wsclean 3.1-1 source package in Ubuntu

Changelog

wsclean (3.1-1) unstable; urgency=medium

  * New upstream version 3.1
  * Rediff patches
  * Update build dependencies
  * Push Standards-Version to 4.6.1. No changes needed

 -- Ole Streicher <email address hidden>  Tue, 24 May 2022 15:46:46 +0200

Upload details

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

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File Size SHA-256 Checksum
wsclean_3.1-1.dsc 2.2 KiB af8822d0e6c508fe862107244fe78221401b5eb4fb41086afc8bdeab2502d675
wsclean_3.1.orig.tar.bz2 1.4 MiB ecc58bdff1aa428c17c9915e6d8fddd5aa397cb5f0848f224f3e7932aa15fce0
wsclean_3.1-1.debian.tar.xz 10.7 KiB 8aa280753b38bbb93df5053625d0f6d0c13ad429320c34adacd862b2817b6f60

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.