175 | Built with Sphinx using a theme provided by Read the Docs. 176 | 177 |
178 | 179 |
180 |
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183 | 184 |
185 | 186 | 187 | 188 | 189 | 190 | 191 | 192 | 193 | 194 | 195 | 196 | 197 | 198 | 199 | 200 | 201 | 202 | 203 | 208 | 211 | 212 | 213 | 214 | 215 | 216 | 217 | -------------------------------------------------------------------------------- /docs/_build/html/searchindex.js: -------------------------------------------------------------------------------- 1 | Search.setIndex({docnames:["index","svo"],envversion:{"sphinx.domains.c":1,"sphinx.domains.changeset":1,"sphinx.domains.cpp":1,"sphinx.domains.javascript":1,"sphinx.domains.math":2,"sphinx.domains.python":1,"sphinx.domains.rst":1,"sphinx.domains.std":1,"sphinx.ext.intersphinx":1,"sphinx.ext.todo":1,"sphinx.ext.viewcode":1,sphinx:55},filenames:["index.rst","svo.rst"],objects:{"":{svo:[1,0,0,"-"]},"svo.Filter":{Band:[1,2,1,""],CalibrationReference:[1,2,1,""],FWHM:[1,2,1,""],Facility:[1,2,1,""],FilterProfileService:[1,2,1,""],MagSys:[1,2,1,""],PhotCalID:[1,2,1,""],PhotSystem:[1,2,1,""],ProfileReference:[1,2,1,""],WavelengthCen:[1,2,1,""],WavelengthEff:[1,2,1,""],WavelengthMax:[1,2,1,""],WavelengthMean:[1,2,1,""],WavelengthMin:[1,2,1,""],WavelengthPeak:[1,2,1,""],WavelengthPhot:[1,2,1,""],WavelengthPivot:[1,2,1,""],WavelengthUCD:[1,2,1,""],WavelengthUnit:[1,2,1,""],WidthEff:[1,2,1,""],ZeroPoint:[1,2,1,""],ZeroPointType:[1,2,1,""],ZeroPointUnit:[1,2,1,""],apply:[1,3,1,""],bin:[1,3,1,""],centers:[1,2,1,""],filterID:[1,2,1,""],flux_units:[1,2,1,""],info:[1,3,1,""],load_TopHat:[1,3,1,""],load_txt:[1,3,1,""],load_xml:[1,3,1,""],overlap:[1,3,1,""],path:[1,2,1,""],plot:[1,3,1,""],refs:[1,2,1,""],rsr:[1,2,1,""],throughput:[1,2,1,""],wave:[1,2,1,""],wave_units:[1,2,1,""]},svo:{Filter:[1,1,1,""],color_gen:[1,4,1,""],filters:[1,4,1,""],rebin_spec:[1,4,1,""]}},objnames:{"0":["py","module","Python module"],"1":["py","class","Python class"],"2":["py","attribute","Python attribute"],"3":["py","method","Python method"],"4":["py","function","Python function"]},objtypes:{"0":"py:module","1":"py:class","2":"py:attribute","3":"py:method","4":"py:function"},terms:{"2mass":0,"break":1,"class":[0,1],"float":1,"import":0,"int":1,"new":1,"return":1,"true":0,"while":1,And:0,The:[0,1],With:0,about:[0,1],absolut:1,actual:0,also:0,altern:0,angstrom:1,ans:1,appli:1,applic:0,arbitrarili:0,argument:0,arrai:1,ascii:1,astropi:[0,1],avail:1,averag:1,band:1,bandpass:[0,1],base:1,bin:[0,1],bokeh:1,bool:1,calcul:1,calibr:1,calibrationrefer:1,can:0,center:1,channel:1,check:1,clone:0,cm2:1,color:1,color_gen:1,colormap:1,column:1,com:0,contain:1,creat:[0,1],current:1,curv:[0,1],data:1,detail:1,dice:1,directori:1,distribut:1,each:1,effect:1,erg:1,exampl:1,facil:1,fals:1,fetch:1,fig:1,file:[0,1],filepath:1,filter:1,filter_directori:1,filterid:1,filterprofileservic:1,flexibl:0,flux:1,flux_unit:1,fmt:1,format:1,from:[0,1],full:1,fwhm:1,g102:1,g141:[0,1],gener:1,get:1,getter:1,git:0,github:0,given:1,great:0,grism:1,h_band:0,hat:1,homogen:0,hover2pi:0,http:0,incorpor:0,index:[],info:[0,1],inform:0,integ:0,kei:1,kwarg:1,lightweight:0,like:[0,1],list:1,load:1,load_tophat:1,load_txt:1,load_xml:1,local:0,magnitud:1,magsi:1,main:1,map:1,max:1,maximum:1,mean:1,metadata:[0,1],method:0,min:1,minimum:1,modul:0,n_bin:[0,1],n_pixel:1,name:[0,1],ndarrai:1,none:1,number:[0,1],object:[0,1],observatori:0,option:1,origin:1,other:1,overlap:1,oversamp:1,packag:0,page:[],palett:1,paper:1,paramet:1,partial:1,pass:0,path:1,peak:1,per:[0,1],photcalid:1,photometr:1,photon:1,photsystem:1,pickl:1,pip:0,pivot:1,pixel:[0,1],pixels_per_bin:[0,1],plot:[0,1],point:1,preserv:1,print:1,profil:[0,1],profilerefer:1,python:[0,1],quantiti:1,rang:1,rebin:1,rebin_spec:1,ref:1,refer:1,rel:1,resourc:0,respect:0,respons:1,rsr:1,search:[],see:0,self:1,sequenc:[0,1],servic:[0,1],setup:0,some:0,someinform:[],sourc:1,spanish:0,spec:[0,1],specifi:0,spectral:1,spectrum:1,standard:1,statu:1,store:[0,1],str:1,svo:0,svo_filt:1,system:1,tabl:1,telescop:1,test:1,thi:1,throughput:1,top:1,total:1,tri:0,txt:1,type:1,unit:[0,1],updat:1,use:[0,1],used:1,useful:1,valu:1,view:0,viridi:1,virtual:0,wave:1,wave_max:1,wave_min:1,wave_unit:1,wavelength:[0,1],wavelengthcen:1,wavelengtheff:1,wavelengthmax:1,wavelengthmean:1,wavelengthmin:1,wavelengthpeak:1,wavelengthphot:1,wavelengthpivot:1,wavelengthucd:1,wavelengthunit:1,wavenew:1,wavnew:1,wfc3_ir:0,which:1,width:1,widtheff:1,wrapper:[0,1],xml:0,you:0,zero:1,zeropoint:1,zeropointtyp:1,zeropointunit:1},titles:["svo_filters","svo module"],titleterms:{appli:0,content:0,document:[],filter:0,grism:0,indic:[],instal:0,load:0,modul:1,photometr:0,spectrum:0,svo:1,svo_filt:0,tabl:[],welcom:[]}}) -------------------------------------------------------------------------------- /docs/conf.py: -------------------------------------------------------------------------------- 1 | # -*- coding: utf-8 -*- 2 | # 3 | # Configuration file for the Sphinx documentation builder. 4 | # 5 | # This file does only contain a selection of the most common options. For a 6 | # full list see the documentation: 7 | # http://www.sphinx-doc.org/en/master/config 8 | 9 | # -- Path setup -------------------------------------------------------------- 10 | 11 | # If extensions (or modules to document with autodoc) are in another directory, 12 | # add these directories to sys.path here. If the directory is relative to the 13 | # documentation root, use os.path.abspath to make it absolute, like shown here. 14 | # 15 | import os 16 | import sys 17 | sys.path.insert(0, os.path.abspath('.')) 18 | sys.path.append(os.path.abspath('../svo_filters/')) 19 | 20 | # -- Project information ----------------------------------------------------- 21 | 22 | project = 'svo_filters' 23 | copyright = '2018, Joe Filippazzo' 24 | author = 'Joe Filippazzo' 25 | 26 | # The short X.Y version 27 | version = '0.2' 28 | # The full version, including alpha/beta/rc tags 29 | release = '0.2.16' 30 | 31 | 32 | # -- General configuration --------------------------------------------------- 33 | 34 | # If your documentation needs a minimal Sphinx version, state it here. 35 | # 36 | # needs_sphinx = '1.0' 37 | 38 | # Add any Sphinx extension module names here, as strings. They can be 39 | # extensions coming with Sphinx (named 'sphinx.ext.