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wsclean package

wsclean 3.1-1build1 source package in Ubuntu

Changelog

wsclean (3.1-1build1) kinetic; urgency=medium

  * No-change rebuild against libcasa-casa7

 -- Steve Langasek <email address hidden>  Sat, 16 Jul 2022 17:51:22 +0000

Upload details

Uploaded by:
Steve Langasek
Uploaded to:
Kinetic
Original maintainer:
Ubuntu Developers
Architectures:
any
Section:
misc
Urgency:
Medium Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Kinetic release universe misc

Downloads

File Size SHA-256 Checksum
wsclean_3.1.orig.tar.bz2 1.4 MiB ecc58bdff1aa428c17c9915e6d8fddd5aa397cb5f0848f224f3e7932aa15fce0
wsclean_3.1-1build1.debian.tar.xz 10.8 KiB f80093d4a4be3b1d82be2e1d9a9ab14f99dc2f58439df4dbeccdc5c90e9df037
wsclean_3.1-1build1.dsc 2.3 KiB 23552f702bf98ef2697f965ccd4507252fd38571067f548f20b8df00d6539f30

Available diffs

View changes file

Binary packages built by this source

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.