wsclean 3.4-2 source package in Ubuntu

Changelog

wsclean (3.4-2) unstable; urgency=medium

  * Link Radler a static instead of shared library. Closes: #1070237
  * Push Standards-Version to 4.7.0. No changes needed
  * Add superficial autopkgtest

 -- Ole Streicher <email address hidden>  Sat, 18 May 2024 17:35:57 +0200

Upload details

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

See full publishing history Publishing

Series Pocket Published Component Section
Oracular release universe misc

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File Size SHA-256 Checksum
wsclean_3.4-2.dsc 2.2 KiB b61c50b7fc1cda8f57a7c5f1c46b3ae113da832bde3ad7502cea51beac8e7c1d
wsclean_3.4.orig.tar.bz2 2.4 MiB b43d8ca490ccf34dd22aae6c5ca88a5dcb3cff0526835d3f97fa6d239745e641
wsclean_3.4-2.debian.tar.xz 13.5 KiB e0ea6b60e61e92929ef3ded25be5399cd066647be16aac4241f93dbde8fbcfab

Available diffs

No changes file available.

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.