*') or your custom 40 | # ones. 41 | extensions = [ 42 | 'sphinx.ext.autodoc', 43 | 'sphinx.ext.doctest', 44 | 'sphinx.ext.napoleon', 45 | 'sphinx.ext.autosummary', 46 | 'sphinx.ext.intersphinx', 47 | 'sphinx.ext.todo', 48 | 'sphinx.ext.coverage', 49 | 'sphinx.ext.mathjax', 50 | 'sphinx.ext.ifconfig', 51 | 'sphinx.ext.viewcode', 52 | 'sphinx.ext.githubpages', 53 | ] 54 | 55 | # Add any paths that contain templates here, relative to this directory. 56 | templates_path = ['_templates'] 57 | 58 | # The suffix(es) of source filenames. 59 | # You can specify multiple suffix as a list of string: 60 | # 61 | # source_suffix = ['.rst', '.md'] 62 | source_suffix = '.rst' 63 | 64 | # The master toctree document. 65 | master_doc = 'index' 66 | 67 | # The language for content autogenerated by Sphinx. Refer to documentation 68 | # for a list of supported languages. 69 | # 70 | # This is also used if you do content translation via gettext catalogs. 71 | # Usually you set "language" from the command line for these cases. 72 | language = None 73 | 74 | # List of patterns, relative to source directory, that match files and 75 | # directories to ignore when looking for source files. 76 | # This pattern also affects html_static_path and html_extra_path. 77 | exclude_patterns = ['_build', 'Thumbs.db', '.DS_Store'] 78 | 79 | # The name of the Pygments (syntax highlighting) style to use. 80 | pygments_style = None 81 | 82 | 83 | # -- Options for HTML output ------------------------------------------------- 84 | 85 | # The theme to use for HTML and HTML Help pages. See the documentation for 86 | # a list of builtin themes. 87 | # 88 | # html_theme = 'alabaster' 89 | # The theme to use for HTML and HTML Help pages. See the documentation for 90 | # a list of builtin themes. 91 | on_rtd = os.environ.get('READTHEDOCS', None) == 'True' 92 | if not on_rtd: # only import and set the theme if we're building docs locally 93 | import sphinx_rtd_theme 94 | html_theme = 'sphinx_rtd_theme' 95 | html_theme_path = [sphinx_rtd_theme.get_html_theme_path()] 96 | 97 | # Theme options are theme-specific and customize the look and feel of a theme 98 | # further. For a list of options available for each theme, see the 99 | # documentation. 100 | # 101 | # html_theme_options = {} 102 | 103 | # Add any paths that contain custom static files (such as style sheets) here, 104 | # relative to this directory. They are copied after the builtin static files, 105 | # so a file named "default.css" will overwrite the builtin "default.css". 106 | html_static_path = ['_static'] 107 | 108 | # Custom sidebar templates, must be a dictionary that maps document names 109 | # to template names. 110 | # 111 | # The default sidebars (for documents that don't match any pattern) are 112 | # defined by theme itself. Builtin themes are using these templates by 113 | # default: ``['localtoc.html', 'relations.html', 'sourcelink.html', 114 | # 'searchbox.html']``. 115 | # 116 | # html_sidebars = {} 117 | 118 | 119 | # -- Options for HTMLHelp output --------------------------------------------- 120 | 121 | # Output file base name for HTML help builder. 122 | htmlhelp_basename = 'svo_filtersdoc' 123 | 124 | 125 | # -- Options for LaTeX output ------------------------------------------------ 126 | 127 | latex_elements = { 128 | # The paper size ('letterpaper' or 'a4paper'). 129 | # 130 | # 'papersize': 'letterpaper', 131 | 132 | # The font size ('10pt', '11pt' or '12pt'). 133 | # 134 | # 'pointsize': '10pt', 135 | 136 | # Additional stuff for the LaTeX preamble. 137 | # 138 | # 'preamble': '', 139 | 140 | # Latex figure (float) alignment 141 | # 142 | # 'figure_align': 'htbp', 143 | } 144 | 145 | # Grouping the document tree into LaTeX files. List of tuples 146 | # (source start file, target name, title, 147 | # author, documentclass [howto, manual, or own class]). 148 | latex_documents = [ 149 | (master_doc, 'svo_filters.tex', 'svo\\_filters Documentation', 150 | 'Joe Filippazzo', 'manual'), 151 | ] 152 | 153 | 154 | # -- Options for manual page output ------------------------------------------ 155 | 156 | # One entry per manual page. List of tuples 157 | # (source start file, name, description, authors, manual section). 158 | man_pages = [ 159 | (master_doc, 'svo_filters', 'svo_filters Documentation', 160 | [author], 1) 161 | ] 162 | 163 | 164 | # -- Options for Texinfo output ---------------------------------------------- 165 | 166 | # Grouping the document tree into Texinfo files. List of tuples 167 | # (source start file, target name, title, author, 168 | # dir menu entry, description, category) 169 | texinfo_documents = [ 170 | (master_doc, 'svo_filters', 'svo_filters Documentation', 171 | author, 'svo_filters', 'A Python wrapper for the SVO Filter Profile Service', 172 | 'Miscellaneous'), 173 | ] 174 | 175 | 176 | # -- Options for Epub output ------------------------------------------------- 177 | 178 | # Bibliographic Dublin Core info. 179 | epub_title = project 180 | 181 | # The unique identifier of the text. This can be a ISBN number 182 | # or the project homepage. 183 | # 184 | # epub_identifier = '' 185 | 186 | # A unique identification for the text. 187 | # 188 | # epub_uid = '' 189 | 190 | # A list of files that should not be packed into the epub file. 191 | epub_exclude_files = ['search.html'] 192 | 193 | 194 | # -- Extension configuration ------------------------------------------------- 195 | 196 | # -- Options for intersphinx extension --------------------------------------- 197 | 198 | # Example configuration for intersphinx: refer to the Python standard library. 199 | intersphinx_mapping = {'https://docs.python.org/': None} 200 | 201 | # -- Options for todo extension ---------------------------------------------- 202 | 203 | # If true, `todo` and `todoList` produce output, else they produce nothing. 