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
|
Source: swarp
Section: science
Priority: optional
Maintainer: Debian Astronomy Maintainers <debian-astro-maintainers@lists.alioth.debian.org>
Uploaders: Ole Streicher <olebole@debian.org>
Build-Depends: debhelper (>= 9), dh-autoreconf
Standards-Version: 3.9.7
Homepage: http://www.astromatic.net/software/swarp
Vcs-Git: git://anonscm.debian.org/debian-astro/packages/swarp.git
Vcs-Browser: https://anonscm.debian.org/gitweb/?p=debian-astro/packages/swarp.git
Package: swarp
Architecture: any
Depends: ${misc:Depends}, ${shlibs:Depends}
Description: Resample and co-add together FITS images
Resample and co-add together FITS images using any arbitrary astrometric
projection defined in the WCS standard. The main features of SWarp
are:
.
* FITS format (including multi-extensions) in input and output,
* Full handling of weight-maps in input and output,
* Ability to work with very large images (up to 500 Mpixels on
32-bit machines and 10^6 Tpixels with 64-bits), thanks to customized
virtual-memory-mapping and buffering,
* Works with arrays in up to 9 dimensions (including or not two spherical
coordinates),
* Selectable high-order interpolation method (up to 8-tap filters) in any
dimension,
* Compatible with WCS and TNX (IRAF) astrometric descriptions,
* Support for equatorial, galactic and equatorial coordinate systems,
* Astrometric and photometric parameters are read from FITS headers or
external ASCIIfiles,
* Built-in background subtraction,
* Built-in noise-level measurement for automatic weighting,
* Automatic centering and sizing functions of the output field,
* Multi-threaded code with load-balancing to take advantageof multiple
processors.
* XML VOTable-compliant output of meta-data.
|
