diff --git a/.github/workflows/bump_on_dependency.yml b/.github/workflows/bump_on_dependency.yml new file mode 100644 index 00000000..fa3bf51b --- /dev/null +++ b/.github/workflows/bump_on_dependency.yml @@ -0,0 +1,21 @@ +name: Bump dev version on dependency PR +on: + pull_request: + types: [closed] + +jobs: + Bump: + name: Bump prerelease version + if: > + github.event.pull_request.merged == true && + github.event.pull_request.base.ref == 'main' && + contains( + github.event.pull_request.labels.*.name, + 'dependencies' + ) + uses: AstarVienna/DevOps/.github/workflows/bump.yml@main + secrets: inherit + with: + rule: prerelease + branch: main + diff --git a/.readthedocs.yaml b/.readthedocs.yaml index 9f344622..389c1d7a 100644 --- a/.readthedocs.yaml +++ b/.readthedocs.yaml @@ -5,7 +5,7 @@ version: 2 build: - os: "ubuntu-22.04" + os: "ubuntu-24.04" tools: python: "3.11" jobs: diff --git a/CHANGELOG.md b/CHANGELOG.md index b2452855..013c8fa8 100644 --- a/CHANGELOG.md +++ b/CHANGELOG.md @@ -1,3 +1,72 @@ +# Version 0.11.4 +**2026-05-20** + +Quick patch to make TipTop PSFs work with ScopeSim effects. + +## What's Changed +### New Features or Improvements +* Squeeze extra dimensions out of PSF kernel by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/908 +### Dependency Changes +* Bump nbconvert from 7.17.0 to 7.17.1 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/906 +* Bump lxml from 6.0.2 to 6.1.0 by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/907 +* Bump pytest and pytest-cov by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/909 +* Bump jupyterlab and notebook by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/914 +* Bump jupyter-server from 2.11.2 to 2.18.0 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/921 +* Bump mistune from 3.0.2 to 3.2.1 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/923 +* Bump urllib3 from 2.6.3 to 2.7.0 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/926 +### Other Changes +* Update hashes for PPS_CFO2 psfs by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/925 + +**Full Changelog**: https://github.com/AstarVienna/ScopeSim/compare/v0.11.3...v0.11.4 + + +# Version 0.11.3 +**2026-04-16** + +Some new effects and a lot of bugfixing. + +## What's Changed +### API Changes +* Plot system transmission components by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/894 +### Bugs fixed +* Read fp_mask_{}.dat explicitely as float by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/869 +* Extend Blackbody wavelength range to cover all filters by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/872 +* Pixel area must be positive by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/878 +* Use NumPy 2.3.5 for Python 3.13+ by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/882 +* Fixes off-by-a-half in FOVs by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/880 +* Fix PupilTransmission emission after update by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/900 +### Changes to or addition of Effects +* Add `PixelResponseNonUniformity` effect for fixed per-pixel gain variation (PRNU) by @ShannonS00 in https://github.com/AstarVienna/ScopeSim/pull/886 +* Add offset to spectral transformations to enable shifted slits by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/875 +* Minor PSF refactor and more logs by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/901 +* Fibre transmission for WCU lasers by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/904 +* Add a large scale illumination effect by @ShannonS00 in https://github.com/AstarVienna/ScopeSim/pull/898 +### Dependency Changes +* Bump synphot, allow packaging 26 by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/870 +* Bump numpydoc from 1.9.0 to 1.10.0 in the dev-dependencies group by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/873 +* Bump ipykernel from 6.31.0 to 7.1.0 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/874 +* Bump nbconvert from 7.16.4 to 7.17.0 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/876 +* Bump pillow from 12.1.0 to 12.1.1 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/877 +* Bump astar-utils from 0.5.0 to 0.5.1 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/881 +* Bump jupytext from 1.18.1 to 1.19.0 in the dev-dependencies group by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/884 +* Bump tqdm from 4.67.1 to 4.67.3 in the main-dependencies group by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/883 +* Bump tornado from 6.5 to 6.5.5 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/888 +* Bump requests from 2.32.4 to 2.33.0 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/891 +* Bump pygments from 2.17.2 to 2.20.0 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/892 +* Bump astar-utils from 0.5.1 to 0.5.2 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/890 +* Bump the dev-dependencies group with 3 updates by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/896 +* Bump pooch from 1.8.2 to 1.9.0 by @dependabot[bot] in https://github.com/AstarVienna/ScopeSim/pull/897 +* Bump pillow from 12.1.1 to 12.2.0 by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/903 +### Documentation Improvements +* Document system transmission plot in getting_started by @oczoske in https://github.com/AstarVienna/ScopeSim/pull/895 +* Docstring and typing fixes in preparation for release by @teutoburg in https://github.com/AstarVienna/ScopeSim/pull/902 + +## New Contributors +* @ShannonS00 made their first contribution in https://github.com/AstarVienna/ScopeSim/pull/886 + +**Full Changelog**: https://github.com/AstarVienna/ScopeSim/compare/v0.11.2...v0.11.3 + + # Version 0.11.2 **2026-01-20** diff --git a/docs/source/5_liners/scopsim_templates_intro.ipynb b/docs/source/5_liners/scopesim_templates_intro.ipynb similarity index 100% rename from docs/source/5_liners/scopsim_templates_intro.ipynb rename to docs/source/5_liners/scopesim_templates_intro.ipynb diff --git a/docs/source/getting_started.ipynb b/docs/source/getting_started.ipynb index 5e18b6b5..48a92397 100644 --- a/docs/source/getting_started.ipynb +++ b/docs/source/getting_started.ipynb @@ -316,6 +316,26 @@ "simulation.settings[\"!ATMO\"]" ] }, + { + "cell_type": "markdown", + "id": "15efee46-576f-4aee-9dd9-3ab2fe68ba14", + "metadata": {}, + "source": [ + "### Inspecting the system transmission\n", + "\n", + "The total system transmission and the contribution from the individual elements in the optical train can be visualised as follows:" + ] + }, + { + "cell_type": "code", + "execution_count": null, + "id": "80c0c1cd-cc6c-4015-9c7c-ed0bc5479c98", + "metadata": {}, + "outputs": [], + "source": [ + "simulation.optical_train.optics_manager.system_transmission(plot=True);" + ] + }, { "cell_type": "markdown", "id": "labeled-railway", @@ -354,7 +374,7 @@ "name": "python", "nbconvert_exporter": "python", "pygments_lexer": "ipython3", - "version": "3.12.7" + "version": "3.12.9" } }, "nbformat": 4, diff --git a/docs/source/index.rst b/docs/source/index.rst index 60250db7..c431552a 100644 --- a/docs/source/index.rst +++ b/docs/source/index.rst @@ -14,15 +14,40 @@ ScopeSim_ is on pip:: pip install scopesim_templates -.. warning:: July 2022: The downloadable content server was retired and the data migrated to a new server. +.. _ScopeSim: https://scopesim.readthedocs.io/en/latest/ +.. _`ScopeSim Templates`: https://scopesim-templates.readthedocs.io/en/latest/ - ScopeSim v0.5.1 and above have been redirected to a new server URL. +.. |metis_logo| image:: https://irdb.readthedocs.io/en/latest/_images/metis_scopesim_logo.png + :height: 100px + :target: https://irdb.readthedocs.io/en/latest/METIS/docs/README.html + +.. |micado_logo| image:: https://irdb.readthedocs.io/en/latest/_images/micado_scopesim_logo.png + :height: 100px + :target: https://irdb.readthedocs.io/en/latest/MICADO/docs/README.html + +.. |mosaic_logo| image:: https://irdb.readthedocs.io/en/latest/_images/mosaic_scopesim_logo.png + :height: 100px + :target: https://irdb.readthedocs.io/en/latest/MOSAIC/docs/README.html + +.. |youtube_icon| image:: https://upload.wikimedia.org/wikipedia/commons/thumb/0/09/YouTube_full-color_icon_%282017%29.svg/960px-YouTube_full-color_icon_%282017%29.svg.png + :height: 30px + :target: https://www.youtube.com/@ScopeSimTutorials + + +.. note:: Looking for ELT specific user documentation? + + See the MICADO, METIS, and MOSAIC user guides on the `IRDB documentation page `_ + + |micado_logo| |metis_logo| |mosaic_logo| + +.. note:: ScopeSim Tutorials on Youtube + + A series of introductory tutorials are now available on youtube + + |youtube_icon| @ScopeSimTutorials - For older verions, please either upgrade to the latest version (``pip install --upgrade scopesim``), or follow these `instructions to update the server URL `_ in the config file. -.. _ScopeSim: https://scopesim.readthedocs.io/en/latest/ -.. _`ScopeSim Templates`: https://scopesim-templates.readthedocs.io/en/latest/ .. toctree:: :maxdepth: 2 @@ -33,6 +58,12 @@ ScopeSim_ is on pip:: 5_liners/index faqs/index +.. warning:: July 2022: The downloadable content server was retired and the data migrated to a new server. + + ScopeSim v0.5.1 and above have been redirected to a new server URL. + + For older verions, please either upgrade to the latest version (``pip install --upgrade scopesim``), or follow these `instructions to update the server URL `_ in the config file. + The ScopeSim python ecosystem ----------------------------- @@ -58,7 +89,7 @@ There are several packages in the ScopeSim_ ecosystem to be aware of: .. _ScopeSim: https://scopesim.readthedocs.io/en/latest/ .. _`ScopeSim Templates`: https://scopesim-templates.readthedocs.io/en/latest/ -.. _IRDB: https://github.com/astronomyk/irdb +.. _IRDB: https://irdb.readthedocs.io/en/latest/ .. _AnisoCADO: https://anisocado.readthedocs.io/en/latest/ .. _skycalc_ipy: https://skycalc-ipy.readthedocs.io/en/latest/ .. _SpeXtra: https://spextra.readthedocs.io/en/latest/ diff --git a/poetry.lock b/poetry.lock index ec146a19..05022a92 100644 --- a/poetry.lock +++ b/poetry.lock @@ -1,4 +1,4 @@ -# This file is automatically @generated by Poetry 2.3.0 and should not be changed by hand. +# This file is automatically @generated by Poetry 2.4.1 and should not be changed by hand. [[package]] name = "accessible-pygments" @@ -167,14 +167,14 @@ test = ["dateparser (==1.