204 | todo_include_todos = True -------------------------------------------------------------------------------- /docs/index.rst: -------------------------------------------------------------------------------- 1 | svo_filters 2 | =========== 3 | 4 | The `Spanish Virtual Observatory (SVO) Filter Profile Service `_ is a great resource for homogenized photometric filter curves and metadata. With `svo_filters`, I tried to create a lightweight and flexible package to incorporate these filters into Python applications. 5 | 6 | Installation 7 | ------------ 8 | 9 | To install **svo_filters**, do:: 10 | 11 | pip install svo_filters 12 | 13 | Alternatively, you can clone from Github with:: 14 | 15 | git clone https://github.com/hover2pi/svo_filters.git 16 | python svo_filters/setup.py install 17 | 18 | Load a Photometric Filter 19 | ---------------------------- 20 | 21 | The actual filters are stored locally as XML files and can be viewed with:: 22 | 23 | from svo_filters import svo 24 | svo.filters() 25 | 26 | To create a filter object, pass a bandpass name to the :py:class:`svo.Filter()` class:: 27 | 28 | H_band = svo.Filter('2MASS.H') 29 | 30 | You can see some information about the filter with:: 31 | 32 | H_band.info() 33 | 34 | And you can plot the bandpass like so:: 35 | 36 | H_band.plot() 37 | 38 | .. image:: ../svo_filters/data/plots/H.png 39 | :align: center 40 | :height: 300px 41 | :alt: Filter bandpass 42 | 43 | Load a Grism 44 | ------------ 45 | 46 | Filters can also be binned arbitrarily, for use with grisms. We can pass integers to the ``n_bins`` or ``pixels_per_bin`` arguments to specify the number of wavelength bins or pixels per bin, respectively:: 47 | 48 | G141 = svo.Filter('WFC3_IR.G141', n_bins=15) 49 | 50 | .. image:: ../svo_filters/data/plots/G141.png 51 | :align: center 52 | :height: 300px 53 | :alt: Filter bandpass 54 | 55 | Apply a Filter to a Spectrum 56 | ---------------------------- 57 | 58 | Filters can be applied to a spectrum by passing a sequence of [W, F] or [W, F, E] with astropy units to the :py:meth:`~svo.Filter.apply` method:: 59 | 60 | filtered = G141.apply(spec, plot=True) 61 | 62 | .. image:: ../svo_filters/data/plots/filtered.png 63 | :align: center 64 | :height: 300px 65 | :alt: Filter bandpass 66 | 67 | Contents 68 | ======== 69 | 70 | .. toctree:: 71 | :maxdepth: 2 72 | 73 | svo 74 | 75 | .. automodule:: svo 76 | -------------------------------------------------------------------------------- /docs/make.bat: -------------------------------------------------------------------------------- 1 | @ECHO OFF 2 | 3 | pushd %~dp0 4 | 5 | REM Command file for Sphinx documentation 6 | 7 | if "%SPHINXBUILD%" == "" ( 8 | set SPHINXBUILD=sphinx-build 9 | ) 10 | set SOURCEDIR=. 11 | set BUILDDIR=_build 12 | 13 | if "%1" == "" goto help 14 | 15 | %SPHINXBUILD% >NUL 2>NUL 16 | if errorlevel 9009 ( 17 | echo. 18 | echo.The 'sphinx-build' command was not found. Make sure you have Sphinx 19 | echo.installed, then set the SPHINXBUILD environment variable to point 20 | echo.to the full path of the 'sphinx-build' executable. Alternatively you 21 | echo.may add the Sphinx directory to PATH. 22 | echo. 23 | echo.If you don't have Sphinx installed, grab it from 24 | echo.http://sphinx-doc.org/ 25 | exit /b 1 26 | ) 27 | 28 | %SPHINXBUILD% -M %1 %SOURCEDIR% %BUILDDIR% %SPHINXOPTS% 29 | goto end 30 | 31 | :help 32 | %SPHINXBUILD% -M help %SOURCEDIR% %BUILDDIR% %SPHINXOPTS% 33 | 34 | :end 35 | popd 36 | -------------------------------------------------------------------------------- /docs/svo.rst: -------------------------------------------------------------------------------- 1 | svo module 2 | ========== 3 | 4 | This is the main module for `svo_filters`. 5 | 6 | .. automodule:: svo 7 | :members: 8 | :undoc-members: 9 | :show-inheritance: -------------------------------------------------------------------------------- /env/environment-3.10.yml: -------------------------------------------------------------------------------- 1 | name: svo_filters-3.10 2 | channels: 3 | - defaults 4 | - http://ssb.stsci.edu/astroconda 5 | dependencies: 6 | - astropy>=5.3.1 7 | - bokeh>=3.2.1 8 | - matplotlib 9 | - numpy>=1.25.1 10 | - numpydoc=1.1.0 11 | - pytest>=7.4.0 12 | - python>=3.10 13 | - pip: 14 | - PyYAML>=5.4 15 | - sphinx_astropy==1.3 16 | - astroquery -------------------------------------------------------------------------------- /env/environment-3.11.yml: -------------------------------------------------------------------------------- 1 | name: svo_filters-3.11 2 | channels: 3 | - defaults 4 | - http://ssb.stsci.edu/astroconda 5 | dependencies: 6 | - astropy>=5.3.1 7 | - bokeh>=3.2.1 8 | - matplotlib 9 | - numpy>=1.25.1 10 | - numpydoc=1.1.0 11 | - pytest>=7.4.0 12 | - python>=3.9 13 | - pip: 14 | - PyYAML>=5.4 15 | - sphinx_astropy==1.3 16 | - astroquery -------------------------------------------------------------------------------- /setup.py: -------------------------------------------------------------------------------- 1 | #!/usr/bin/env python 2 | import os 3 | from setuptools import setup, find_packages 4 | 5 | REQUIRES = ['astropy', 6 | 'bokeh', 7 | 'ipython', 8 | 'matplotlib', 9 | 'numpy', 10 | 'numpydoc', 11 | 'pytest', 12 | 'pyyaml'] 13 | 14 | DEPENDENCY_LINKS = [ 15 | 'git+https://github.com/astropy/astroquery.git@ccc96185beeff86f3a12a31a00a801afcebe1dbe'] 16 | 17 | FILES = [] 18 | for root, _, files in os.walk("svo_filters"): 19 | FILES += [os.path.join(root.replace("svo_filters/", ""), fname) 20 | for fname in files if not fname.endswith(".py") and not fname.endswith(".pyc")] 21 | 22 | setup( 23 | name='svo_filters', 24 | version='0.5.2', 25 | description='A Python wrapper for the SVO Filter Profile Service', 26 | packages=find_packages( 27 | ".", 28 | exclude=["*.tests"]), 29 | package_data={ 30 | 'svo_filters': FILES}, 31 | install_requires=REQUIRES, 32 | dependency_links=DEPENDENCY_LINKS, 33 | author='Joe Filippazzo', 34 | author_email='jfilippazzo@stsci.edu', 