Binary package “wsclean-dev” in ubuntu mantic
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.
Source package
Published versions
- wsclean-dev 3.1-3 in amd64 (Release)
- wsclean-dev 3.1-4 in amd64 (Proposed)
- wsclean-dev 3.1-4 in amd64 (Release)
- wsclean-dev 3.1-3 in arm64 (Release)
- wsclean-dev 3.1-4 in arm64 (Proposed)
- wsclean-dev 3.1-4 in arm64 (Release)
- wsclean-dev 3.1-3 in armhf (Release)
- wsclean-dev 3.1-4 in armhf (Proposed)
- wsclean-dev 3.1-4 in armhf (Release)
- wsclean-dev 3.1-3 in ppc64el (Release)
- wsclean-dev 3.1-4 in ppc64el (Proposed)
- wsclean-dev 3.1-4 in ppc64el (Release)
- wsclean-dev 3.1-3 in riscv64 (Release)
- wsclean-dev 3.1-4 in riscv64 (Proposed)
- wsclean-dev 3.1-4 in riscv64 (Release)
- wsclean-dev 3.1-3 in s390x (Release)
- wsclean-dev 3.1-4 in s390x (Proposed)
- wsclean-dev 3.1-4 in s390x (Release)