*)", "pre-commit", "pytest", "pytest-cov", "pytest-mock [[package]] name = "astar-utils" -version = "0.5.0" +version = "0.5.3" description = "Contains commonly-used utilities for AstarVienna's projects." optional = false python-versions = "<3.15,>=3.10" groups = ["main"] files = [ - {file = "astar_utils-0.5.0-py3-none-any.whl", hash = "sha256:d3262076319423e65782a2635673a2380c1edbfd24ff4eb51c7498674f05ec5e"}, - {file = "astar_utils-0.5.0.tar.gz", hash = "sha256:0d0759138f829b8720a62ff2065148d9a9e4e8405f7ef81aa4a0be51e92d251e"}, + {file = "astar_utils-0.5.3-py3-none-any.whl", hash = "sha256:2b595b3c5acc20888e6beb8cffcbb5999d17311a358ba97c75d331883a6e0e8e"}, + {file = "astar_utils-0.5.3.tar.gz", hash = "sha256:57423f4c5eeece04b7d92ca6d1f8923f1a25ccfa972f6ddb8194dbcd9197533b"}, ] [package.dependencies] @@ -238,14 +238,14 @@ typing = ["typing_extensions (>=4.0.0)"] [[package]] name = "astropy-iers-data" 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safelist-based HTML-sanitizing tool." optional = false -python-versions = ">=3.8" +python-versions = ">=3.10" groups = ["dev", "docs"] files = [ - {file = "bleach-6.1.0-py3-none-any.whl", hash = "sha256:3225f354cfc436b9789c66c4ee030194bee0568fbf9cbdad3bc8b5c26c5f12b6"}, - {file = "bleach-6.1.0.tar.gz", hash = "sha256:0a31f1837963c41d46bbf1331b8778e1308ea0791db03cc4e7357b97cf42a8fe"}, + {file = "bleach-6.4.0-py3-none-any.whl", hash = "sha256:4b6b6a54fff2e69a3dde9d21cc6301220bee3c3cb792187d11403fd795031081"}, + {file = "bleach-6.4.0.tar.gz", hash = "sha256:4202482733d85cedd04e59fcb2f89f4e4c7c385a78d3c3c23c30446843a37452"}, ] [package.dependencies] -six = ">=1.9.0" +tinycss2 = {version = ">=1.1.0", optional = true, markers = "extra == \"css\""} webencodings = "*" [package.extras] -css = ["tinycss2 (>=1.1.0,<1.3)"] +css = ["tinycss2 (>=1.1.0)"] [[package]] name = "certifi" -version = "2025.6.15" +version = "2026.4.22" description = "Python package for providing Mozilla's CA Bundle." optional = false python-versions = ">=3.7" groups = ["main", "dev", "docs"] files = [ - {file = "certifi-2025.6.15-py3-none-any.whl", hash = "sha256:2e0c7ce7cb5d8f8634ca55d2ba7e6ec2689a2fd6537d8dec1296a477a4910057"}, - {file = "certifi-2025.6.15.tar.gz", hash = "sha256:d747aa5a8b9bbbb1bb8c22bb13e22bd1f18e9796defa16bab421f7f7a317323b"}, + {file = "certifi-2026.4.22-py3-none-any.whl", hash = "sha256:3cb2210c8f88ba2318d29b0388d1023c8492ff72ecdde4ebdaddbb13a31b1c4a"}, + {file = "certifi-2026.4.22.tar.gz", hash = "sha256:8d455352a37b71bf76a79caa83a3d6c25afee4a385d632127b6afb3963f1c580"}, ] [[package]] @@ -1141,6 +1141,28 @@ http2 = ["h2 (>=3,<5)"] socks = ["socksio (==1.*)"] trio = ["trio (>=0.22.0,<1.0)"] +[[package]] +name = "httpcorexyz" +version = "1.1.1" +description = "A minimal low-level HTTP client." +optional = false +python-versions = ">=3.9" +groups = ["main"] +files = [ + {file = "httpcorexyz-1.1.1-py3-none-any.whl", hash = "sha256:58becd21f127c0a846813d0705f9e0c27c16c867bb436813667f569d4f0ba94e"}, + {file = "httpcorexyz-1.1.1.tar.gz", hash = "sha256:0b8dbbe8ffaccd20b7c755d92129f9fb04a23f2ef22b32ff82e2d1c7fcfee803"}, +] + +[package.dependencies] +certifi = ">=2026.2.25" +h11 = ">=0.16" + +[package.extras] +asyncio = ["anyio (>=4.5.0,<5.0)"] +http2 = ["h2 (>=3,<5)"] +socks = ["socksio (==1.*)"] +trio = ["trio (>=0.22.0,<1.0)"] + [[package]] name = "httpx" version = "0.28.1" @@ -1166,20 +1188,45 @@ http2 = ["h2 (>=3,<5)"] socks = ["socksio (==1.*)"] zstd = ["zstandard (>=0.18.0)"] +[[package]] +name = "httpxyz" +version = "0.31.2" +description = "Friendly fork of the next generation HTTP client." +optional = false +python-versions = ">=3.9" +groups = ["main"] +files = [ + {file = "httpxyz-0.31.2-py3-none-any.whl", hash = "sha256:1e8058b7324aaf875efb6b4cf5a5a423f4ac101fd4af515349fb4e1d3e4d4441"}, + {file = "httpxyz-0.31.2.tar.gz", hash = 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"2.7.0" description = "HTTP library with thread-safe connection pooling, file post, and more." optional = false -python-versions = ">=3.9" +python-versions = ">=3.10" groups = ["main", "dev", "docs"] files = [ - {file = "urllib3-2.6.3-py3-none-any.whl", hash = "sha256:bf272323e553dfb2e87d9bfd225ca7b0f467b919d7bbd355436d3fd37cb0acd4"}, - {file = "urllib3-2.6.3.tar.gz", hash = "sha256:1b62b6884944a57dbe321509ab94fd4d3b307075e0c2eae991ac71ee15ad38ed"}, + {file = "urllib3-2.7.0-py3-none-any.whl", hash = "sha256:9fb4c81ebbb1ce9531cce37674bbc6f1360472bc18ca9a553ede278ef7276897"}, + {file = "urllib3-2.7.0.tar.gz", hash = "sha256:231e0ec3b63ceb14667c67be60f2f2c40a518cb38b03af60abc813da26505f4c"}, ] [package.extras] @@ -4495,4 +4652,4 @@ type = ["pytest-mypy"] [metadata] lock-version = "2.1" python-versions = ">=3.10,<3.15" -content-hash = "cd1380850b44ed39baa36bc970ef510e9e28d466926efb923cd6f240af616249" +content-hash = "9d466fdf8137d22f15be3a77237a6a8bd2d3f344d34a7c95f18d02f3d56f0192" diff --git a/pyproject.toml b/pyproject.toml index 9ad4c503..cb4ecb88 100644 --- a/pyproject.toml +++ b/pyproject.toml @@ -1,6 +1,6 @@ [project] name = "ScopeSim" -version = "0.11.3a0" +version = "0.11.5a3" description = "Generalised telescope observation simulator" license = {text = "GPL-3.0-or-later"} authors = [ @@ -17,9 +17,7 @@ dynamic = [ "classifiers" ] requires-python = ">=3.10,<3.15" dependencies = [ "numpy (>=1.26.4,<2.3.0) ; python_version >= '3.10' and python_version < '3.13'", - "numpy (>=2.2.6,<3.0.0) ; python_version >= '3.13'", - # SciPy is only an indirect dependency through synphot, but has limited - # wheels for Python versions, so needs to be specified explicitly. + "numpy (>=2.3.5,<3.0.0) ; python_version >= '3.13'", "scipy (>=1.15.3,<1.16.0) ; python_version >= '3.10' and python_version < '3.11'", "scipy (>=1.17.0,<1.18.0) ; python_version >= '3.11'", @@ -28,18 +26,18 @@ dependencies = [ "pooch (>=1.8.2,<2.0.0)", "docutils (>=0.19,<1.0)", - "httpx (>=0.28.1,<1.0)", + "httpxyz (>=0.31.2,<1.0)", "beautifulsoup4 (>=4.13.3,<5.0.0)", "lxml (>=6.0.2,<7.0.0)", "pyyaml (>=6.0.3,<7.0.0)", "more-itertools (>=10.2.0,<11.0.0)", "tqdm (>=4.66.6,<5.0.0)", - "packaging (>=25.0,<26.0)", + "packaging (>=25.0,<27.0)", - "synphot (>=1.5.0,<2.0.0)", + "synphot (>=1.6.1,<2.0.0)", "skycalc-ipy (>=0.7.0,<1.0)", "anisocado (>=0.5.0,<1.0)", - "astar-utils (>=0.5.0,<1.0)" + "astar-utils (>=0.5.3,<1.0)" ] [project.urls] @@ -61,14 +59,14 @@ optional = true [tool.poetry.group.dev.dependencies] jupyter = "^1.1.1" -jupytext = "^1.18.1" -ipykernel = "^6.31.0" -ipympl = "^0.9.8" +jupytext = "^1.19.3" +ipykernel = "^7.3.0" +ipympl = "^0.10.0" [tool.poetry.group.test.dependencies] -pytest = "^9.0.2" -pytest-cov = "^7.0.0" -ipykernel = "^6.31.0" +pytest = "^9.0.3" +pytest-cov = "^7.1.0" +ipykernel = "^7.3.0" [tool.poetry.group.docs] optional = true @@ -78,13 +76,13 @@ sphinx = "^8.1.3" sphinx-book-theme = "^1.1.4" jupyter-sphinx = ">=0.5.3" sphinx-copybutton = ">=0.5.2,<1.0" -myst-nb = "^1.3.0" +myst-nb = "^1.4.0" sphinxcontrib-apidoc = ">=0.6.0,<1.0" sphinxcontrib-mermaid = "^2.0" nbsphinx = "^0.9.8" -numpydoc = "^1.9.0" -ipykernel = "^6.31.0" -ipympl = "^0.9.8" +numpydoc = "^1.10.0" +ipykernel = "^7.3.0" +ipympl = "^0.10.0" [build-system] diff --git a/scopesim/__init__.py b/scopesim/__init__.py index c58d6009..17a33030 100644 --- a/scopesim/__init__.py +++ b/scopesim/__init__.py @@ -21,6 +21,8 @@ import yaml from astropy.utils.exceptions import AstropyWarning +from .utils import ScopesimPendingDeprecationWarning + warnings.simplefilter('ignore', UserWarning) warnings.simplefilter('ignore', RuntimeWarning) # warnings for the developer @@ -28,7 +30,7 @@ if __version__.is_prerelease or __version__.is_devrelease: # Those are usually ignored, but in development we should see them. warnings.simplefilter("default", DeprecationWarning) - warnings.simplefilter("default", PendingDeprecationWarning) + warnings.simplefilter("default", ScopesimPendingDeprecationWarning) except AttributeError: # catch __version__ = "undetermined" pass diff --git a/scopesim/commands/user_commands.py b/scopesim/commands/user_commands.py index 50455b83..4a51d684 100644 --- a/scopesim/commands/user_commands.py +++ b/scopesim/commands/user_commands.py @@ -8,7 +8,7 @@ from typing import Any import yaml -import httpx +import httpxyz as httpx from packaging.version import parse from astar_utils import NestedMapping, RecursiveNestedMapping, NestedChainMap @@ -163,6 +163,11 @@ def __init__(self, *maps, **kwargs): # Don't add another layer when .new_child() is called. maps = [RecursiveNestedMapping(title="CurrSys"), *maps] + # Guard against wrong args to avoid cryptical error downstream. + if not all(isinstance(m, Mapping) for m in maps): + raise TypeError( + "Non-keyword args to UserCommands must be dict-like.") + super().