35 | license='MIT', 36 | url='https://github.com/hover2pi/svo_filters', 37 | long_description='', 38 | zip_safe=True, 39 | use_2to3=False) 40 | -------------------------------------------------------------------------------- /svo_filters/__init__.py: -------------------------------------------------------------------------------- 1 | from .svo import Filter -------------------------------------------------------------------------------- /svo_filters/data/filters/.gitkeep: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/svo_filters/data/filters/.gitkeep -------------------------------------------------------------------------------- /svo_filters/data/filters/2MASS.H: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | Photometric system 13 | 14 | 15 | 16 | Observational facility 17 | 18 | 19 | 20 | 21 | 22 | Manually specified. See reference 23 | 24 | 25 | Manually specified. See reference 26 | 27 | 28 | Minimum filter wavelength. Defined as the first lambda value with a transmission at least 1% of maximum transmission 29 | 30 | 31 | Maximum filter wavelength. Defined as the last lambda value with a transmission at least 1% of maximum transmission 32 | 33 | 34 | Effective width. Defined as integ[x*filter(x) dx].\nEquivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve. 35 | 36 | 37 | Central wavelength. Defined as the central wavelength between the two points defining FWMH 38 | 39 | 40 | Peak wavelength. Defined as sqrt{integ[x*filter(x) dx]/integ[filter(x) dx/x]} 41 | 42 | 43 | Peak wavelength. Defined as the lambda value with larger transmission 44 | 45 | 46 | Photon distribution based effective wavelength. Defined as integ[x^2*filter(x)*vega(x) dx]/integ[x*filter(x)*vega(x) dx] 47 | 48 | 49 | Full width at half maximum. Defined as the difference between the two wavelengths for which filter transmission is half maximum 50 | 51 | 52 | 53 | 54 | 55 | 56 | 57 | 58 | 59 | 60 | 61 | 62 | 63 | 64 | 65 | 66 | 67 | 68 | 69 | 70 | 71 | 72 | 73 | 74 | 75 | 76 | 77 | 78 | 79 | 80 | 81 | 82 | 83 | 84 | 85 | 86 | 87 | 88 | 89 | 90 | 91 | 92 | 93 | 94 | 95 | 96 | 97 | 98 | 99 | 100 | 101 | 102 | 103 | 104 | 105 | 106 | 107 | 108 | 109 | 110 | 111 | 112 | 113 | 114 | 115 | 116 | 117 | 118 | 119 | 120 | 121 | 122 | 123 | 124 | 125 | 126 | 127 | 128 | 129 | 130 | 131 | 132 | 133 | 134 | 135 | 136 | 137 | 138 | 139 | 140 | 141 | 142 | 143 | 144 | 145 | 146 | 147 | 148 | 149 | 150 | 151 | 152 | 153 | 154 | 155 | 156 | 157 | 158 | 159 | 160 | 161 | 162 | 163 | 164 | 165 | 166 | 167 | 168 | 169 | 170 | 171 | 172 | 173 | 174 | 175 | 176 | 177 | 178 | 179 | 180 | 181 | 182 | 183 | 184 | 185 | 186 | 187 | 188 | 189 | 190 | 191 | 192 | 193 | 194 | 195 | 196 | 197 | 198 | 199 | 200 | 201 | 202 | 203 | 204 | 205 | 206 | 207 | 208 | 209 | 210 | 211 | 212 | 213 | 214 | 215 | 216 | 217 | 218 | 219 | 220 | 221 | 222 | 223 | 224 | 225 | 226 | 227 | 228 | 229 | 230 | 231 | 232 | 233 | 234 | 235 | 236 | 237 | 238 | 239 | 240 | 241 | 242 | 243 | 244 | 245 | 246 | 247 | 248 | 249 | 250 | 251 | 252 | 253 | 254 | 255 | 256 | 257 | 258 | 259 | 260 | 261 | 262 | 263 | 264 | 265 | 266 | 267 | 268 | 269 | 270 | 271 | 272 | 273 | 274 | 275 | 276 | 277 | 278 | 279 | 280 | 281 | 282 | 283 | 284 | 285 | 286 | 287 | 288 | 289 | 290 | 291 | 292 | 293 | 294 |
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295 | 296 | 297 | -------------------------------------------------------------------------------- /svo_filters/data/filters/Cousins.I: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | Photometric system 13 | 14 | 15 | 16 | 17 | 18 | Mean wavelength. Defined as integ[x*filter(x) dx]/integ[filter(x) dx] 19 | 20 | 21 | Effective wavelength. Defined as integ[x*filter(x)*vega(x) dx]/integ[filter(x)*vega(x) dx] 22 | 23 | 24 | Minimum filter wavelength. Defined as the first lambda value with a transmission at least 1% of maximum transmission 25 | 26 | 27 | Maximum filter wavelength. Defined as the last lambda value with a transmission at least 1% of maximum transmission 28 | 29 | 30 | Effective width. Defined as integ[x*filter(x) dx].\nEquivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve. 31 | 32 | 33 | Central wavelength. Defined as the central wavelength between the two points defining FWMH 34 | 35 | 36 | Peak wavelength. Defined as sqrt{integ[x*filter(x) dx]/integ[filter(x) dx/x]} 37 | 38 | 39 | Peak wavelength. Defined as the lambda value with larger transmission 40 | 41 | 42 | Photon distribution based effective wavelength. Defined as integ[x^2*filter(x)*vega(x) dx]/integ[x*filter(x)*vega(x) dx] 43 | 44 | 45 | Full width at half maximum. Defined as the difference between the two wavelengths for which filter transmission is half maximum 46 | 47 | 48 | 49 | 50 | 51 | 52 | 53 | 54 | 55 | 56 | 57 | 58 | 59 | 60 | 61 | 62 | 63 | 64 | 65 | 66 | 67 | 68 | 69 | 70 | 71 | 72 | 73 | 74 | 75 | 76 | 77 | 78 | 79 | 80 | 81 | 82 | 83 | 84 | 85 | 86 | 87 | 88 | 89 | 90 | 91 | 92 | 93 | 94 | 95 | 96 | 97 | 98 | 99 | 100 | 101 | 102 | 103 | 104 | 105 | 106 | 107 | 108 | 109 | 110 | 111 | 112 | 113 | 114 | 115 | 116 | 117 | 118 | 119 | 120 | 121 | 122 | 123 | 124 | 125 | 126 | 127 | 128 | 129 | 130 | 131 | 132 | 133 | 134 | 135 | 136 | 137 | 138 | 139 | 140 | 141 | 142 | 143 | 144 | 145 | 146 | 147 | 148 | 149 | 150 | 151 | 152 | 153 | 154 | 155 | 156 | 157 | 158 | 159 | 160 | 161 | 162 | 163 | 164 | 165 | 166 | 167 | 168 | 169 | 170 | 171 | 172 | 173 | 174 | 175 | 176 | 177 | 178 | 179 | 180 | 181 | 182 | 183 | 184 | 185 | 186 | 187 | 188 | 189 | 190 | 191 | 192 | 193 | 194 | 195 | 196 | 197 | 198 | 199 | 200 | 201 | 202 | 203 | 204 | 205 | 206 | 207 | 208 | 209 | 210 | 211 | 212 | 213 | 214 | 215 | 216 | 217 | 218 | 219 | 220 | 221 | 222 | 223 | 224 | 225 | 226 | 227 | 228 | 229 | 230 |
