Date: Sun, 22 Sep 2024 05:51:25 GMT From: Yuri Victorovich <yuri@FreeBSD.org> To: ports-committers@FreeBSD.org, dev-commits-ports-all@FreeBSD.org, dev-commits-ports-main@FreeBSD.org Subject: git: 680659e894bc - main - science/py-pyphot: New port: Library for computing photometry from spectra Message-ID: <202409220551.48M5pPSo022081@gitrepo.freebsd.org>
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The branch main has been updated by yuri: URL: https://cgit.FreeBSD.org/ports/commit/?id=680659e894bca358d011c66bdba3b770b78d0896 commit 680659e894bca358d011c66bdba3b770b78d0896 Author: Yuri Victorovich <yuri@FreeBSD.org> AuthorDate: 2024-09-22 04:11:53 +0000 Commit: Yuri Victorovich <yuri@FreeBSD.org> CommitDate: 2024-09-22 05:51:20 +0000 science/py-pyphot: New port: Library for computing photometry from spectra --- science/Makefile | 1 + science/py-pyphot/Makefile | 27 +++++++++++++++++++++++++++ science/py-pyphot/distinfo | 3 +++ science/py-pyphot/pkg-descr | 13 +++++++++++++ 4 files changed, 44 insertions(+) diff --git a/science/Makefile b/science/Makefile index 195da3c9f7c4..377a3db7e439 100644 --- a/science/Makefile +++ b/science/Makefile @@ -409,6 +409,7 @@ SUBDIR += py-pymbd SUBDIR += py-pymol SUBDIR += py-pyosf + SUBDIR += py-pyphot SUBDIR += py-pyprecice SUBDIR += py-pyqubo SUBDIR += py-pysal diff --git a/science/py-pyphot/Makefile b/science/py-pyphot/Makefile new file mode 100644 index 000000000000..341f86eac817 --- /dev/null +++ b/science/py-pyphot/Makefile @@ -0,0 +1,27 @@ +PORTNAME= pyphot +DISTVERSION= 1.4.7 +CATEGORIES= science +MASTER_SITES= PYPI +PKGNAMEPREFIX= ${PYTHON_PKGNAMEPREFIX} + +MAINTAINER= yuri@FreeBSD.org +COMMENT= Library for computing photometry from spectra +WWW= https://mfouesneau.github.io/pyphot/ + +LICENSE= MIT +LICENSE_FILE= ${WRKSRC}/LICENSE + +BUILD_DEPENDS= ${PY_SETUPTOOLS} +RUN_DEPENDS= ${PYTHON_PKGNAMEPREFIX}astropy>0:astro/py-astropy@${PY_FLAVOR} \ + ${PYTHON_PKGNAMEPREFIX}matplotlib>0:math/py-matplotlib@${PY_FLAVOR} \ + ${PYTHON_PKGNAMEPREFIX}numpy>=2.0:math/py-numpy@${PY_FLAVOR} \ + ${PYTHON_PKGNAMEPREFIX}pandas>0:math/py-pandas@${PY_FLAVOR} \ + ${PYTHON_PKGNAMEPREFIX}scipy>0:science/py-scipy@${PY_FLAVOR} \ + ${PYTHON_PKGNAMEPREFIX}tables>0:devel/py-tables@${PY_FLAVOR} + +USES= python +USE_PYTHON= distutils autoplist pytest + +NO_ARCH= yes + +.include <bsd.port.mk> diff --git a/science/py-pyphot/distinfo b/science/py-pyphot/distinfo new file mode 100644 index 000000000000..eb2396349fd3 --- /dev/null +++ b/science/py-pyphot/distinfo @@ -0,0 +1,3 @@ +TIMESTAMP = 1726947143 +SHA256 (pyphot-1.4.7.tar.gz) = 001ebeb7741e81bf864b0240ecf32eed9c613e79ab06d2274042d7669f754df6 +SIZE (pyphot-1.4.7.tar.gz) = 14971120 diff --git a/science/py-pyphot/pkg-descr b/science/py-pyphot/pkg-descr new file mode 100644 index 000000000000..e52d54b01669 --- /dev/null +++ b/science/py-pyphot/pkg-descr @@ -0,0 +1,13 @@ +PYPHOT is a set of tools to compute synthetic photometry in a simple way, ideal +to integrate in larger projects. + +The inputs are photonic or energetic response functions for the desired +photometric bands and stellar spectra. The modules are flexible to handle units +in the wavelength definition through a simplified version of pint. + +Filters are represented individually by a Filter object. Collections of filters +are handled with a Library. We provide an internal library that contains a +signitificant amount of common filters. + +Each filter is minimally defined by a wavelength and throughput. Many properties +such as central of pivot wavelength are computed internally.
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