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%global _empty_manifest_terminate_build 0
Name: python-ztv
Version: 0.2.3.post4
Release: 1
Summary: Simple python image viewer, largely intended for astronomical applications
License: MIT License
URL: https://github.com/henryroe/ztv
Source0: https://mirrors.aliyun.com/pypi/web/packages/56/30/65674e2ea9b18388e75d019ec353d59db95d94f5fdff0f90f231431b8961/ztv-0.2.3.post4.tar.gz
BuildArch: noarch
Requires: python3-astropy
Requires: python3-astropy-helpers
Requires: python3-matplotlib
Requires: python3-psutil
Requires: python3-wxPython
%description
*ztv* is an astronomical image viewer designed to be used from a python
command line for display and analysis.
*ztv* is useful as-is for display and simple analysis of images already
loaded in to `numpy arrays <http://www.numpy.org>`__, as well as `FITS
files <http://fits.gsfc.nasa.gov/fits_primer.html>`__. It can display
the most recently acquired image by watching a directory for new FITS
files to appear or watching a single FITS file for when it changes. It
can also receive new images via an `ActiveMQ message
stream <http://activemq.apache.org>`__.
*ztv* is intended for real-time display and analysis. *ztv* is not
intended to produce publication quality figures.
*ztv* comes with a number of built-in control panels, for: - selecting
input source (FITS file, auto-reload from FITS file, etc) - selecting a
frame to subtract (e.g. sky or dark) and a flat field frame to divide by
- setting colormap, stretch, and lower/upper limits - doing basic slice
plots, statistics, and aperture photometry. Additional panels can be
written and added, for e.g. controlling a camera. (One example add-on
panel is included that generates faked images in the FITS format.)
If proper FITS header keywords are available, *ztv* will display the
ra/dec of the cursor point.
%package -n python3-ztv
Summary: Simple python image viewer, largely intended for astronomical applications
Provides: python-ztv
BuildRequires: python3-devel
BuildRequires: python3-setuptools
BuildRequires: python3-pip
%description -n python3-ztv
*ztv* is an astronomical image viewer designed to be used from a python
command line for display and analysis.
*ztv* is useful as-is for display and simple analysis of images already
loaded in to `numpy arrays <http://www.numpy.org>`__, as well as `FITS
files <http://fits.gsfc.nasa.gov/fits_primer.html>`__. It can display
the most recently acquired image by watching a directory for new FITS
files to appear or watching a single FITS file for when it changes. It
can also receive new images via an `ActiveMQ message
stream <http://activemq.apache.org>`__.
*ztv* is intended for real-time display and analysis. *ztv* is not
intended to produce publication quality figures.
*ztv* comes with a number of built-in control panels, for: - selecting
input source (FITS file, auto-reload from FITS file, etc) - selecting a
frame to subtract (e.g. sky or dark) and a flat field frame to divide by
- setting colormap, stretch, and lower/upper limits - doing basic slice
plots, statistics, and aperture photometry. Additional panels can be
written and added, for e.g. controlling a camera. (One example add-on
panel is included that generates faked images in the FITS format.)
If proper FITS header keywords are available, *ztv* will display the
ra/dec of the cursor point.
%package help
Summary: Development documents and examples for ztv
Provides: python3-ztv-doc
%description help
*ztv* is an astronomical image viewer designed to be used from a python
command line for display and analysis.
*ztv* is useful as-is for display and simple analysis of images already
loaded in to `numpy arrays <http://www.numpy.org>`__, as well as `FITS
files <http://fits.gsfc.nasa.gov/fits_primer.html>`__. It can display
the most recently acquired image by watching a directory for new FITS
files to appear or watching a single FITS file for when it changes. It
can also receive new images via an `ActiveMQ message
stream <http://activemq.apache.org>`__.
*ztv* is intended for real-time display and analysis. *ztv* is not
intended to produce publication quality figures.
*ztv* comes with a number of built-in control panels, for: - selecting
input source (FITS file, auto-reload from FITS file, etc) - selecting a
frame to subtract (e.g. sky or dark) and a flat field frame to divide by
- setting colormap, stretch, and lower/upper limits - doing basic slice
plots, statistics, and aperture photometry. Additional panels can be
written and added, for e.g. controlling a camera. (One example add-on
panel is included that generates faked images in the FITS format.)
If proper FITS header keywords are available, *ztv* will display the
ra/dec of the cursor point.
%prep
%autosetup -n ztv-0.2.3.post4
%build
%py3_build
%install
%py3_install
install -d -m755 %{buildroot}/%{_pkgdocdir}
if [ -d doc ]; then cp -arf doc %{buildroot}/%{_pkgdocdir}; fi
if [ -d docs ]; then cp -arf docs %{buildroot}/%{_pkgdocdir}; fi
if [ -d example ]; then cp -arf example %{buildroot}/%{_pkgdocdir}; fi
if [ -d examples ]; then cp -arf examples %{buildroot}/%{_pkgdocdir}; fi
pushd %{buildroot}
if [ -d usr/lib ]; then
find usr/lib -type f -printf "\"/%h/%f\"\n" >> filelist.lst
fi
if [ -d usr/lib64 ]; then
find usr/lib64 -type f -printf "\"/%h/%f\"\n" >> filelist.lst
fi
if [ -d usr/bin ]; then
find usr/bin -type f -printf "\"/%h/%f\"\n" >> filelist.lst
fi
if [ -d usr/sbin ]; then
find usr/sbin -type f -printf "\"/%h/%f\"\n" >> filelist.lst
fi
touch doclist.lst
if [ -d usr/share/man ]; then
find usr/share/man -type f -printf "\"/%h/%f.gz\"\n" >> doclist.lst
fi
popd
mv %{buildroot}/filelist.lst .
mv %{buildroot}/doclist.lst .
%files -n python3-ztv -f filelist.lst
%dir %{python3_sitelib}/*
%files help -f doclist.lst
%{_docdir}/*
%changelog
* Tue Jun 20 2023 Python_Bot <Python_Bot@openeuler.org> - 0.2.3.post4-1
- Package Spec generated
|