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231 | 232 | 233 | -------------------------------------------------------------------------------- /svo_filters/data/filters/Cousins.R: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | Photometric system 13 | 14 | 15 | 16 | 17 | 18 | Mean wavelength. Defined as integ[x*filter(x) dx]/integ[filter(x) dx] 19 | 20 | 21 | Effective wavelength. Defined as integ[x*filter(x)*vega(x) dx]/integ[filter(x)*vega(x) dx] 22 | 23 | 24 | Minimum filter wavelength. Defined as the first lambda value with a transmission at least 1% of maximum transmission 25 | 26 | 27 | Maximum filter wavelength. Defined as the last lambda value with a transmission at least 1% of maximum transmission 28 | 29 | 30 | Effective width. Defined as integ[x*filter(x) dx].\nEquivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve. 31 | 32 | 33 | Central wavelength. Defined as the central wavelength between the two points defining FWMH 34 | 35 | 36 | Peak wavelength. Defined as sqrt{integ[x*filter(x) dx]/integ[filter(x) dx/x]} 37 | 38 | 39 | Peak wavelength. Defined as the lambda value with larger transmission 40 | 41 | 42 | Photon distribution based effective wavelength. Defined as integ[x^2*filter(x)*vega(x) dx]/integ[x*filter(x)*vega(x) dx] 43 | 44 | 45 | Full width at half maximum. Defined as the difference between the two wavelengths for which filter transmission is half maximum 46 | 47 | 48 | 49 | 50 | 51 | 52 | 53 | 54 | 55 | 56 | 57 | 58 | 59 | 60 | 61 | 62 | 63 | 64 | 65 | 66 | 67 | 68 | 69 | 70 | 71 | 72 | 73 | 74 | 75 | 76 | 77 | 78 | 79 | 80 | 81 | 82 | 83 | 84 | 85 | 86 | 87 | 88 | 89 | 90 | 91 | 92 | 93 | 94 | 95 | 96 | 97 | 98 | 99 | 100 | 101 | 102 | 103 | 104 | 105 | 106 | 107 | 108 | 109 | 110 | 111 | 112 | 113 | 114 | 115 | 116 | 117 | 118 | 119 | 120 | 121 | 122 | 123 | 124 | 125 | 126 | 127 | 128 | 129 | 130 | 131 | 132 | 133 | 134 | 135 | 136 | 137 | 138 | 139 | 140 | 141 | 142 | 143 | 144 | 145 | 146 | 147 | 148 | 149 | 150 | 151 | 152 | 153 | 154 | 155 | 156 | 157 | 158 | 159 | 160 | 161 | 162 | 163 | 164 | 165 | 166 | 167 | 168 | 169 | 170 | 171 | 172 | 173 | 174 | 175 | 176 | 177 | 178 | 179 | 180 | 181 | 182 | 183 | 184 | 185 | 186 | 187 | 188 | 189 | 190 | 191 | 192 | 193 | 194 | 195 | 196 | 197 | 198 | 199 | 200 | 201 | 202 | 203 | 204 | 205 | 206 | 207 | 208 | 209 | 210 | 211 | 212 | 213 | 214 | 215 | 216 | 217 | 218 | 219 | 220 | 221 | 222 | 223 | 224 | 225 | 226 | 227 | 228 | 229 | 230 | 231 | 232 | 233 | 234 | 235 | 236 | 237 | 238 | 239 | 240 | 241 | 242 | 243 | 244 | 245 | 246 | 247 | 248 | 249 | 250 | 251 | 252 | 253 | 254 | 255 | 256 | 257 | 258 | 259 | 260 | 261 | 262 | 263 | 264 | 265 | 266 | 267 | 268 | 269 | 270 |
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271 | 272 | 273 | -------------------------------------------------------------------------------- /svo_filters/data/filters/Johnson.V: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | Photometric system 13 | 14 | 15 | 16 | 17 | Mean wavelength. Defined as integ[x*filter(x) dx]/integ[filter(x) dx] 18 | 19 | 20 | Effective wavelength. Defined as integ[x*filter(x)*vega(x) dx]/integ[filter(x)*vega(x) dx] 21 | 22 | 23 | Minimum filter wavelength. Defined as the first lambda value with a transmission at least 1% of maximum transmission 24 | 25 | 26 | Maximum filter wavelength. Defined as the last lambda value with a transmission at least 1% of maximum transmission 27 | 28 | 29 | Effective width. Defined as integ[x*filter(x) dx].\nEquivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve. 30 | 31 | 32 | Central wavelength. Defined as the central wavelength between the two points defining FWMH 33 | 34 | 35 | Peak wavelength. Defined as sqrt{integ[x*filter(x) dx]/integ[filter(x) dx/x]} 36 | 37 | 38 | Peak wavelength. Defined as the lambda value with larger transmission 39 | 40 | 41 | Photon distribution based effective wavelength. Defined as integ[x^2*filter(x)*vega(x) dx]/integ[x*filter(x)*vega(x) dx] 42 | 43 | 44 | Full width at half maximum. Defined as the difference between the two wavelengths for which filter transmission is half maximum 45 | 46 | 47 | 48 | 49 | 50 | 51 | 52 | 53 | 54 | 55 | 56 | 57 | 58 | 59 | 60 | 61 | 62 | 63 | 64 | 65 | 66 | 67 | 68 | 69 | 70 | 71 | 72 | 73 | 74 | 75 | 76 | 77 | 78 | 79 | 80 | 81 | 82 | 83 | 84 | 85 | 86 | 87 | 88 | 89 | 90 | 91 | 92 | 93 | 94 | 95 | 96 | 97 | 98 | 99 | 100 | 101 | 102 | 103 | 104 | 105 | 106 | 107 | 108 | 109 | 110 | 111 | 112 | 113 | 114 | 115 | 116 | 117 |
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5600.00.7200000000
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6400.00.0800000000
6600.00.0200000000
6800.00.0100000000
7000.00.0100000000
7200.00.0100000000
7400.00.0000000000
118 | 119 | 120 | -------------------------------------------------------------------------------- /svo_filters/data/filters/NIRCam.F164N: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | Photometric system 13 | 14 | 15 | Detector type 16 | 17 | 18 | Instrument 19 | 20 | 21 | Observational facility 22 | 23 | 24 | 25 | 26 | 27 | Mean wavelength. Defined as integ[x*filter(x) dx]/integ[filter(x) dx] 28 | 29 | 30 | Effective wavelength. Defined as integ[x*filter(x)*vega(x) dx]/integ[filter(x)*vega(x) dx] 31 | 32 | 33 | Minimum filter wavelength. Defined as the first lambda value with a transmission at least 1% of maximum transmission 34 | 35 | 36 | Maximum filter wavelength. Defined as the last lambda value with a transmission at least 1% of maximum transmission 37 | 38 | 39 | Effective width. Defined as integ[x*filter(x) dx].\nEquivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve. 40 | 41 | 42 | Central wavelength. Defined as the central wavelength between the two points defining FWMH 43 | 44 | 45 | Peak wavelength. Defined as sqrt{integ[x*filter(x) dx]/integ[filter(x) dx/x]} 46 | 47 | 48 | Peak wavelength. Defined as the lambda value with larger transmission 49 | 50 | 51 | Photon distribution based effective wavelength. Defined as integ[x^2*filter(x)*vega(x) dx]/integ[x*filter(x)*vega(x) dx] 52 | 53 | 54 | Full width at half maximum. Defined as the difference between the two wavelengths for which filter transmission is half maximum 55 | 56 | 57 | 58 | 59 | 60 | 61 | 62 | 63 | 64 | 65 | 66 | 67 | 68 | 69 | 70 | 71 | 72 | 73 | 74 | 75 | 76 | 77 | 78 | 79 | 80 | 81 | 82 | 83 | 84 | 85 | 86 | 87 | 88 | 89 | 90 | 91 | 92 | 93 | 94 | 95 | 96 | 97 | 98 | 99 | 100 | 101 | 102 | 103 | 104 | 105 | 106 | 107 | 108 | 109 | 110 | 111 | 112 | 113 | 114 | 115 | 116 | 117 | 118 | 119 | 120 | 121 | 122 | 123 | 124 | 125 | 126 | 127 | 128 | 129 | 130 | 131 | 132 | 133 | 134 | 135 | 136 | 137 | 138 | 139 | 140 | 141 | 142 | 143 | 144 | 145 | 146 | 147 | 148 | 149 | 150 | 151 | 152 | 153 | 154 | 155 | 156 | 157 | 158 | 159 | 160 | 161 | 162 | 163 | 164 | 165 | 166 | 167 | 168 | 169 | 170 | 171 | 172 | 173 | 174 | 175 | 176 | 177 | 178 | 179 | 180 | 181 | 182 | 183 | 184 | 185 | 186 | 187 | 188 | 189 | 190 | 191 | 192 | 193 | 194 | 195 | 196 | 197 | 198 | 199 | 200 | 201 | 202 | 203 | 204 | 205 | 206 | 207 | 208 | 209 | 210 | 211 | 212 | 213 | 214 | 215 | 216 | 217 | 218 | 219 | 220 | 221 | 222 | 223 | 224 | 225 | 226 | 227 | 228 | 229 | 230 | 231 | 232 | 233 | 234 | 235 | 236 | 237 | 238 | 239 | 240 | 241 | 242 | 243 | 244 | 245 | 246 | 247 | 248 | 249 | 250 | 251 | 252 | 253 | 254 | 255 | 256 | 257 | 258 | 259 | 260 | 261 | 262 | 263 | 264 | 265 | 266 | 267 | 268 | 269 | 270 | 271 | 272 | 273 | 274 | 275 | 276 | 277 | 278 | 279 | 280 | 281 | 282 | 283 | 284 | 285 | 286 | 287 | 288 | 289 | 290 | 291 | 292 | 293 | 294 | 295 | 296 | 297 | 298 | 299 | 300 | 301 | 302 | 303 | 304 | 305 | 306 | 307 | 308 | 309 | 310 | 311 | 312 | 313 | 314 | 315 | 316 | 317 | 318 | 319 | 320 | 321 | 322 | 323 | 324 | 325 | 326 | 327 | 328 | 329 | 330 | 331 | 332 | 333 | 334 | 335 | 336 | 337 | 338 | 339 | 340 | 341 | 342 | 343 | 344 | 345 | 346 | 347 | 348 | 349 | 350 | 351 | 352 | 353 | 354 | 355 |
160940.000131894
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356 | 357 | 358 | -------------------------------------------------------------------------------- /svo_filters/data/filters/SDSS.u: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | Photometric system 13 | 14 | 15 | Observational facility 16 | 17 | 18 | 19 | 20 | 21 | Mean wavelength. Defined as integ[x*filter(x) dx]/integ[filter(x) dx] 22 | 23 | 24 | Effective wavelength. Defined as integ[x*filter(x)*vega(x) dx]/integ[filter(x)*vega(x) dx] 25 | 26 | 27 | Minimum filter wavelength. Defined as the first lambda value with a transmission at least 1% of maximum transmission 28 | 29 | 30 | Maximum filter wavelength. Defined as the last lambda value with a transmission at least 1% of maximum transmission 31 | 32 | 33 | Effective width. Defined as integ[x*filter(x) dx].\nEquivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve. 34 | 35 | 36 | Central wavelength. Defined as the central wavelength between the two points defining FWMH 37 | 38 | 39 | Peak wavelength. Defined as sqrt{integ[x*filter(x) dx]/integ[filter(x) dx/x]} 40 | 41 | 42 | Peak wavelength. Defined as the lambda value with larger transmission 43 | 44 | 45 | Photon distribution based effective wavelength. Defined as integ[x^2*filter(x)*vega(x) dx]/integ[x*filter(x)*vega(x) dx] 46 | 47 | 48 | Full width at half maximum. Defined as the difference between the two wavelengths for which filter transmission is half maximum 49 | 50 | 51 | 52 | 53 | 54 | 55 | 56 | 57 | 58 | 59 | 60 | 61 | 62 | 63 | 64 | 65 | 66 | 67 | 68 | 69 | 70 | 71 | 72 | 73 | 74 | 75 | 76 | 77 | 78 | 79 | 80 | 81 | 82 | 83 | 84 | 85 | 86 | 87 | 88 | 89 | 90 | 91 | 92 | 93 | 94 | 95 | 96 | 97 | 98 | 99 | 100 | 101 | 102 | 103 | 104 | 105 | 106 | 107 | 108 | 109 | 110 | 111 | 112 | 113 | 114 | 115 | 116 | 117 | 118 | 119 | 120 | 121 | 122 | 123 | 124 | 125 | 126 | 127 | 128 | 129 | 130 | 131 | 132 | 133 | 134 | 135 | 136 | 137 | 138 | 139 | 140 | 141 | 142 | 143 | 144 | 145 | 146 | 147 | 148 | 149 | 150 | 151 | 152 | 153 | 154 | 155 | 156 | 157 | 158 | 159 | 160 | 161 | 162 | 163 | 164 | 165 | 166 | 167 | 168 | 169 | 170 | 171 | 172 | 173 | 174 | 175 | 176 | 177 | 178 | 179 | 180 | 181 | 182 | 183 | 184 | 185 | 186 | 187 | 188 | 189 | 190 | 191 | 192 | 193 | 194 | 195 | 196 | 197 | 198 | 199 | 200 | 201 | 202 | 203 | 204 | 205 | 206 | 207 | 208 | 209 | 210 | 211 | 212 | 213 | 214 | 215 | 216 | 217 | 218 | 219 | 220 | 221 | 222 | 223 | 224 | 225 | 226 | 227 | 228 | 229 | 230 | 231 | 232 | 233 | 234 | 235 | 236 | 237 | 238 | 239 | 240 | 241 | 242 | 243 | 244 | 245 | 246 | 247 | 248 | 249 |
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250 | 251 | 252 | -------------------------------------------------------------------------------- /svo_filters/data/filters/WFPC2.f656n: -------------------------------------------------------------------------------- 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | Instrument 13 | 14 | 15 | Observational facility 16 | 17 | 18 | 19 | 20 | Mean wavelength. Defined as integ[x*filter(x) dx]/integ[filter(x) dx] 21 | 22 | 23 | Effective wavelength. Defined as integ[x*filter(x)*vega(x) dx]/integ[filter(x)*vega(x) dx] 24 | 25 | 26 | Minimum filter wavelength. Defined as the first lambda value with a transmission at least 1% of maximum transmission 27 | 28 | 29 | Maximum filter wavelength. Defined as the last lambda value with a transmission at least 1% of maximum transmission 30 | 31 | 32 | Effective width. Defined as integ[x*filter(x) dx].\nEquivalent to the horizontal size of a rectangle with height equal to maximum transmission and with the same area that the one covered by the filter transmission curve. 33 | 34 | 35 | Central wavelength. Defined as the central wavelength between the two points defining FWMH 36 | 37 | 38 | Peak wavelength. Defined as sqrt{integ[x*filter(x) dx]/integ[filter(x) dx/x]} 39 | 40 | 41 | Peak wavelength. Defined as the lambda value with larger transmission 42 | 43 | 44 | Photon distribution based effective wavelength. Defined as integ[x^2*filter(x)*vega(x) dx]/integ[x*filter(x)*vega(x) dx] 45 | 46 | 47 | Full width at half maximum. Defined as the difference between the two wavelengths for which filter transmission is half maximum 48 | 49 | 50 | 51 | 52 | 53 | 54 | 55 | 56 | 57 | 58 | 59 | 60 | 61 | 62 | 63 | 64 | 65 | 66 | 67 | 68 | 69 | 70 | 71 | 72 | 73 | 74 | 75 | 76 | 77 | 78 | 79 | 80 | 81 | 82 | 83 | 84 | 85 | 86 | 87 | 88 | 89 | 90 | 91 | 92 | 93 | 94 | 95 | 96 | 97 | 98 | 99 | 100 | 101 | 102 | 103 | 104 | 105 | 106 | 107 | 108 | 109 | 110 | 111 | 112 | 113 | 114 | 115 | 116 | 117 | 118 | 119 | 120 | 121 | 122 | 123 | 124 | 125 | 126 | 127 | 128 | 129 | 130 | 131 | 132 | 133 | 134 | 135 | 136 | 137 | 138 | 139 | 140 | 141 | 142 | 143 | 144 | 145 | 146 | 147 | 148 | 149 | 150 | 151 | 152 | 153 | 154 | 155 | 156 | 157 | 158 | 159 | 160 | 161 | 162 | 163 | 164 |