__init__(*maps) self.yaml_dicts = [] diff --git a/scopesim/effects/__init__.py b/scopesim/effects/__init__.py index 14ab0fc7..da03ffc0 100644 --- a/scopesim/effects/__init__.py +++ b/scopesim/effects/__init__.py @@ -24,4 +24,5 @@ from .metis_wcu import * from .metis_ifu_simple import * +from .illumination import * # from . import effects_utils diff --git a/scopesim/effects/electronic/__init__.py b/scopesim/effects/electronic/__init__.py index 9ae7c4ff..5d10e0d4 100644 --- a/scopesim/effects/electronic/__init__.py +++ b/scopesim/effects/electronic/__init__.py @@ -9,6 +9,7 @@ - PoorMansHxRGReadoutNoise - simple readout noise for HAWAII detectors - BasicReadoutNoise - readout noise - ShotNoise - realisation of Poissonian photon noise +- PixelResponseNonUniformity - per-pixel gain variation (PRNU) - DarkCurrent - add dark current - LinearityCurve - apply detector (non-)linearity and saturation - ReferencePixelBorder @@ -23,7 +24,7 @@ from .electrons import LinearityCurve, ADConversion, InterPixelCapacitance from .noise import (Bias, PoorMansHxRGReadoutNoise, BasicReadoutNoise, - ShotNoise, DarkCurrent) + ShotNoise, DarkCurrent, PixelResponseNonUniformity) from .exposure import AutoExposure, ExposureIntegration, ExposureOutput from .pixels import ReferencePixelBorder, BinnedImage, UnequalBinnedImage from .dmps import DetectorModePropertiesSetter diff --git a/scopesim/effects/electronic/electrons.py b/scopesim/effects/electronic/electrons.py index 50670c51..c860362b 100644 --- a/scopesim/effects/electronic/electrons.py +++ b/scopesim/effects/electronic/electrons.py @@ -307,12 +307,13 @@ def apply_to(self, obj, **kwargs): # Apply the gain value (copy from DarkCurrent) # Note that this does not cater for the case where the gain is given # as a plain dictionary. Should we implement that? - logger.info(f"Applying gain {from_currsys(self.cmds['!DET.gain'])}") if hasattr(self.cmds["!DET.gain"], "dic"): dtcr_id = obj.meta[real_colname("id", obj.meta)] gain = self.cmds["!DET.gain"].dic[dtcr_id] + logger.info(f"Detector {dtcr_id}: applying gain {gain}") elif isinstance(self.cmds["!DET.gain"], (float, int)): gain = self.cmds["!DET.gain"] + logger.info(f"Applying gain {gain}") else: raise ValueError(".meta['gain'] must be either " f"dict or float, but is {self.cmds['!DET.gain']}") @@ -341,7 +342,7 @@ def apply_to(self, obj, **kwargs): # This used to create a new ImageHDU with the same header but the data # set to the modified data. It should be fine to simply re-assign the # data attribute, but just in case it's not... - logger.info("Applying digitization to dtype %s.", new_dtype) + logger.debug("Applying digitization to dtype %s.", new_dtype) obj._hdu.data = obj._hdu.data.astype(new_dtype) return obj diff --git a/scopesim/effects/electronic/exposure.py b/scopesim/effects/electronic/exposure.py index aeadbb6e..8ff88e1e 100644 --- a/scopesim/effects/electronic/exposure.py +++ b/scopesim/effects/electronic/exposure.py @@ -26,6 +26,9 @@ class AutoExposure(Effect): The effects sets the parameters `!OBS.dit` and `!OBS.ndit`. + The effect is the first detector effect, hence essentially operates on the + `ImagePlane`, mapped to the detector array. + Examples -------- The parameters `!OBS.exptime`, `!DET.full_well` and `!DET.mindit` should @@ -45,10 +48,6 @@ class AutoExposure(Effect): z_order: ClassVar[tuple[int, ...]] = (902,) def __init__(self, **kwargs): - """ - The effect is the first detector effect, hence essentially operates - on the `ImagePlane`, mapped to the detector array. - """ super().__init__(**kwargs) self.meta.update(kwargs) if self.cmds is None: @@ -223,7 +222,7 @@ def apply_to(self, obj, **kwargs): return obj def set_mode(self, new_mode): - """Set new mode for ExposureOutput (average or sum)""" + """Set new mode for ExposureOutput (average or sum).""" if new_mode in self.modes: self.current_mode = new_mode self.meta["current_mode"] = self.current_mode @@ -234,7 +233,6 @@ def set_mode(self, new_mode): class ExposureIntegration(Effect): """Integrate the expected flux over ``exptime``. - This effect multiplies the expected photon flux from the ``ImagePlane`` by the total exposure time, computed as the product of ``dit`` and ``ndit``. diff --git a/scopesim/effects/electronic/noise.py b/scopesim/effects/electronic/noise.py index d2ce522a..0698c09f 100644 --- a/scopesim/effects/electronic/noise.py +++ b/scopesim/effects/electronic/noise.py @@ -2,6 +2,7 @@ """Any kinds of electronic or photonic noise.""" from typing import ClassVar +from numbers import Real import numpy as np from astropy.io import fits @@ -83,11 +84,13 @@ def apply_to(self, det, **kwargs): return det def plot(self, det, **kwargs): + """Plot effect image.""" dtcr = self.apply_to(det) fig, ax = figure_factory() ax.imshow(dtcr.data, origin="lower") def plot_hist(self, det, **kwargs): + """Plot effect histogram.""" dtcr = self.apply_to(det) fig, ax = figure_factory() ax.hist(dtcr.data.flatten()) @@ -124,16 +127,107 @@ def apply_to(self, det, **kwargs): return det def plot(self, det): + """Plot effect image.""" dtcr = self.apply_to(det) fig, ax = figure_factory() ax.imshow(dtcr.data) def plot_hist(self, det, **kwargs): + """Plot effect histogram.""" dtcr = self.apply_to(det) fig, ax = figure_factory() ax.hist(dtcr.data.flatten()) +# TODO: Is this really a "noise" effect? Sounds more like "electrons" tbh. +class PixelResponseNonUniformity(Effect): + """Pixel Response Non-Uniformity (PRNU). + + Models the fixed pattern of per-pixel gain variations across the detector + arising from manufacturing differences in quantum efficiency. Each pixel is + multiplied by a gain factor drawn from N(1, ``prnu_std``) keyed by detector + ID. The gain map is generated once per detector on first use and reused + identically across all subsequent exposures. + + .. versionadded:: 0.11.3 + + Parameters + ---------- + prnu_std : float or dict + Standard deviation of the per-pixel gain distribution. + + prnu_seed : int, fixed + + include: "!DET.include_prnu" + + Example + ------- + :: + + - name: prnu + description: Pixel response non-uniformity + class: PixelResponseNonUniformity + kwargs: + prnu_std: 0.001 + prnu_seed: 42 + include: "!DET.include_prnu" + + """ + + required_keys: ClassVar[set] = set() + z_order: ClassVar[tuple[int, ...]] = (805,) + + def __init__(self, **kwargs): + super().__init__(**kwargs) + self.meta.update(kwargs) + self._gain_maps = {} # keyed by dtcr_id + + def apply_to(self, obj, **kwargs): + if not isinstance(obj, Detector): + return obj + + random_seed = from_currsys(self.meta.get("prnu_seed"), self.cmds) + id_key = real_colname("id", obj.meta) + dtcr_id = obj.meta[id_key] if id_key is not None else None + + prnu_std_meta = from_currsys(self.meta["prnu_std"], self.cmds) + if isinstance(prnu_std_meta, dict): + prnu_std = float(from_currsys(prnu_std_meta[dtcr_id], self.cmds)) + elif isinstance(prnu_std_meta, Real): + prnu_std = float(prnu_std_meta) + else: + raise TypeError( + ".meta['prnu_std'] must be a float " + f"or a dict keyed by detector ID, got {type(prnu_std_meta)}" + ) + + shape = obj._hdu.data.shape + if dtcr_id not in self._gain_maps: + rng = np.random.default_rng(random_seed) + self._gain_maps[dtcr_id] = rng.normal( + loc=1.0, scale=prnu_std, size=shape, + ) + + if self._gain_maps[dtcr_id].shape != shape: + raise ValueError("gain map shape mismatch") + + obj._hdu.data = obj._hdu.data * self._gain_maps[dtcr_id] + return obj + + def plot(self, det_id=None): + """Plot effect.""" + if not self._gain_maps: + raise RuntimeError("No gain map yet - run a simulation first.") + key = det_id if det_id in self._gain_maps else next(iter(self._gain_maps)) + gain_map = self._gain_maps[key] + dev = np.max(np.abs(gain_map - 1.0)) + fig, ax = figure_factory() + im = ax.imshow(gain_map, origin="lower", aspect="auto", + vmin=1 - dev, vmax=1 + dev) + fig.colorbar(im, ax=ax, label="per-pixel gain") + return fig + + class ShotNoise(Effect): z_order: ClassVar[tuple[int, ...]] = (820,) @@ -196,11 +290,13 @@ def apply_to(self, det, **kwargs): return det def plot(self, det): + """Plot effect image.""" dtcr = self.apply_to(det) fig, ax = figure_factory() ax.imshow(dtcr.data) def plot_hist(self, det, **kwargs): + """Plot effect histogram.""" dtcr = self.apply_to(det) fig, ax = figure_factory() ax.hist(dtcr.data.flatten()) @@ -225,8 +321,8 @@ def apply_to(self, obj, **kwargs): if isinstance(from_currsys(self.meta["value"], self.cmds), dict): dtcr_id = obj.meta[real_colname("id", obj.meta)] dark = from_currsys(self.meta["value"][dtcr_id], self.cmds) - elif isinstance(from_currsys(self.meta["value"], self.cmds), float): - dark = from_currsys(self.meta["value"], self.cmds) + elif isinstance(from_currsys(self.meta["value"], self.cmds), Real): + dark = float(from_currsys(self.meta["value"], self.cmds)) else: raise ValueError(".meta['value'] must be either " f"dict or float, but is {self.meta['value']}") @@ -240,6 +336,7 @@ def apply_to(self, obj, **kwargs): return obj def plot(self, det, **kwargs): + """Plot effect.""" dit = from_currsys(self.meta["dit"], self.cmds) ndit = from_currsys(self.meta["ndit"], self.cmds) total_time = dit * ndit diff --git a/scopesim/effects/illumination.py b/scopesim/effects/illumination.py new file mode 100644 index 00000000..eaa34085 --- /dev/null +++ b/scopesim/effects/illumination.py @@ -0,0 +1,208 @@ +# -*- coding: utf-8 -*- +"""Image-plane illumination effects.""" + +from typing import ClassVar +from collections.abc import Callable, Mapping + +import numpy as np +from astropy import units as u +from astropy.modeling.functional_models import Gaussian2D + +from . import Effect +from ..optics.image_plane import ImagePlane +from ..utils import figure_factory + + +__all__ = ["Illumination", "gaussian2d", "quadratic_vignetting"] + + +def gaussian2d( + shape: tuple[int, int], + amp: float = 1.0, + mu: tuple[float, float] = (0.0, 0.0), + sigma: tuple[float, float] = (2000.0, 2000.0), + theta: u.Quantity[u.deg] | float = 0.0 * u.deg, +) -> np.ndarray: + """ + 2D elliptical Gaussian to be used for vignetting map. + + .. versionadded:: 0.11.3 + + Parameters + ---------- + shape : tuple[int, int] + Image shape in pixels (ny, nx). + amp : float, optional + Peak throughput. The default is 1.0. + mu : tuple[float, float], optional + Offset of the peak center in pixels (x, y) from the image center. + The default is (0.0, 0.0), i.e. no offset. + sigma : tuple[float, float], optional + Gaussian widths in pixels (sx, sy). The default is (2000.0, 2000.0). + theta : float, optional + Rotation angle (if float, the angle is interpreted in degrees), + counterclockwise. The default is 0°. + + Returns + ------- + np.ndarray + Vignetting map. + + """ + nx, ny = reversed(shape) + y, x = np.ogrid[:ny, :nx] + x = x - nx / 2 + y = y - ny / 2 + + model = Gaussian2D( + amplitude=amp, + x_mean=mu[0], + y_mean=mu[1], + x_stddev=sigma[0], + y_stddev=sigma[1], + theta=theta << u.deg, + ) + return model(x, y) + + +def quadratic_vignetting( + shape: tuple[int, int], + falloff: float = 0.01, + r_ref: float | None = None, + mu: tuple[float, float] = (0.0, 0.0), + stretch: tuple[float, float, float, float] = (1.0, 1.0, 1.0, 1.0), +) -> np.ndarray: + """ + Quadratic vignetting pattern with independent stretch factors. + + .. versionadded:: 0.11.3 + + Parameters + ---------- + shape : tuple[int, int] + Image shape in pixels (ny, nx). + falloff : float, optional + Fractional illumination drop at `r_ref`. The default is 0.01 (= 1 %). + r_ref : float | None, optional + Reference radius in stretched pixels. If None (the default), use the + corner distance. + mu : tuple[float, float], optional + Offset of the vignetting center in pixels (x, y) from the image center. + The default is (0.0, 0.0), i.e. no offset. + stretch : tuple[float, float, float, float], optional + ``(+x, -x, +y, -y)`` independent scale factors for half-planes + respectively. All 1.0 gives a circular pattern. A value > 1 widens the + falloff in that direction (shallower); < 1 narrows it (steeper). + The default is (1.0, 1.0, 1.0, 1.0). + + Returns + ------- + np.ndarray + Vignetting map. + + """ + nx, ny = reversed(shape) + + yy, xx = np.ogrid[:ny, :nx] + dx = xx - (nx / 2 + mu[0]) + dy = yy - (ny / 2 + mu[1]) + + sx = np.where(dx >= 0, stretch[0], stretch[1]) + sy = np.where(dy >= 0, stretch[2], stretch[3]) + + r2 = (dx / sx)**2 + (dy / sy)**2 + + if r_ref is None: + r2_ref = r2.max() + else: + r2_ref = r_ref**2 + + return np.clip(1.0 - falloff * r2 / r2_ref, 0.0, 1.0) + + +class Illumination(Effect): + """Large-scale illumination variation across the image plane. + + .. versionadded:: 0.11.3 + + Parameters + ---------- + model : callable, optional + Function ``f(shape, **kwargs) -> ndarray`` returning the + illumination map. Defaults to :func:`gaussian2d`. + modelargs : dict, optional + Keyword arguments forwarded to ``model``. If omitted, the model's + own defaults are used. + + include : str + Turn effect on/off from the IRDB + default.yaml. Defaults to ``"!DET.include_illumination"``. + + Examples + -------- + Polynomial vignetting with <1 % falloff (auto r_ref from image shape) + + >>> eff = Illumination( + ... model=quadratic_vignetting, + ... modelargs={"falloff": 0.01}, + ... ) + + Custom model + + >>> def my_model(shape, slope=-0.001): + >>> ny, nx = shape[-2], shape[-1] + >>> y, x = np.ogrid[:ny, :nx] + >>> r = np.sqrt((x - nx / 2)**2 + (y - ny / 2)**2) + >>> return np.clip(1 + slope * r, 0, None) + >>> + >>> eff = Illumination(model=my_model, modelargs={"slope": -0.0005}) + + """ + + z_order: ClassVar[tuple[int, ...]] = (750,) + + def __init__( + self, + model: Callable = gaussian2d, + modelargs: Mapping | None = None, + **kwargs, + ) -> None: + super().__init__(**kwargs) + self.meta.setdefault("include", "!DET.include_illumination") + self._model = model + self._modelargs = modelargs or {} + self._map = None + self._map_shape = None + + def apply_to(self, obj, **kwargs): + if not isinstance(obj, ImagePlane): + return obj + + shape = obj.hdu.data.shape + if self._map is None or shape != self._map_shape: + self._map = self._make_map(shape) + self._map_shape = shape + + obj.hdu.data *= self._map + return obj + + def _make_map(self, shape): + illumination_map = self._model(shape, **self._modelargs) + return illumination_map.astype(np.float32) + + def plot(self): + """Plot effect.""" + if self._map is None: + raise RuntimeError( + "No illumination map cached — run a simulation first." + ) + + fig, ax = figure_factory() + im = ax.imshow( + self._map, origin="lower", vmin=0.98, vmax=1., cmap="gray_r", + ) + fig.colorbar(im, ax=ax, label="Relative illumination") + ax.set_title("Illumination") + ax.set_xlabel("x [px]") + ax.set_ylabel("y [px]") + return fig diff --git a/scopesim/effects/metis_wcu/metis_wcu.py b/scopesim/effects/metis_wcu/metis_wcu.py index 0a03ca75..02086fa5 100644 --- a/scopesim/effects/metis_wcu/metis_wcu.py +++ b/scopesim/effects/metis_wcu/metis_wcu.py @@ -18,7 +18,7 @@ import yaml from .fpmask import FPMask -from ..ter_curves import TERCurve, FilterCurve +from ..ter_curves import TERCurve from ...utils import get_logger, seq, find_file, from_currsys from ...source.source import Source from ...source.source_fields import BackgroundSourceField @@ -124,6 +124,7 @@ def __init__(self, **kwargs): self.rho_tube = get_reflectivity(self.meta["rho_tube"]) self.rho_is = get_reflectivity(self.meta["rho_is"]) self.emiss_mask = self.meta["emiss_mask"] + self.fibre_trans = self.meta["fibre_transmission"] # Compute the emission components self.compute_lamp_emission() @@ -207,13 +208,15 @@ def get_wavelength(self): dlam = self.cmds["!SIM.spectral.spectral_bin_width"] lam = seq(lamc - 3200 * dlam, lamc + 3200 * dlam, dlam) * u.um else: - filter_name = self.cmds["!OBS.filter_name"] - filename_format = self.cmds["!INST.filter_file_format"] - tempfilter = FilterCurve(filter_name=filter_name, - filename_format=filename_format) - lammin, lammax = tempfilter.throughput.waverange << u.um + #filter_name = self.cmds["!OBS.filter_name"] + #filename_format = self.cmds["!INST.filter_file_format"] + #tempfilter = FilterCurve(filter_name=filter_name, + # filename_format=filename_format) + #lammin, lammax = tempfilter.throughput.waverange << u.um + lammin = self.cmds["!SIM.spectral.wave_min"] + lammax = self.cmds["!SIM.spectral.wave_max"] dlam = self.cmds["!SIM.spectral.spectral_bin_width"] - lam = seq(lammin.value, lammax.value, dlam) * u.um + lam = seq(lammin, lammax, dlam) * u.um self.wavelength = lam @@ -417,9 +420,10 @@ def _laser_intensity(self): """ Compute the intensity for the single-line lasers. - The function computes both lasers at once. This is possible because the - lines are so far apart that there is no band that sees them both. + The function computes all three lasers at once. This is possible because + the lines are so far apart that there is no band that sees them both. """ + print("Computing laser intensity") lam = self.wavelength dlam = lam[1] - lam[0] @@ -438,6 +442,11 @@ def _laser_intensity(self): lamc_m = 5.26 * u.um power_m = 20e-3 * u.W / (c.c * c.h / lamc_m) * u.ph + # Apply fibre transmission + power_l *= self.fibre_trans + power_t *= self.fibre_trans + power_m *= self.fibre_trans + sigma = 2 * dlam amp = 1/(sigma * np.sqrt(2 * np.pi)) @@ -447,8 +456,9 @@ def _laser_intensity(self): line_t = sum(list_t[1:], start=list_t[0]) flux = ((power_l * line_l(lam) + power_m * line_m(lam) + power_t - * line_t(lam)) / (np.pi * self.d_is**2 / 4)) + * line_t(lam)) / (np.pi * self.d_is**2)) + # emergent intensity from the IS output port intens = mult_is * flux / (np.pi * u.sr) return intens.to(self.bb_scale) diff --git a/scopesim/effects/psfs/discrete.py b/scopesim/effects/psfs/discrete.py index 3da2da59..78a1a42b 100644 --- a/scopesim/effects/psfs/discrete.py +++ b/scopesim/effects/psfs/discrete.py @@ -222,14 +222,15 @@ def get_kernel(self, fov): if abs(pix_ratio - 1) > self.meta["flux_accuracy"]: spline_order = from_currsys( "!SIM.computing.spline_order", cmds=self.cmds) - self.kernel = _rescale_kernel(self.kernel, pix_ratio, spline_order) + self.kernel = _rescale_kernel(self.kernel, pix_ratio, + image_header=hdr) if ((fov.header["NAXIS1"] < hdr["NAXIS1"]) or (fov.header["NAXIS2"] < hdr["NAXIS2"])): self.kernel = _cutout_kernel( self.kernel, fov.header, kernel_header=hdr) - return self.kernel + return np.atleast_2d(self.kernel.squeeze()) def make_psf_cube(self, fov): """Create a wavelength-dependent psf cube.""" @@ -452,8 +453,7 @@ def get_kernel(self, fov): spline_order = from_currsys( "!SIM.computing.spline_order", cmds=self.cmds) for ii, kern in enumerate(self.kernel): - self.kernel[ii][0] = _rescale_kernel( - kern[0], pix_ratio, spline_order) + self.kernel[ii][0] = _rescale_kernel(kern[0], pix_ratio) for i, kern in enumerate(self.kernel): self.kernel[i][0] /= np.sum(kern[0]) @@ -510,31 +510,79 @@ def _make_strehl_map_from_table(tbl, pixel_scale=1*u.arcsec): return map_hdu -def _rescale_kernel(image, scale_factor, spline_order): - sum_image = np.sum(image) - image = zoom(image, scale_factor, order=spline_order) - image = np.nan_to_num(image, copy=False) # numpy version >=1.13 - - # Re-centre kernel - im_shape = image.shape - # TODO: this might be another off-by-something - dy, dx = np.divmod(np.argmax(image), im_shape[1]) - np.array(im_shape) // 2 - if dy > 0: - image = image[2*dy:, :] - elif dy < 0: - image = image[:2*dy, :] - if dx > 0: - image = image[:, 2*dx:] - elif dx < 0: - image = image[:, :2*dx] - - sum_new_image = np.sum(image) - image *= sum_image / sum_new_image +def _rescale_kernel(image, scale_factor, method="linear", + image_header=None): + """Rescale `image` by `scale_factor` - return image + Parameters + ---------- + image : array_like, 2D + the image to be rescaled + + scale_factor : float + ratio of input pixel size to output pixel size. Values larger than 1 + zoom the image. + + method : str + interpolation method to be passed to ``RegularGridInterpolator``. + Default is "linear" + + image_header : astropy.fits.Header + an optional image header with a WCS. If ``None``, a WCS is constructed + that counts image pixels. + + Notes + ----- + The function uses ``scipy.interpolate.RegularGridInterpolator``. + The output kernel size is always odd to avoid half-pixel shift when + convolved with an image with ``mode="same"``. + """ + nxin, nyin = image.shape + interp_img = RegularGridInterpolator( + (np.arange(nyin), np.arange(nxin)), + image, method=method, + bounds_error=False, + fill_value=0, + ) + + # Make the output size odd so that the image remains centred (important + # for PSF convolution). + nxout = int(nxin * scale_factor) + if nxout % 2 == 0: + nxout += 1 + nyout = int(nyin * scale_factor) + if nyout % 2 == 0: + nyout += 1 + + if image_header is not None: + inwcs = WCS(image_header) + outwcs = WCS(image_header) + outwcs.wcs.crpix = [(nxout + 1)/2, (nyout + 1)/2] + outwcs.wcs.cdelt = inwcs.wcs.cdelt / scale_factor + else: + inwcs = WCS(naxis=2) + inwcs.wcs.ctype = ["LINEAR", "LINEAR"] + inwcs.wcs.crpix = [(nxin + 1)/2, (nyin + 1)/2] + inwcs.wcs.crval = [0., 0.] + inwcs.wcs.cdelt = [1, 1] + outwcs = WCS(naxis=2) + outwcs.wcs.ctype = ["LINEAR", "LINEAR"] + outwcs.wcs.crpix = [(nxout + 1)/2, (nyout + 1)/2] + outwcs.wcs.crval = [0., 0.] + outwcs.wcs.cdelt = inwcs.wcs.cdelt / scale_factor + xout, yout = np.meshgrid(np.arange(nxout), np.arange(nyout)) + xworld, yworld = outwcs.all_pix2world(xout, yout, 0) + xin, yin = inwcs.all_world2pix(xworld, yworld, 0) + outimage = interp_img( (yin.ravel(), xin.ravel()) ).reshape((nyout, nxout)) + logger.info("Interpolating PSF onto %s image", outimage.shape) + + outimage *= image.sum() / outimage.sum() + + return outimage def _cutout_kernel(image, fov_header, kernel_header=None): + logger.debug("Going into _cutout_kernel") wk = WCS(kernel_header) h, w = image.shape xcen, ycen = 0.5 * w, 0.5 * h diff --git a/scopesim/effects/psfs/psf_base.py b/scopesim/effects/psfs/psf_base.py index 613ac012..11a1b7cc 100644 --- a/scopesim/effects/psfs/psf_base.py +++ b/scopesim/effects/psfs/psf_base.py @@ -49,7 +49,7 @@ def __init__(self, **kwargs): "wave_key": "WAVE0", "normalise_kernel": True, "rounded_edges": True, - "rotational_blur_angle": 0, + "rotational_blur_angle": 0*u.deg, } self.meta.update(params) self.meta.update(kwargs) @@ -74,9 +74,13 @@ def apply_to(self, obj, **kwargs): (obj.hdu is not None)): kernel = self.get_kernel(obj).astype(float) + # This doesn't work because of a "Delta PSF" in some mocks... + # if kernel.size == 1: # only 1 pixel + # raise ValueError("Cannot convolve single pixel PSF.") + # apply rotational blur for field-tracking observations rot_blur_angle = self.meta["rotational_blur_angle"] - if abs(rot_blur_angle) > 0: + if abs(rot_blur_angle << u.deg) > 0*u.deg: # makes a copy of kernel kernel = rotational_blur(kernel, rot_blur_angle) @@ -150,35 +154,41 @@ def plot(self, obj=None, **kwargs): return fig -def rotational_blur(image, angle): +@u.quantity_input +def rotational_blur(image, angle: u.Quantity[u.deg]): """ Rotate and coadd an image over a given angle to imitate a blur. Parameters ---------- - image : array - Image to blur - angle : float - [deg] Angle over which the image should be rotationally blurred + image : array-like + Image to blur. + angle : u.Quantity["angle"] + Angle over which the image should be rotationally blurred. + + .. versionchanged:: 0.11.3 + + Require `angle` to be a Quantity. Returns ------- - image_rot : array + image_rot : np.ndarray Blurred image """ image_rot = np.copy(image) - n_angles = 1 - rad_to_deg = 57.29578 - edge_pixel_unit_angle = np.arctan2(1, (image.shape[0] // 2)) * rad_to_deg - while abs(angle) > edge_pixel_unit_angle and n_angles < 25: - angle /= 2. - image_rot += rotate(image_rot, angle, reshape=False, order=1) + edge_pixel_unit_angle = np.arctan2(1, (image.shape[0] // 2)) * u.rad + n_steps = np.ceil(np.log2(abs(angle) / edge_pixel_unit_angle)) + n_steps = int(min(n_steps, 8)) # avoid overrun + + current_angle = angle.copy() + for _ in range(n_steps): + current_angle /= 2. + image_rot += rotate(image_rot, current_angle, reshape=False, order=3) # each time kernel is rotated and added, the frame total doubles - n_angles *= 2 - return image_rot / n_angles + return image_rot / image_rot.sum() * image.sum() def get_bkg_level(obj, bg_w): diff --git a/scopesim/effects/psfs/semianalytical.py b/scopesim/effects/psfs/semianalytical.py index 6d26b48a..1b12aa4e 100644 --- a/scopesim/effects/psfs/semianalytical.py +++ b/scopesim/effects/psfs/semianalytical.py @@ -11,10 +11,18 @@ from .. import ter_curves_utils as tu from ...optics.fov import FieldOfView -from ...utils import (figure_factory, figure_grid_factory, from_currsys, - quantify, check_keys) +from ...utils import ( + figure_factory, + figure_grid_factory, + from_currsys, + quantify, + check_keys, + get_logger, +) from . import PSF +logger = get_logger(__name__) + class SemiAnalyticalPSF(PSF): """Base class for semianalytical PSFs.""" @@ -115,9 +123,11 @@ def get_kernel(self, fov): n = self.meta["psf_side_length"] wave = self.wavelength + logger.debug(" start AnisoCADO") self._psf_object = aniso.AnalyticalScaoPsf(pixelSize=pixel_scale, N=n, wavelength=wave, nmRms=self.nmRms) + logger.debug(" done AnisoCADO") if np.any(self.meta["offset"]): self._psf_object.shift_off_axis(self.meta["offset"][0], self.meta["offset"][1]) diff --git a/scopesim/effects/spectral_trace_list.py b/scopesim/effects/spectral_trace_list.py index 45120f9f..d455fc08 100644 --- a/scopesim/effects/spectral_trace_list.py +++ b/scopesim/effects/spectral_trace_list.py @@ -89,6 +89,10 @@ class SpectralTraceList(Effect): - x : float : [mm] : x position of aperture image on focal plane - y : float : [mm] : y position of aperture image on focal plane + .. versionchanged:: 0.11.3 + + Added support for slit offset. + """ _class_params = { @@ -121,13 +125,14 @@ def __init__(self, **kwargs): "x_colname": "x", "y_colname": "y", "s_colname": "s", + "offset_x": 0, # [mm] in detector plane + "offset_y": 0, # [mm] in detector plane "wave_colname": "wavelength", "center_on_wave_mid": False, "dwave": 0.002, # [um] for finding the best fit dispersion "invalid_value": None, # for dodgy trace file values } self.meta.update(params) - # Parameters that are specific to the subclass self.meta.update(self._class_params) self.meta.update(kwargs) @@ -239,6 +244,18 @@ def apply_to(self, obj, **kwargs): logger.info("Making cube") obj.cube = obj.make_hdu() + # Check whether an offset slit is used. If so, recompute spectral traces. + offset_x = obj.cube.header["CRVAL1D"] + offset_y = obj.cube.header["CRVAL2D"] + if (offset_x != self.meta["offset_x"] or + offset_y != self.meta["offset_y"]): + logger.debug("Recomputing spectral traces for offset (%.1g, %.1g)", + offset_x, offset_y) + self.meta["offset_x"] = offset_x + self.meta["offset_y"] = offset_y + self.make_spectral_traces() + self.update_meta() + spt = self.spectral_traces[obj.trace_id] obj.hdu = spt.map_spectra_to_focal_plane(obj) @@ -333,7 +350,7 @@ def rectify_traces(self, hdulist, xi_min=None, xi_max=None, interps=None, bin_width = kwargs.get("bin_width", None) if interps is None: - logger.info("Computing interpolation functions") + logger.debug("Computing interpolation functions") interps = make_image_interpolations(hdulist) pdu = fits.PrimaryHDU() diff --git a/scopesim/effects/spectral_trace_list_utils.py b/scopesim/effects/spectral_trace_list_utils.py index 44b4f5a5..7541f9cb 100644 --- a/scopesim/effects/spectral_trace_list_utils.py +++ b/scopesim/effects/spectral_trace_list_utils.py @@ -49,6 +49,8 @@ class SpectralTrace: "x_colname": "x", "y_colname": "y", "s_colname": "s", + "offset_x": 0, + "offset_y": 0, "wave_colname": "wavelength", "dwave": 0.002, "aperture_id": 0, @@ -119,9 +121,12 @@ def compute_interpolation_functions(self): Focal plane coordinates are `x` and `y`, in mm. Slit coordinates are `xi` (spatial coordinate along the slit, in arcsec) and `lam` (wavelength, in um). + + The interpolation functions include a shift in the focal-plane + coordinates, determined from the CRVAL of the source FOV. """ - x_arr = self.table[self.meta["x_colname"]] - y_arr = self.table[self.meta["y_colname"]] + x_arr = self.table[self.meta["x_colname"]] + self.meta["offset_x"] + y_arr = self.table[self.meta["y_colname"]] + self.meta["offset_y"] xi_arr = self.table[self.meta["s_colname"]] lam_arr = self.table[self.meta["wave_colname"]] @@ -317,18 +322,17 @@ def rectify(self, hdulist, interps=None, wcs=None, **kwargs): Spatial limits of the slit on the sky. This should be taken from the header of the hdulist, but this is not yet provided by scopesim """ - logger.info("Rectifying %s", self.trace_id) - wave_min = kwargs.get("wave_min", self.wave_min) wave_max = kwargs.get("wave_max", self.wave_max) if wave_max < self.wave_min or wave_min > self.wave_max: - logger.info(" Outside filter range") + logger.debug(" Outside filter range") return None wave_min = max(wave_min, self.wave_min) wave_max = min(wave_max, self.wave_max) - logger.info(" %.02f .. %.02f um", wave_min, wave_max) + logger.info("Rectifying %s (%.02f .. %.02f um)", + self.trace_id, wave_min, wave_max) # bin_width is taken as the minimum dispersion of the trace # ..todo: if wcs is given take bin width from cdelt1 @@ -336,7 +340,7 @@ def rectify(self, hdulist, interps=None, wcs=None, **kwargs): if bin_width is None: self._set_dispersion(wave_min, wave_max) bin_width = np.abs(self.dlam_per_pix.y).min() - logger.info(" Bin width %.02g um", bin_width) + logger.debug(" Bin width %.02g um", bin_width) pixscale = from_currsys(self.meta["pixel_scale"], self.cmds) diff --git a/scopesim/effects/ter_curves.py b/scopesim/effects/ter_curves.py index 962c311b..c653fd73 100644 --- a/scopesim/effects/ter_curves.py +++ b/scopesim/effects/ter_curves.py @@ -1065,7 +1065,7 @@ def update_transmission(self, transmission, **kwargs): """Set a new transmission value""" self.surface = SpectralSurface(wavelength=self.meta['wavelength'], transmission=[transmission, transmission], - emission=[0, 0]) + emissivity=[0., 0.], **kwargs) self.meta.update(self.surface.meta) diff --git a/scopesim/optics/image_plane.py b/scopesim/optics/image_plane.py index ba192456..794c03fb 100644 --- a/scopesim/optics/image_plane.py +++ b/scopesim/optics/image_plane.py @@ -152,7 +152,7 @@ def add(self, hdus_or_tables, sub_pixel=None, spline_order=None, logger.warning("Added mismatched BUNIT %s to %s.", img_bunit, imp_bunit) else: - logger.info("No BUNIT found in added HDU.") + logger.warning("No BUNIT found in added HDU.") @property def header(self): diff --git a/scopesim/optics/optical_train.py b/scopesim/optics/optical_train.py index 24cf178b..4b3448cb 100644 --- a/scopesim/optics/optical_train.py +++ b/scopesim/optics/optical_train.py @@ -158,6 +158,15 @@ def load(self, user_commands): # Nevertheless, I'm a bit reluctant to removing this code just # yet. So it is commented out. # rc.