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wsclean 2.10.1-1
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Source: wsclean
Section: science
Priority: optional
Maintainer: Debian Astro Team <debian-astro-maintainers@lists.alioth.debian.org>
Uploaders: Gijs Molenaar <gijs@pythonic.nl>,
           Ole Streicher <olebole@debian.org>
Build-Depends: casacore-dev,
               cmake,
               debhelper-compat (= 13),
               libboost-dev,
               libboost-filesystem-dev,
               libboost-program-options-dev,
               libboost-system-dev,
               libboost-thread-dev,
               libcfitsio-dev | libcfitsio3-dev,
               libfftw3-dev,
               libgsl0-dev,
               libhdf5-dev
Standards-Version: 4.5.0
Vcs-Git: https://salsa.debian.org/debian-astro-team/wsclean.git
Vcs-Browser: https://salsa.debian.org/debian-astro-team/wsclean
Homepage: https://sourceforge.net/projects/wsclean/
Rules-Requires-Root: no

Package: wsclean
Architecture: any
Depends: ${misc:Depends}, ${shlibs:Depends}
Suggests: wsclean-dev
Description: Fast generic widefield interferometric imager
 WSClean (w-stacking clean) is a fast generic widefield imager. It uses the
 w-stacking algorithm and can make use of the w-snapshot algorithm. As of
 Feb 2014, it is 2-12 times faster than CASA's w-projection, depending on the
 array configuration. It supports full-sky imaging and proper beam correction
 for homogeneous dipole arrays such as the MWA.
 .
 WSClean allows Hogbom and Cotton-Schwab cleaning, and can clean polarizations
 joinedly. All operations are performed on the CPU (it is not specialized for
 GPUs).

Package: libwsclean2
Architecture: any
Multi-Arch: same
Section: libs
Depends: ${misc:Depends}, ${shlibs:Depends}
Description: Fast generic widefield interferometric imager (shared library)
 WSClean (w-stacking clean) is a fast generic widefield imager. It uses the
 w-stacking algorithm and can make use of the w-snapshot algorithm. As of
 Feb 2014, it is 2-12 times faster than CASA's w-projection, depending on the
 array configuration. It supports full-sky imaging and proper beam correction
 for homogeneous dipole arrays such as the MWA.
 .
 WSClean allows Hogbom and Cotton-Schwab cleaning, and can clean polarizations
 joinedly. All operations are performed on the CPU (it is not specialized for
 GPUs).
 .
 This package contains the shared library.

Package: wsclean-dev
Architecture: any
Section: libdevel
Depends: libwsclean2 (= ${binary:Version}),${misc:Depends}, ${shlibs:Depends}
Recommends: wsclean
Description: Fast generic widefield interferometric imager (development files)
 WSClean (w-stacking clean) is a fast generic widefield imager. It uses the
 w-stacking algorithm and can make use of the w-snapshot algorithm. As of
 Feb 2014, it is 2-12 times faster than CASA's w-projection, depending on the
 array configuration. It supports full-sky imaging and proper beam correction
 for homogeneous dipole arrays such as the MWA.
 .
 WSClean allows Hogbom and Cotton-Schwab cleaning, and can clean polarizations
 joinedly. All operations are performed on the CPU (it is not specialized for
 GPUs).
 .
 This package contains the static library and the header file to
 compile own programs against the library.