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6552.0000000.590489
6554.0000000.704917
6556.0000000.749567
6558.0000000.767464
6560.0000000.777044
6562.0000000.778400
6564.0000000.770989
6566.0000000.755081
6568.0000000.734563
6570.0000000.718113
6572.0000000.713865
6574.0000000.709888
6576.0000000.647160
6578.0000000.439003
6580.0000000.199933
6582.0000000.076105
6584.0000000.029448
6586.0000000.012509
6588.0000000.005741
165 | 166 | 167 | -------------------------------------------------------------------------------- /svo_filters/data/plots/G141.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/svo_filters/data/plots/G141.png -------------------------------------------------------------------------------- /svo_filters/data/plots/H.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/svo_filters/data/plots/H.png -------------------------------------------------------------------------------- /svo_filters/data/plots/filtered.png: -------------------------------------------------------------------------------- https://raw.githubusercontent.com/hover2pi/svo_filters/ac7fe3a7c405627810ae4d35dc29c118d1b6def8/svo_filters/data/plots/filtered.png -------------------------------------------------------------------------------- /svo_filters/setup_package.py: -------------------------------------------------------------------------------- 1 | from distutils.extension import Extension 2 | 3 | def get_package_data(): 4 | return {'svo_filters': ['data/*', 'data/filters/*', 'data/plots/*', 'data/spectra/*']} 5 | -------------------------------------------------------------------------------- /svo_filters/test_svo.py: -------------------------------------------------------------------------------- 1 | """Some tests to make sure the filters work as intended""" 2 | import unittest 3 | 4 | import astropy.units as q 5 | import astropy.table as at 6 | import numpy as np 7 | from bokeh.plotting import figure 8 | 9 | from svo_filters import svo 10 | 11 | 12 | class TestFilter(unittest.TestCase): 13 | """Tests for Filter class""" 14 | def setUp(self): 15 | pass 16 | 17 | def test_info(self): 18 | """Test that the info attr works""" 19 | filt = svo.Filter('2MASS.J') 20 | self.assertTrue(filt.info() == None) 21 | self.assertTrue(isinstance(filt.info(fetch=True), at.Table)) 22 | self.assertRaises(ValueError, setattr, filt, 'wave', np.arange(10)) 23 | self.assertRaises(ValueError, setattr, filt, 'throughput', np.arange(1)) 24 | 25 | def test_no_filter(self): 26 | """Test if exception is raised for bogus filter""" 27 | self.assertRaises(IndexError, svo.Filter, 'BAD_FILTER') 28 | 29 | def test_filter_web(self): 30 | """Test if Filter object is created from web query""" 31 | filt = svo.Filter('Generic/Johnson.B') 32 | 33 | self.assertTrue(isinstance(filt, svo.Filter)) 34 | 35 | def test_filter_xml(self): 36 | """Test if Filter object is created properly""" 37 | filt = svo.Filter('2MASS.J') 38 | 39 | self.assertTrue(isinstance(filt, svo.Filter)) 40 | 41 | def test_filter_txt(self): 42 | """Test if Filter object is created properly""" 43 | filt = svo.Filter('NIRISS.GR700XD.1') 44 | 45 | self.assertTrue(isinstance(filt, svo.Filter)) 46 | 47 | def test_filter_tophat(self): 48 | """Test if Filter object is created properly""" 49 | # Good tophat 50 | filt = svo.Filter('tophat', wave_min=0.8*q.um, wave_max=1.2*q.um) 51 | self.assertTrue(isinstance(filt, svo.Filter)) 52 | 53 | # Bad tophat 54 | self.assertRaises(ValueError, svo.Filter, 'tophat') 55 | 56 | def test_filter_bin(self): 57 | """Test that the binning works""" 58 | # Test n_bins 59 | filt = svo.Filter('WFC3_IR.G141', n_bins=10) 60 | self.assertTrue(filt.wave.shape[0] == 10) 61 | 62 | # Test pixels_per_bin 63 | filt = svo.Filter('WFC3_IR.G141', pixels_per_bin=50) 64 | self.assertTrue(filt.wave.shape[1] == 50) 65 | 66 | # Test neither throws an error 67 | self.assertRaises(ValueError, svo.Filter, 'WFC3_IR.G141', n_bins=None, 68 | pixels_per_bin=None) 69 | 70 | def test_filter_units_bad(self): 71 | """Test that changing the wave units to non-length raises exception""" 72 | filt = svo.Filter('WFC3_IR.G141') 73 | 74 | # Fun syntax to test attribute setting 75 | self.assertRaises(ValueError, setattr, filt, 'wave_units', q.second) 76 | self.assertRaises(ValueError, setattr, filt, 'flux_units', q.second) 77 | 78 | def test_spectrum(self): 79 | """Test that the filter gets applied to a spectrum properly""" 80 | filt = svo.Filter('2MASS.J') 81 | spec = [np.linspace(0.9, 2, 1000)*q.um, 82 | np.ones(1000)*q.erg/q.s/q.cm**2/q.AA] 83 | 84 | # Apply the filter to the spectrum 85 | filtered, err_filtered = filt.apply(spec) 86 | self.assertEqual(filtered.shape, filt.wave.squeeze().shape) 87 | 88 | # Check that the propagated errors are all nans since none were given 89 | self.assertTrue(np.all([np.isnan(i) for i in err_filtered])) 90 | 91 | # Check overlap 92 | self.assertEqual(svo.Filter('2MASS.J').overlap(spec), 'full') 93 | self.assertEqual(svo.Filter('2MASS.Ks').overlap(spec), 'partial') 94 | self.assertEqual(svo.Filter('WISE.W4').overlap(spec), 'none') 95 | 96 | def test_filter_apply_binned(self): 97 | """Test that the filter gets applied to a spectrum properly""" 98 | filt = svo.Filter('2MASS.J', n_bins=4) 99 | spec = [np.linspace(0.9, 2, 1000)*q.um, 100 | np.ones(1000)*q.erg/q.s/q.cm**2/q.AA] 101 | 102 | # Apply the filter to the spectrum 103 | filtered, err_filtered = filt.apply(spec, plot=True) 104 | self.assertEqual(filtered.shape, filt.wave.squeeze().shape) 105 | 106 | def test_filter_apply_binned_err(self): 107 | """Test that