Ubuntu
wsclean package

wsclean 3.1-4 source package in Ubuntu

Changelog

wsclean (3.1-4) unstable; urgency=medium

  * Team upload.
  * Add fix-gcc-13.patch to fix gcc-13 build issues. (Closes: #1037899)

 -- Bo YU <email address hidden>  Wed, 26 Jul 2023 16:43:38 +0800

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
Mantic release universe misc

Downloads

File Size SHA-256 Checksum
wsclean_3.1-4.dsc 2.1 KiB 15b5db78eac13eeed5634ffbf79855d6106bab99567e2db41bfadedebde13e55
wsclean_3.1.orig.tar.bz2 1.4 MiB ecc58bdff1aa428c17c9915e6d8fddd5aa397cb5f0848f224f3e7932aa15fce0
wsclean_3.1-4.debian.tar.xz 12.4 KiB fcad5a5ecd5ee929ddf3da1ad455cfabc83f266a04fc6a7340d9bcac48a18125

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.