File: control

package info (click to toggle)
gwcs 0.10.0-2
  • links: PTS, VCS
  • area: main
  • in suites: buster
  • size: 1,220 kB
  • sloc: python: 6,621; makefile: 125; ansic: 88
file content (50 lines) | stat: -rw-r--r-- 1,896 bytes parent folder | download
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
42
43
44
45
46
47
48
49
50
Source: gwcs
Section: python
Priority: optional
Maintainer: Debian Astro Team <debian-astro-maintainers@lists.alioth.debian.org>
Uploaders: Miguel de Val-Borro <miguel@archlinux.net>
Build-Depends: cython3,
               debhelper (>= 11),
               dh-python,
               libjs-jquery,
               libjs-underscore,
               python3-all,
               python3-asdf,
               python3-astropy (>= 3.1),
               python3-astropy-helpers,
               python3-pytest,
               python3-scipy,
               python3-setuptools,
               python3-sphinx
Standards-Version: 4.3.0
Homepage: https://gwcs.readthedocs.io
Vcs-Git: https://salsa.debian.org/debian-astro-team/gwcs.git
Vcs-Browser: https://salsa.debian.org/debian-astro-team/gwcs

Package: python3-gwcs
Architecture: all
Depends: ${misc:Depends},
         ${python3:Depends}
Description: Tools for managing the WCS of astronomical data (Python 3)
 GWCS takes a general approach to WCS. It supports a data model which includes
 the entire transformation pipeline from input coordinates (detector by
 default) to world coordinates.  The goal is to provide a flexible toolkit
 which is easily extendible by adding new transforms and frames.
 .
 This package contains the Python 3 version of the package.

Package: python-gwcs-doc
Architecture: all
Multi-Arch: foreign
Section: doc
Depends: libjs-jquery,
         libjs-underscore,
         ${misc:Depends},
         ${sphinxdoc:Depends}
Description: Tools for managing the WCS of astronomical data (documentation)
 GWCS takes a general approach to WCS. It supports a data model which includes
 the entire transformation pipeline from input coordinates (detector by
 default) to world coordinates.  The goal is to provide a flexible toolkit
 which is easily extendible by adding new transforms and frames.
 .
 This is the common documentation package.