the filter gets applied to a spectrum with errors properly""" 108 | filt = svo.Filter('2MASS.J', n_bins=4) 109 | funit = q.erg/q.s/q.cm**2/q.AA 110 | spec = [np.linspace(0.9, 2, 1000)*q.um, 111 | np.ones(1000)*funit, 112 | np.ones(1000)*0.05*funit] 113 | 114 | # Apply the filter to the spectrum 115 | filtered, err_filtered = filt.apply(spec) 116 | 117 | # Check that the units are still there 118 | self.assertEqual(filtered.unit,funit) 119 | self.assertEqual(err_filtered.shape, filt.wave.squeeze().shape) 120 | 121 | def test_filter_apply_no_units(self): 122 | """Test that the apply method works with and without units""" 123 | filt = svo.Filter('2MASS.J') 124 | spec = [np.linspace(0.9, 2, 1000), 125 | np.ones(1000)] 126 | 127 | # Apply the filter to the spectrum 128 | filtered, err_filtered = filt.apply(spec) 129 | self.assertFalse(hasattr(filtered, 'unit')) 130 | self.assertTrue(np.all([np.isnan(i) for i in err_filtered])) 131 | 132 | def test_plot(self): 133 | """Test that the plots are produced properly""" 134 | filt = svo.Filter('2MASS.J') 135 | filt.plot(details=True) 136 | plt = filt.plot(draw=False) 137 | 138 | self.assertTrue(type(plt) == figure) 139 | 140 | def test_filter_monotonic(self): 141 | """Test that non-monotonic filters are treated correctly""" 142 | filt = svo.Filter('Palomar/ZTF.g') 143 | self.assertFalse(np.any(np.diff(filt.wave)<=0)) 144 | 145 | 146 | class TestFilterList(unittest.TestCase): 147 | """Tests for filter function""" 148 | def setUp(self): 149 | pass 150 | 151 | def test_default(self): 152 | """Test default directory""" 153 | filts = svo.filters() 154 | self.assertTrue(len(filts) > 0) 155 | -------------------------------------------------------------------------------- /svo_filters/utils.py: -------------------------------------------------------------------------------- 1 | import astropy.units as q 2 | import numpy as np 3 | 4 | 5 | def _padded_differences(arr, pad_val=1e20): 6 | """ 7 | 8 | Parameters 9 | ---------- 10 | arr: array-like 11 | pad_val: astropy.units.quantity, float, int 12 | value for padding the first element of the difference array by when calculating 13 | monotonically increasing (or not) differences. 14 | """ 15 | if isinstance(arr, q.Quantity): 16 | # Quantity units cannot be padded by non-quantity unless using this wrapper. 17 | diff = arr.ediff1d(to_begin=pad_val) 18 | else: 19 | diff = np.ediff1d(arr, to_begin=pad_val) 20 | return diff 21 | 22 | def incremented_monotonic(arr, increment=None, increment_step=1000): 23 | """Returns input if monotonically increasing. Otherwise 24 | increment repeated elements by `increment`, which will be set to 1/`increment_step` 25 | of the smallest difference in array if `None`, the default. 26 | If not monotonically increasing (ignoring repeated elements), raises `ValueError`. 27 | 28 | Parameters 29 | ---------- 30 | arr: array-like 31 | array to check for increment. Also handles astropy.units.quantity.Quantity arrays. 32 | increment: astropy.units.quantity, float, int (optional) 33 | value to increment repeated elements by. Set to 1/`increment_step` of the smallest difference 34 | in array if `None`, the default. Unit conversion will be attempted if array is an instance 35 | of astropy.units.quantity.Quantity. 36 | increment_step: float, int 37 | The relative size difference between repeated elements if automatically determining. Only 38 | used if `increment = None`. 39 | 40 | Returns 41 | ------- 42 | array-like 43 | Input array if monotonically increasing else input array where repeat values 44 | have been incremented by `increment`. 45 | """ 46 | diff = _padded_differences(arr) 47 | 48 | if np.any(diff<0): 49 | raise ValueError("Input array must be monotonically increasing except for repeated values.") 50 | non_monotonic_mask = diff<=0 51 | 52 | # Exit early if monotonic 53 | if np.all(~non_monotonic_mask): 54 | return arr 55 | 56 | if increment is None: 57 | # a thousanth of the minimimum non-zero increment. 58 | increment = np.nanmin(diff[~non_monotonic_mask])/increment_step 59 | # Try to help user with unit conversion, will fail if unconvertable. 60 | elif isinstance(arr, q.Quanity): 61 | increment = increment << arr.unit 62 | 63 | #non_monotonic_mask = non_monotonic_mask.reshape(arr.shape) 64 | repeats, multiples = get_multipliers(non_monotonic_mask) 65 | if isinstance(increment, q.Quantity): 66 | multiples = multiples << q.dimensionless_unscaled 67 | multiples *= increment 68 | 69 | flatarr = arr.flatten() 70 | flatarr[repeats] += multiples 71 | return flatarr.reshape(arr.shape) 72 | 73 | 74 | def breadth_first(repeats, state, row): 75 | """somewhat convoluted 1D breadth first search 76 | for getting multiples of repeated elements. 77 | """ 78 | queue = [repeats[row]] 79 | index = 1 80 | additions = [index] 81 | state.append(row) 82 | while len(queue) > 0: 83 | idx = queue.pop(0) 84 | 85 | #print(idx, idx+1, repeats) 86 | if idx+1 in repeats: 87 | neighbor = idx+1 88 | state.append(row+index) 89 | index += 1 90 | queue.append(neighbor) 91 | additions.append(index) 92 | 93 | return additions, state 94 | 95 | 96 | def get_multipliers(mask): 97 | """Get all repeats and their multiples using breadth first search 98 | 99 | Parameters 100 | ---------- 101 | mask: array_like 102 | array of booleans representing repeated elements. True for repeated. 103 | 104 | Returns 105 | ------- 106 | tuple 107 | tuple of array_like of repeated indexes and their multiples for use in 108 | shifting multiple repeated indexes. 109 | """ 110 | repeats = np.nonzero(mask.flatten())[0] 111 | if len(repeats)==0: 112 | raise ValueError("No repeats found. Input mask all False") 113 | groups = [] 114 | state = [] 115 | for j,val in enumerate(repeats): 116 | if j in state: 117 | continue 118 | additions, state = breadth_first(repeats, state, j) 119 | groups.append(additions) 120 | groups = np.array([element for sublist in groups for element in sublist]) 121 | 122 | return repeats, groups 123 | --------------------------------------------------------------------------------