__currsys__ = user_commands + + # Guard against all-empty cmds to avoid cryptical error downstream. + if all(len(m) == 0 for m in self.cmds.maps): + raise ValueError("Empty cmds, cannot construct OpticalTrain.") + + # Guard against empty yamls to avoid cryptical error downstream. + if not self.cmds.yaml_dicts: + raise ValueError("No YAMLS found, cannot construct OpticalTrain.") + self.yaml_dicts = self.cmds.yaml_dicts self.optics_manager = OpticsManager(self.yaml_dicts, self.cmds) self.update() @@ -358,6 +367,7 @@ def prepare_source(self, source): # ..todo: lower needed because "DEG" is not understood, this is ugly pixarea = (header["CDELT1"] * u.Unit(header["CUNIT1"].lower()) * header["CDELT2"] * u.Unit(header["CUNIT2"].lower())).to(u.arcsec**2) + pixarea = np.abs(pixarea) # CDELTi can be negative, pixarea cannot data = data / pixarea.value # cube is per arcsec2 data = (data * factor).value diff --git a/scopesim/optics/optics_manager.py b/scopesim/optics/optics_manager.py index 74a9c8cb..08649848 100644 --- a/scopesim/optics/optics_manager.py +++ b/scopesim/optics/optics_manager.py @@ -7,6 +7,8 @@ from collections.abc import Sequence import numpy as np +from matplotlib import pyplot as plt + from astropy import units as u from astropy.table import Table from synphot import SpectralElement, Empirical1D @@ -253,20 +255,52 @@ def all_effects(self) -> list[efs.Effect]: """Get all effects in all optical elements.""" return [eff for opt_eff in self.optical_elements for eff in opt_eff] - @property - def system_transmission(self): + def system_transmission(self, plot=False): + """Compute system transmission + + The method computes the total system transmission and returns it as a + ``synphot.spectrum.SpectralElement``. + + When ``plot`` is ``True``, it creates a plot of the transmission + curves of the indivdual elements in the system as well as the system + transmission. + """ wave_unit = u.Unit(from_currsys("!SIM.spectral.wave_unit", self.cmds)) dwave = from_currsys("!SIM.spectral.spectral_bin_width", self.cmds) wave_min = from_currsys("!SIM.spectral.wave_min", self.cmds) wave_max = from_currsys("!SIM.spectral.wave_max", self.cmds) wave = np.arange(wave_min, wave_max, dwave) - trans = np.ones_like(wave) sys_trans = SpectralElement(Empirical1D, points=wave*u.Unit(wave_unit), - lookup_table=trans) + lookup_table=np.ones_like(wave)) for effect in self.get_z_order_effects(100): sys_trans *= effect.throughput + if plot: + # only plot range where sys_trans is larger than zero + wave <<= wave_unit + transval = sys_trans(wave).value + wmin = np.min(wave[transval > 0.01]) + wmax = np.max(wave[transval > 0.01]) + wmin = wmin - 0.1 * (wmax - wmin) + wmax = wmax + 0.1 * (wmax - wmin) + wave = wave[(wave > wmin) * (wave < wmax)] + + _, ax = plt.subplots() + for effect in self.get_z_order_effects(100): + lw, alpha = 2, 1 + if isinstance(effect, efs.SkycalcTERCurve): + lw, alpha = 1, 0.5 + ax.plot(wave, effect.throughput(wave), lw=lw, alpha=alpha, + label=effect.display_name) + ax.plot(wave, sys_trans(wave), lw=2, color="black", + label="System transmission") + ax.legend(bbox_to_anchor=(0.5, 1.02), fancybox=True, + loc="lower center", ncol=2) + ax.set_xlabel("Wavelength [um]") + ax.set_ylabel("Transmission") + plt.show() + return sys_trans @property diff --git a/scopesim/server/database.py b/scopesim/server/database.py index e1d73cc0..f7d92560 100644 --- a/scopesim/server/database.py +++ b/scopesim/server/database.py @@ -7,7 +7,7 @@ from collections.abc import Iterator, Iterable, Mapping import yaml -import httpx +import httpxyz as httpx from more_itertools import first, last, groupby_transform from .github_utils import download_github_folder diff --git a/scopesim/server/download_utils.py b/scopesim/server/download_utils.py index fbce1817..2ea7e127 100644 --- a/scopesim/server/download_utils.py +++ b/scopesim/server/download_utils.py @@ -6,7 +6,7 @@ from zipfile import ZipFile from pathlib import Path -import httpx +import httpxyz as httpx import bs4 import pooch diff --git a/scopesim/server/psfs_registry.txt b/scopesim/server/psfs_registry.txt index cd4fe1b5..94e64c92 100644 --- a/scopesim/server/psfs_registry.txt +++ b/scopesim/server/psfs_registry.txt @@ -4,8 +4,8 @@ METIS_psfs/PSF_CLS-LM.fits e4f52b5942180f1b60b297b3a42780d3ec3df3c9afe7215157e04 METIS_psfs/PSF_CLS-N-b.fits 7cda4d44bdffb5fb781cefe77060dee52ba7c46bb104e7d16324bfc0320759f6 METIS_psfs/PSF_CLS-N.fits e0823e79d3279f312b14b7bbd64e8fd0c9754e0213b6e242dda51cc6d4491c79 METIS_psfs/PSF_METISsim.fits 1532f32036e8a446fe30e115e161a6d09873179a4f8ad52cc2a9cf1355c4840c -METIS_psfs/PSF_PPS-CFO2.fits e5bc55a4657b41ef6f242f1600efcc83199d4dc9149fd99673200621a0471004 -METIS_psfs/PSF_PPS-CFO2_WCU.fits ddb21c55f4a6295fe0202abef11e8ca76d5538948e20c63ded76751fd7ec4705 +METIS_psfs/PSF_PPS-CFO2.fits 2a65e6f6794c083305422cf38beff5296e8abf596bd0ffa8f2b1ef32db07e89b +METIS_psfs/PSF_PPS-CFO2_WCU.fits d30b20bd3e38efd4433a0d59a319e2a49d21cef61fab0836f76e6b203d53ba2e METIS_psfs/PSF_PPS-LM.fits fddbb4bda2f4c83eabe757b783b6a55ea10a5b24936cc57f8ae189757dbd4c27 METIS_psfs/PSF_PPS-LM_WCU.fits d17b7f2bcc85a5dffe03aea6e2e4f284ea8575800d9ee68a9b4d7a29753e03d1 METIS_psfs/PSF_PPS-N.fits 5cb3d370c2eb8f852aa83c31960d9fb8fa7d60c2cddaa114f2e6d4fa9b646092 diff --git a/scopesim/source/source_fields.py b/scopesim/source/source_fields.py index 2745e9e9..3ca2a2c1 100644 --- a/scopesim/source/source_fields.py +++ b/scopesim/source/source_fields.py @@ -81,6 +81,7 @@ class HDUSourceField{+wcs} convert_table_comments_to_dict, unit_includes_per_physical_type, pixel_area, + ScopesimPendingDeprecationWarning, ) @@ -109,7 +110,7 @@ def __getitem__(self, key): # this and force the use of .field... warn("Direct item access for source fields may become deprecated " "in the future. Use the .field attribute instead.", - PendingDeprecationWarning, stacklevel=2) + ScopesimPendingDeprecationWarning, stacklevel=2) return self.field.__getitem__(key) def __setitem__(self, key, value): @@ -118,7 +119,7 @@ def __setitem__(self, key, value): # this and force the use of .field... warn("Direct item assignment for source fields may become deprecated " "in the future. Use the .field attribute instead.", - PendingDeprecationWarning, stacklevel=2) + ScopesimPendingDeprecationWarning, stacklevel=2) self.field.__setitem__(key, value) @property diff --git a/scopesim/tests/tests_effects/test_ConstPSF.py b/scopesim/tests/tests_effects/test_ConstPSF.py index 3a798de3..7f6ae9a8 100644 --- a/scopesim/tests/tests_effects/test_ConstPSF.py +++ b/scopesim/tests/tests_effects/test_ConstPSF.py @@ -20,6 +20,7 @@ from pytest import approx import numpy as np +from numpy import testing as npt import matplotlib.pyplot as plt @@ -39,15 +40,20 @@ def centre_fov(): return _centre_fov() +@pytest.fixture(scope="function") +def const_psf(mock_path): + constpsf = FieldConstantPSF( + filename=str(mock_path / "test_ConstPSF.fits")) + return constpsf + + class TestInit: def test_errors_when_initialised_with_nothing(self): with pytest.raises(ValueError): isinstance(FieldConstantPSF(), FieldConstantPSF) - def test_initialised_when_passed_fits_filename(self, mock_path): - constpsf = FieldConstantPSF( - filename=str(mock_path / "test_ConstPSF.fits")) - assert isinstance(constpsf, FieldConstantPSF) + def test_initialised_when_passed_fits_filename(self, const_psf): + assert isinstance(const_psf, FieldConstantPSF) def test_initialised_when_passed_fits_filename_with_waveleng(self, mock_path): @@ -61,9 +67,11 @@ def test_initialised_with_psf_name_and_file_format(self, mock_path): # actually tests code in parent class DiscretePSF psf_name = "ConstPSF" file_format = "test_{}_WAVELENG.fits" - constpsf = FieldConstantPSF(psf_name=psf_name, - psf_path=mock_path, - filename_format=file_format) + constpsf = FieldConstantPSF( + psf_name=psf_name, + psf_path=mock_path, + filename_format=file_format, + ) assert isinstance(constpsf, FieldConstantPSF) @@ -74,33 +82,45 @@ class TestGetKernel: ([1.9, 2.5], 1.), ([0.9, 1.1], 1 / 3.), ([1.875, 1.876], 1.)]) - def test_returns_array_with_single_kernel_from_fov(self, waves, max_pixel, - mock_path): - constpsf = FieldConstantPSF( - filename=str(mock_path / "test_ConstPSF.fits")) + def test_returns_array_with_single_kernel_from_fov( + self, + waves, + max_pixel, + const_psf, + ): fov = _centre_fov(n=10, waverange=waves) fov.view() - kernel = constpsf.get_kernel(fov) - - assert np.sum(kernel) == approx(1) - assert np.max(kernel) == approx(max_pixel) - - @pytest.mark.parametrize("factor", [1/3., 1, 5]) - def test_kernel_is_scale_properly_if_cdelts_differ(self, factor, - mock_path): + kernel = const_psf.get_kernel(fov) + + npt.assert_allclose(kernel.sum(), 1) + npt.assert_allclose(kernel.max(), max_pixel) + + @pytest.mark.parametrize("scale_factor", ( + pytest.param(1/3, marks=pytest.mark.xfail(reason="PSF center off")), + 1, + pytest.param(5, marks=pytest.mark.xfail(reason="1x1 array turned into scalar")), + )) + def test_kernel_is_scale_properly_if_cdelts_differ( + self, + scale_factor, + const_psf, + ): fov = _centre_fov(n=10, waverange=[1.5, 1.7]) - fov.header["CDELT1"] *= factor - fov.header["CDELT2"] *= factor + fov.header["CDELT1"] *= scale_factor + fov.header["CDELT2"] *= scale_factor fov.view() - constpsf = FieldConstantPSF( - filename=str(mock_path / "test_ConstPSF.fits")) - kernel = constpsf.get_kernel(fov) - - psf_shape = np.array(constpsf._file[2].data.shape) - kernel_shape = kernel.shape + kernel = const_psf.get_kernel(fov) + kernel_shape = np.array(kernel.shape) - assert np.all(kernel_shape == psf_shape / factor) + # Check if kernel is scaled by correct factor in both dimensions + npt.assert_allclose( + const_psf._file[2].data.shape / kernel_shape, + scale_factor, + ) + # Check if max of kernel is in the center pixel + assert (tuple(kernel_shape // 2) == + np.unravel_index(kernel.argmax(), kernel.shape)) class TestApplyTo: @@ -108,25 +128,27 @@ class TestApplyTo: [([1.1, 1.3], 1 / 3.), ([1.5, 1.7], 1 / 3.), ([1.9, 2.5], 1.)]) - def test_convolves_with_basic_fov_for_each_waveleng(self, waves, max_pixel, - mock_path): + def test_convolves_with_basic_fov_for_each_waveleng( + self, + waves, + max_pixel, + const_psf, + ): centre_fov = _centre_fov(n=10, waverange=waves) nax1, nax2 = centre_fov.header["NAXIS1"], centre_fov.header["NAXIS2"] centre_fov.view("image") centre_fov.hdu.data = np.zeros((nax2, nax1)) centre_fov.hdu.data[1::4, 1::4] = 1 - constpsf = FieldConstantPSF( - filename=str(mock_path / "test_ConstPSF.fits")) - fov_returned = constpsf.apply_to(centre_fov) + fov_returned = const_psf.apply_to(centre_fov) if PLOTS: plt.imshow(fov_returned.hdu.data, origin="lower") plt.show() - assert np.max(fov_returned.hdu.data) == approx(max_pixel) + npt.assert_allclose(fov_returned.hdu.data.max(), max_pixel) - def test_convolution_leaves_constant_background_intact(self, mock_path): + def test_convolution_leaves_constant_background_intact(self, const_psf): """FOV object with constant data must be unchanged by PSF convolution 1. Set up initial FOV object with constant data array @@ -139,9 +161,7 @@ def test_convolution_leaves_constant_background_intact(self, mock_path): centre_fov.view() centre_fov.hdu.data = np.ones((nax2, nax1), dtype=np.float32) - constpsf = FieldConstantPSF( - filename=str(mock_path / "test_ConstPSF.fits")) - fov_returned = constpsf.apply_to(centre_fov) + fov_returned = const_psf.apply_to(centre_fov) if PLOTS: fig, (ax1, ax2) = plt.subplots(1, 2, figsize=(7,3)) @@ -153,5 +173,4 @@ def test_convolution_leaves_constant_background_intact(self, mock_path): fig.colorbar(plot_a, ax=ax2) plt.show() - assert np.all(np.equal(fov_returned.hdu.data, - centre_fov.hdu.data)) + npt.assert_array_equal(fov_returned.hdu.data, centre_fov.hdu.data) diff --git a/scopesim/tests/tests_effects/test_MetisWCU.py b/scopesim/tests/tests_effects/test_MetisWCU.py index 4679aabc..5261e406 100644 --- a/scopesim/tests/tests_effects/test_MetisWCU.py +++ b/scopesim/tests/tests_effects/test_MetisWCU.py @@ -7,6 +7,7 @@ import pytest import numpy as np +from numpy import testing as npt from astropy import units as u from scopesim import UserCommands @@ -35,6 +36,7 @@ def _patched_cmds_lss(mode="wcu_lss", filtername="J", bin_width=0.002): @pytest.fixture(name="bbsource", scope="function") def fixture_bbsource(): return WCUSource(current_lamp="bb", + lamps=["bb", "laser", "off"], bb_temp=1000*u.K, is_temp=300*u.K, wcu_temp=300*u.K, @@ -47,6 +49,7 @@ def fixture_bbsource(): diam_is_in=25.4, diam_is_out=100., emiss_bb=0.98, + fibre_transmission=0.1, current_fpmask="open", fpmask_angle=0, fpmask_shift=(0, 0), @@ -59,69 +62,69 @@ def test_wcu_initialises_correctly(self, bbsource): assert isinstance(bbsource, WCUSource) def test_bbsource_has_temperatures(self, bbsource): - assert bbsource.meta['bb_temp'] == 1000 * u.K - assert bbsource.meta['wcu_temp'] == 300 * u.K + npt.assert_equal(bbsource.meta['bb_temp'], 1000 * u.K) + npt.assert_equal(bbsource.meta['wcu_temp'], 300 * u.K) def test_bbsource_has_table(self, bbsource): assert bbsource.surface.table def test_bbsource_table_has_correct_columns(self, bbsource): - assert (bbsource.surface.table.colnames == - ['wavelength', 'transmission', 'emission']) + npt.assert_equal(bbsource.surface.table.colnames, + ['wavelength', 'transmission', 'emission']) def test_bbsource_has_correct_emission_units(self, bbsource): - assert (bbsource.surface.table['emission'].unit == - u.ph / (u.s * u.arcsec**2 * u.um * u.m**2)) + npt.assert_equal(bbsource.surface.table['emission'].unit, + u.ph / (u.s * u.arcsec**2 * u.um * u.m**2)) def test_can_set_bb_temperature(self, bbsource): old_temp = bbsource.meta['bb_temp'] new_temp = 1.5 * old_temp bbsource.set_temperature(new_temp) - assert bbsource.meta['bb_temp'] == new_temp - assert (bbsource.meta['bb_temp_c'] == - np.round((new_temp - 273.15 * u.K).value, 7)) + npt.assert_equal(bbsource.meta['bb_temp'], new_temp) + npt.assert_equal(bbsource.meta['bb_temp_c'], + np.round((new_temp - 273.15 * u.K).value, 7)) def test_can_set_wcu_temperature(self, bbsource): old_temp = bbsource.meta['wcu_temp'] new_temp = old_temp + 12 * u.K bbsource.set_temperature(wcu_temp=new_temp) - assert bbsource.meta['wcu_temp'] == new_temp - assert (bbsource.meta['wcu_temp_c'] == - np.round((new_temp - 273.15 * u.K).value, 7)) + npt.assert_equal(bbsource.meta['wcu_temp'], new_temp) + npt.assert_equal(bbsource.meta['wcu_temp_c'], + np.round((new_temp - 273.15 * u.K).value, 7)) def test_can_set_temperature_in_celsius(self, bbsource): bbsource.set_temperature(bb_temp=30*u.deg_C) - assert bbsource.meta['bb_temp'] == 303.15 * u.K - assert bbsource.meta['bb_temp_c'] == 30 + npt.assert_equal(bbsource.meta['bb_temp'], 303.15 * u.K) + npt.assert_equal(bbsource.meta['bb_temp_c'], 30) def test_can_change_temperature_units_with_float(self, bbsource): bbsource.meta['is_temp'] = 293.15 bbsource._kelvin2celsius() - assert bbsource.meta['is_temp_c'] == 20. + npt.assert_equal(bbsource.meta['is_temp_c'], 20.) def test_ignore_incompatible_units_bb(self, bbsource): old_temp = bbsource.meta['bb_temp'] with pytest.raises(u.UnitConversionError): bbsource.set_temperature(bb_temp=2*u.Jy) - assert bbsource.meta['bb_temp'] == old_temp + npt.assert_equal(bbsource.meta['bb_temp'], old_temp) def test_ignore_incompatible_units_wcu(self, bbsource): old_temp = bbsource.meta['wcu_temp'] with pytest.raises(u.UnitConversionError): bbsource.set_temperature(wcu_temp=2*u.Tesla) - assert bbsource.meta['wcu_temp'] == old_temp + npt.assert_equal(bbsource.meta['wcu_temp'], old_temp) def test_ignore_negative_bb_temperature(self, bbsource): old_temp = bbsource.meta['bb_temp'] with pytest.raises(ValueError): bbsource.set_temperature(bb_temp=-1000 * u.K) - assert bbsource.meta['bb_temp'] == old_temp + npt.assert_equal(bbsource.meta['bb_temp'], old_temp) def test_ignore_negative_wcu_temperature(self, bbsource): old_temp = bbsource.meta['wcu_temp'] with pytest.raises(ValueError): bbsource.set_temperature(wcu_temp=-1000 * u.K) - assert bbsource.meta['wcu_temp'] == old_temp + npt.assert_equal(bbsource.meta['wcu_temp'], old_temp) def test_emission_increases_with_temperature(self, bbsource): """ @@ -137,8 +140,7 @@ def test_emission_increases_with_temperature(self, bbsource): bbsource.set_temperature(bb_temp=new_temp) new_emission = bbsource.surface.emission lam_ref = seq(2.2, 15, 0.1) * u.um - assert all(new_emission(lam_ref) > old_emission(lam_ref)) - + npt.assert_array_less(old_emission(lam_ref), new_emission(lam_ref)) def test_black_body_source_fails_without_parameters(self): with pytest.raises(ValueError): @@ -152,40 +154,45 @@ def test_get_wavelength_for_lms(self, bbsource): bbsource.cmds = _patched_cmds(mode="wcu_lms", wavelen=lamc, bin_width=binw) bbsource.get_wavelength() lam = 3.58 + (np.arange(6401) * binw) - assert len(bbsource.wavelength) == len(lam) - assert np.all(bbsource.wavelength.value == lam) + npt.assert_equal(len(bbsource.wavelength), len(lam)) + npt.assert_array_equal(bbsource.wavelength.value, lam) def test_get_wavelength_for_lss(self, bbsource): + wave_min = 2.85 + wave_max = 14.0 + dlam = 0.002 bbsource.cmds.update(properties={"!OBS.modes": "wcu_lss", - "!SIM.spectral.spectral_bin_width": 0.002, + "!SIM.spectral.spectral_bin_width": dlam, + "!SIM.spectral.wave_min": wave_min, + "!SIM.spectral.wave_max": wave_max, "!OBS.filter_name": "J", "!INST.filter_file_format": "filters/TC_filter_{}.dat"}) print(bbsource.cmds["!OBS.modes"]) bbsource.get_wavelength() - lam = seq(1.15, 1.37, 0.002) - assert np.all(bbsource.wavelength.value == lam) + lam = seq(wave_min, wave_max, dlam) + npt.assert_array_equal(bbsource.wavelength.value, lam) def test_bb_aperture_initialises_correctly(self, bbsource): - assert bbsource.bb_aperture == 1. + npt.assert_equal(bbsource.bb_aperture, 1.) def test_bb_aperture_set_good_value(self, bbsource): bbsource.set_bb_aperture(0.3) - assert bbsource.bb_aperture == 0.3 + npt.assert_equal(bbsource.bb_aperture, 0.3) def test_bb_aperture_set_clip_negative_value(self, bbsource): bbsource.set_bb_aperture(-3) - assert bbsource.bb_aperture == 0 + npt.assert_equal(bbsource.bb_aperture, 0) def test_bb_aperture_set_clip_large_value(self, bbsource): bbsource.set_bb_aperture(13) - assert bbsource.bb_aperture == 1 + npt.assert_equal(bbsource.bb_aperture, 1) @pytest.mark.parametrize("newvalue", [1., 0.6, 0.]) def test_bb_aperture_changes_lamp_emission(self, bbsource, newvalue): bbsource.set_bb_aperture(1.) ref_lamp = bbsource.intens_lamp bbsource.set_bb_aperture(newvalue) - assert np.allclose(bbsource.intens_lamp, newvalue * ref_lamp) + npt.assert_allclose(bbsource.intens_lamp, newvalue * ref_lamp) @pytest.mark.parametrize("newvalue", [1., 0.6, 0.]) def test_bb_aperture_does_not_change_background_emission(self, bbsource, @@ -193,7 +200,18 @@ def test_bb_aperture_does_not_change_background_emission(self, bbsource, bbsource.set_bb_aperture(1.) ref_bg = bbsource.intens_bg bbsource.set_bb_aperture(newvalue) - assert np.all(bbsource.intens_bg == ref_bg) + npt.assert_equal(bbsource.intens_bg, ref_bg) + + def test_laser_brighter_with_fibre_transmission(self, bbsource): + bbsource.set_lamp("laser") + ft_1 = bbsource.fibre_trans + intens_1 = np.sum(bbsource.intens_lamp) + bbsource.fibre_trans = 0.853 + ft_2 = bbsource.fibre_trans + bbsource.set_lamp("laser") + intens_2 = np.sum(bbsource.intens_lamp) + + assert intens_2 / intens_1 == ft_2 / ft_1 @pytest.fixture(name="fpmask", scope="function") @@ -225,10 +243,10 @@ def test_fpmask_open_has_correct_hdus(self, openmask): @pytest.mark.usefixtures("no_file_error") def test_fpmask_uses_file_format(self, fpmask, pinholemask): - assert fpmask.data_container.meta['filename'] == \ - pinholemask.data_container.meta['filename'] - assert np.all(fpmask.holehdu.data == pinholemask.holehdu.data) - assert np.all(fpmask.opaquehdu.data == pinholemask.opaquehdu.data) + npt.assert_equal(fpmask.data_container.meta['filename'], + pinholemask.data_container.meta['filename']) + npt.assert_equal(fpmask.holehdu.data, pinholemask.holehdu.data) + npt.assert_equal(fpmask.opaquehdu.data, pinholemask.opaquehdu.data) def test_has_table(self, fpmask): assert fpmask.data_container.table is not None @@ -242,16 +260,16 @@ def test_has_opaquehdu(self, fpmask): def test_pixarea_correct(self, fpmask): hdr = fpmask.holehdu.header