Package: wsclean
Version: 3.6-2
Architecture: arm64
Maintainer: Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
Original-Maintainer: Debian Astro Team <debian-astro-maintainers@lists.alioth.debian.org>
Installed-Size: 15639
Depends: libboost-filesystem1.88.0 (>= 1.88.0), libc6 (>= 2.38), libcasa-casa8 (>= 3.7.1), libcasa-fits8 (>= 3.7.1), libcasa-measures8 (>= 3.7.1), libcasa-ms8 (>= 3.7.1), libcasa-tables8 (>= 3.7.1), libcfitsio10t64 (>= 4.2.0~), libfftw3-double3 (>= 3.3.10), libfftw3-single3 (>= 3.3.10), libgcc-s1 (>= 4.2), libgsl28 (>= 2.8+dfsg), libhdf5-310 (>= 1.14.3), libhdf5-cpp-310 (>= 1.14.4.3), liblapack3 | liblapack.so.3, libpython3.13 (>= 3.13.0~rc3), libstdc++6 (>= 14)
Suggests: wsclean-dev
Section: science
Priority: optional
Homepage: https://gitlab.com/aroffringa/wsclean/
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).
