wsclean 2.8-1 source package in Ubuntu
Changelog
wsclean (2.8-1) unstable; urgency=low * New upstream version 2.8. Rediff patches * Add gitlab-ci.yml for salsa -- Ole Streicher <email address hidden> Fri, 20 Sep 2019 11:20:08 +0200
Upload details
- Uploaded by:
- Debian Astronomy Maintainers
- Uploaded to:
- Sid
- Original maintainer:
- Debian Astronomy Maintainers
- Architectures:
- any
- Section:
- misc
- Urgency:
- Low Urgency
See full publishing history Publishing
Series | Published | Component | Section |
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Downloads
File | Size | SHA-256 Checksum |
---|---|---|
wsclean_2.8-1.dsc | 2.2 KiB | b44f4d5b21d25fd0d6711d9b0fead928462fd14c7ee5d785fe32208ddead6959 |
wsclean_2.8.orig.tar.bz2 | 278.9 KiB | 30c7b1ba31e88b85266206e17d95987c2b24d7849c572c3c8c7c86fd1396a729 |
wsclean_2.8-1.debian.tar.xz | 10.7 KiB | c9fc9a4de57b19cfd614812f6b96b7c9fdd983f4f14d6a28619b48729fbb91eb |
Available diffs
- diff from 2.7-1build1 (in Ubuntu) to 2.8-1 (52.8 KiB)
No changes file available.
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.