wsclean 2.8-1 source package in Ubuntu

Changelog

wsclean (2.8-1) unstable; urgency=low

  * New upstream version 2.8. Rediff patches
  * Add gitlab-ci.yml for salsa

 -- Ole Streicher <email address hidden>  Fri, 20 Sep 2019 11:20:08 +0200

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Uploaded by:
Debian Astronomy Maintainers
Uploaded to:
Sid
Original maintainer:
Debian Astronomy Maintainers
Architectures:
any
Section:
misc
Urgency:
Low Urgency

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File Size SHA-256 Checksum
wsclean_2.8-1.dsc 2.2 KiB b44f4d5b21d25fd0d6711d9b0fead928462fd14c7ee5d785fe32208ddead6959
wsclean_2.8.orig.tar.bz2 278.9 KiB 30c7b1ba31e88b85266206e17d95987c2b24d7849c572c3c8c7c86fd1396a729
wsclean_2.8-1.debian.tar.xz 10.7 KiB c9fc9a4de57b19cfd614812f6b96b7c9fdd983f4f14d6a28619b48729fbb91eb

Available diffs

No changes file available.

Binary packages built by this source

libwsclean2: 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.

libwsclean2-dbgsym: debug symbols for libwsclean2
wsclean: 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).

wsclean-dbgsym: debug symbols for wsclean
wsclean-dev: 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.