1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
|
Source: pybdsf
Maintainer: Debian Astro Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
Uploaders: Ole Streicher <olebole@debian.org>
Section: python
Priority: optional
Build-Depends: debhelper-compat (= 13),
dh-python,
meson,
pybuild-plugin-pyproject,
python3-all-dev,
python3-astropy,
python3-setuptools,
python3-setuptools-scm,
python3-numpy,
python3-numpy-dev,
python3-scipy,
python3-skbuild,
libboost-python-dev,
libboost-numpy-dev,
gfortran
Standards-Version: 4.7.2
Vcs-Browser: https://salsa.debian.org/debian-astro-team/pybdsf
Vcs-Git: https://salsa.debian.org/debian-astro-team/pybdsf.git
Homepage: https://pybdsf.readthedocs.io/
Package: python3-bdsf
Architecture: any
Depends: ${shlibs:Depends},
${python3:Depends},
${misc:Depends},
python3-astropy
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.
|
