wsclean 2.9-2build1 source package in Ubuntu

Changelog

wsclean (2.9-2build1) groovy; urgency=medium

  * No-change rebuild against libgsl25

 -- Graham Inggs <email address hidden>  Thu, 07 May 2020 21:39:51 +0000

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Uploaded by:
Graham Inggs
Uploaded to:
Groovy
Original maintainer:
Debian Astronomy Maintainers
Architectures:
any
Section:
misc
Urgency:
Medium Urgency

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Series Pocket Published Component Section

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File Size SHA-256 Checksum
wsclean_2.9.orig.tar.bz2 305.9 KiB d3e6d2de3cb923f5fa37638977c58bbe56a9db79ac2523ef0d0dbb3c1afe065d
wsclean_2.9-2build1.debian.tar.xz 10.8 KiB 45e4731ca831043346f058a12bb143d97255071441512c8c2bce4283691437e6
wsclean_2.9-2build1.dsc 2.2 KiB de63175d43f20f2eddc124a3c0189f9fbf1d141a16386cc062c63b9e8cc54e23

Available diffs

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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.