Ubuntu
wsclean package

wsclean 2.7-1build1 source package in Ubuntu

Changelog

wsclean (2.7-1build1) eoan; urgency=medium

  * No-change rebuild against libcfitsio8

 -- Steve Langasek <email address hidden>  Sun, 04 Aug 2019 05:56:15 +0000

Upload details

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

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Series Pocket Published Component Section

Downloads

File Size SHA-256 Checksum
wsclean_2.7.orig.tar.bz2 273.9 KiB 8307990b7d2bec8e4a52f2cd10c6433c908458bcc4475121e99ec88f824cc2e8
wsclean_2.7-1build1.debian.tar.xz 10.7 KiB 0f606208a2c4277e38af838b413f2e2be0da840d0c4f3dc81ef0f5a434f95a56
wsclean_2.7-1build1.dsc 2.3 KiB ce20572c0d8eb6c549efbde9fcc39a3cc0cb5ac6688b0f47fae30932704cbee4

Available diffs

View changes file

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: No summary available for libwsclean2-dbgsym in ubuntu eoan.

No description available for libwsclean2-dbgsym in ubuntu eoan.

wsclean: No summary available for wsclean in ubuntu eoan.

No description available for wsclean in ubuntu eoan.

wsclean-dbgsym: No summary available for wsclean-dbgsym in ubuntu eoan.

No description available for wsclean-dbgsym in ubuntu eoan.

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.