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 | Published | Component | Section | |
---|---|---|---|---|
Oracular | release | universe | misc |
Downloads
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.