Package: python3-bdsf
Source: pybdsf
Version: 1.10.1-1
Architecture: amd64
Maintainer: Ubuntu Developers <ubuntu-devel-discuss@lists.ubuntu.com>
Original-Maintainer: Debian Astro Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
Installed-Size: 1395
Depends: libboost-numpy1.74.0 (>= 1.74.0), libboost-python1.74.0 (>= 1.74.0), libc6 (>= 2.32), libgcc-s1 (>= 3.3.1), libgfortran5 (>= 8), libstdc++6 (>= 5.2), python3-numpy (>= 1:1.20.0), python3-numpy-abi9, python3 (<< 3.11), python3 (>= 3.10~), python3-astropy, python3-scipy, python3:any
Section: python
Priority: optional
Homepage: https://www.astron.nl/citt/pybdsf/
Description: Python Blob Detection and Source Finder
 PyBDSF (the Python Blob Detection and Source Finder) is a tool
 designed to decompose radio interferometry images into sources and
 make available their properties for further use. PyBDSF can decompose
 an image into a set of Gaussians, shapelets, or wavelets as well as
 calculate spectral indices and polarization properties of sources and
 measure the psf variation across an image. PyBDSF uses an interactive
 environment based on CASA that will be familiar to most radio
 astronomers.  Additionally, PyBDSF may also be used in Python
 scripts.