pixarea = hdr['CDELT1'] * hdr['CDELT2'] * u.arcsec**2 - assert fpmask.pixarea == pixarea + npt.assert_equal(fpmask.pixarea, pixarea) def test_data_correct(self, fpmask): - assert fpmask.holehdu.data[241, 1943] == 0 - assert fpmask.holehdu.data[1023, 1023] < 1 - assert fpmask.holehdu.data[1021:1025, 1021:1025].sum() == pytest.approx( - np.pi * (0.007532**2) / 4 / fpmask.pixarea.value) - assert (fpmask.opaquehdu.data[1023, 1023] + fpmask.holehdu.data[1023, 1023] - == 1) - assert fpmask.opaquehdu.data[748, 1308] == 1. + npt.assert_equal(fpmask.holehdu.data[241, 1943], 0) + npt.assert_array_less(fpmask.holehdu.data[1023, 1023], 1) + npt.assert_allclose(fpmask.holehdu.data[1021:1025, 1021:1025].sum(), + np.pi * (0.007532**2) / 4 / fpmask.pixarea.value) + npt.assert_equal (fpmask.opaquehdu.data[1023, 1023] + fpmask.holehdu.data[1023, 1023], + 1) + npt.assert_equal(fpmask.opaquehdu.data[748, 1308], 1.) def test_no_error_with_integer_positions(self, pinholemask_int): """Tests that the bug in Scopesim#868 does not occur""" diff --git a/scopesim/tests/tests_effects/test_PSF.py b/scopesim/tests/tests_effects/test_PSF.py index 6b70a679..c49f3f41 100644 --- a/scopesim/tests/tests_effects/test_PSF.py +++ b/scopesim/tests/tests_effects/test_PSF.py @@ -3,9 +3,11 @@ from pytest import approx import numpy as np from matplotlib import pyplot as plt +from astropy import units as u from scopesim.effects import PSF from scopesim.effects.psfs.psf_base import get_bkg_level +from scopesim.effects.psfs.discrete import _rescale_kernel from scopesim.optics import ImagePlane from scopesim.tests.mocks.py_objects.header_objects import _implane_header @@ -42,9 +44,20 @@ def test_returns_array_from_kernel(self): assert np.sum(psf.kernel) == approx(np.sum(psf.get_kernel(None))) + @pytest.mark.parametrize("nkern, scale_factor", [(128, 1.3), + (129, 1.3), + (512, 2.41), + (511, 2.41)]) + def test_rescale_produces_odd_size_kernel(self, nkern, scale_factor): + psf = PSF() + psf.kernel = basic_kernel(n=nkern) + outkern = _rescale_kernel(psf.kernel, scale_factor) + n_y, n_x = outkern.shape + assert n_y % 2 == 1 + assert n_x % 2 == 1 class TestRotationBlur: - @pytest.mark.parametrize("angle", ([1, 5, 15, 60])) + @pytest.mark.parametrize("angle", ([1, 5, 15, 60]*u.deg)) def test_returns_rotated_kernel_array_has_same_sum(self, angle): # Without blur implane = basic_image_plane() @@ -157,7 +170,7 @@ def test_convolves_with_3D_cube(self): plt.subplot(231) plt.imshow(implane.data[1, :, :]) - psf = PSF(rotational_blur_angle=15, bkg_width=5, rounded_edges=False) + psf = PSF(rotational_blur_angle=15*u.deg, bkg_width=5, rounded_edges=False) psf.kernel = basic_kernel(n=63) implane = psf.apply_to(implane) diff --git a/scopesim/tests/tests_effects/test_PupilTransmission.py b/scopesim/tests/tests_effects/test_PupilTransmission.py index 652ed2e1..bfd83f9b 100644 --- a/scopesim/tests/tests_effects/test_PupilTransmission.py +++ b/scopesim/tests/tests_effects/test_PupilTransmission.py @@ -1,5 +1,7 @@ -import pytest +"""Tests for PupilTransmission""" + from unittest.mock import patch +import pytest from astropy import units as u @@ -8,7 +10,7 @@ from scopesim.effects.ter_curves import TERCurve from scopesim.effects.ter_curves import PupilTransmission -# pylint: disable=no-self-use, missing-class-docstring +# pylint: disable=missing-class-docstring # pylint: disable=missing-function-docstring THROUGHPUT = 0.764 # random value @@ -35,7 +37,9 @@ def test_has_correct_throughput(self, pupilmask): def test_has_zero_emission(self, pupilmask): assert pupilmask.emission(3.5 * u.um) == 0 * PHOTLAM - def test_update_transmission_works(self, pupilmask): + @pytest.mark.parametrize("newtrans", (0., 0.5)) + def test_update_transmission_works(self, pupilmask, newtrans): assert pupilmask.throughput(3.5 * u.um) == THROUGHPUT - pupilmask.update_transmission(0.5) - assert pupilmask.throughput(3.5 * u.um) == 0.5 + pupilmask.update_transmission(newtrans) + assert pupilmask.throughput(3.5 * u.um) == newtrans + assert pupilmask.emission(3.5 * u.um).unit == PHOTLAM diff --git a/scopesim/tests/tests_effects/test_illumination.py b/scopesim/tests/tests_effects/test_illumination.py new file mode 100644 index 00000000..e8156741 --- /dev/null +++ b/scopesim/tests/tests_effects/test_illumination.py @@ -0,0 +1,75 @@ +"""Tests for illumination effects""" +import pytest +import numpy as np + +from scopesim.effects.illumination import Illumination, gaussian2d, quadratic_vignetting +from scopesim.optics.image_plane import ImagePlane +from scopesim.tests.mocks.py_objects.imagehdu_objects import _image_hdu_square + +PLOTS = False + + +@pytest.fixture +def imageplane(): + ip = ImagePlane(_image_hdu_square().header) + ip.hdu.data = np.ones((100, 100), dtype=np.float64) + return ip + + +# --- gaussian2d --- + +def test_gaussian2d_peak_at_centre(): + result = np.asarray(gaussian2d((100, 100))) + assert result.max() == pytest.approx(1.0) + + + +def test_gaussian2d_values_leq_amp(): + result = gaussian2d((101, 101)) + assert result.max() <= 1.0 + 1e-12 + + +# --- quadratic_vignetting --- + +def test_quadratic_vignetting_centre_is_one(): + result = quadratic_vignetting((101, 101)) + assert result[50, 50] == pytest.approx(1.0) + +def test_quadratic_vignetting_values_in_range(): + result = quadratic_vignetting((101, 101)) + assert np.all(result >= 0.0) and np.all(result <= 1.0) + + +# --- Illumination --- + +def test_illumination_instantiates(): + assert isinstance(Illumination(), Illumination) + +def test_illumination_apply_to_returns_imageplane(imageplane): + eff = Illumination() + assert eff.apply_to(imageplane) is imageplane + +def test_illumination_apply_to_skips_non_imageplane(): + eff = Illumination() + obj = object() + assert eff.apply_to(obj) is obj + +def test_illumination_modifies_data(imageplane): + original = imageplane.hdu.data.copy() + Illumination().apply_to(imageplane) + assert not np.array_equal(imageplane.hdu.data, original) + +def test_illumination_caches_map(imageplane): + eff = Illumination() + eff.apply_to(imageplane) + assert eff._map is not None and eff._map_shape == (100, 100) + +def test_illumination_make_map_shape_and_dtype(): + eff = Illumination() + m = eff._make_map((80, 60)) + assert m.shape == (80, 60) and m.dtype == np.float32 + +def test_illumination_plot_raises_before_apply(): + with pytest.raises(RuntimeError): + Illumination().plot() + diff --git a/scopesim/tests/tests_effects/test_prnu.py b/scopesim/tests/tests_effects/test_prnu.py new file mode 100644 index 00000000..2c7bbcbd --- /dev/null +++ b/scopesim/tests/tests_effects/test_prnu.py @@ -0,0 +1,73 @@ +from matplotlib import pyplot as plt +import numpy as np +import pytest + +from scopesim.detector import Detector +from scopesim.effects.electronic import PixelResponseNonUniformity +from scopesim.optics.image_plane_utils import header_from_list_of_xy + +PLOTS = False + +def make_detector(value=1000, size=10): + hdr = header_from_list_of_xy([-size/2, size/2], [-size/2, size/2], 1, "D") + dtcr = Detector(hdr) + dtcr._hdu.data[:] = value + return dtcr + + +class TestApplyTo: + def test_output_std_matches_prnu_std(self): + """Relative std of output should be close to prnu_std.""" + prnu_std = 0.05 + dtcr = make_detector(value=1000, size=100) + PixelResponseNonUniformity(prnu_std=prnu_std, prnu_seed=42).apply_to(dtcr) + rel_std = dtcr._hdu.data.std() / dtcr._hdu.data.mean() + assert abs(rel_std - prnu_std) < 0.01 + + def test_gain_map_is_reused(self): + """Same map should be applied on repeated calls (fixed pattern).""" + dtcr1 = make_detector() + dtcr2 = make_detector() + prnu = PixelResponseNonUniformity(prnu_std=0.01, prnu_seed=42) + prnu.apply_to(dtcr1) + prnu.apply_to(dtcr2) + np.testing.assert_array_equal(dtcr1._hdu.data, dtcr2._hdu.data) + + def test_dict_prnu_std(self): + """Dict mode: different amplitude per detector ID.""" + hdr = header_from_list_of_xy([-5, 5], [-5, 5], 1, "D") + dtcr = Detector(hdr) + dtcr.meta["id"] = "H2RG" + dtcr._hdu.data[:] = 1000 + prnu = PixelResponseNonUniformity( + prnu_std={"H2RG": 0.005, "GeoSnap": 0.020}, prnu_seed=42) + prnu.apply_to(dtcr) + assert dtcr._hdu.data.std() > 0 + + def test_multiplicative_zero_signal(self): + """Zero signal should remain zero — confirms multiplicative (not additive).""" + dtcr = make_detector(value=0) + PixelResponseNonUniformity(prnu_std=0.01, prnu_seed=42).apply_to(dtcr) + assert dtcr._hdu.data.sum() == 0 + + def test_non_detector_passthrough(self): + """Non-Detector objects should be returned unchanged.""" + prnu = PixelResponseNonUniformity(prnu_std=0.01) + result = prnu.apply_to("not a detector") + assert result == "not a detector" + + def test_invalid_prnu_std_raises(self): + prnu = PixelResponseNonUniformity(prnu_std="not a number nor a dict") + with pytest.raises(TypeError): + prnu.apply_to(make_detector()) + + def test_plot_raises_before_simulation(self): + prnu = PixelResponseNonUniformity(prnu_std=0.01) + with pytest.raises(RuntimeError): + prnu.plot() + + def test_plot_returns_figure(self): + prnu = PixelResponseNonUniformity(prnu_std=0.01, prnu_seed=42) + prnu.apply_to(make_detector()) + if PLOTS: + assert isinstance(prnu.plot(), plt.Figure) diff --git a/scopesim/tests/tests_server/test_database.py b/scopesim/tests/tests_server/test_database.py index 3c25174f..efb6858f 100644 --- a/scopesim/tests/tests_server/test_database.py +++ b/scopesim/tests/tests_server/test_database.py @@ -13,7 +13,7 @@ @pytest.fixture(scope="class") def mock_client(): - # TODO: investigate proper mocking via httpx + # TODO: investigate proper mocking via httpxyz with db.create_client(db.get_base_url()) as client: yield client diff --git a/scopesim/utils.py b/scopesim/utils.py index e9fc748f..c8db463d 100644 --- a/scopesim/utils.py +++ b/scopesim/utils.py @@ -30,6 +30,9 @@ logger = get_logger(__name__) bug_logger = get_logger("bug_report") +class ScopesimPendingDeprecationWarning(PendingDeprecationWarning): + """A scopesim-specific subclass of PendingDeprecationWarning""" + def parallactic_angle(ha, de, lat=-24.589167): r"""