Ubuntu
swarp package

swarp 2.38.0+dfsg-2 source package in Ubuntu

Changelog

swarp (2.38.0+dfsg-2) unstable; urgency=low

  * Replace the build date with the last changed date of configure.ac
  * Unify debian/copyright with other astromatic packages

 -- Ole Streicher <email address hidden>  Sat, 30 May 2015 09:53:14 +0200

Upload details

Uploaded by:
Debian Astronomy Maintainers
Uploaded to:
Sid
Original maintainer:
Debian Astronomy Maintainers
Architectures:
any
Section:
misc
Urgency:
Low Urgency

See full publishing history Publishing

Series Pocket Published Component Section

Downloads

File Size SHA-256 Checksum
swarp_2.38.0+dfsg-2.dsc 1.9 KiB d348a235e883d81e1d9ac40b60679bd6596bd4ec288e5085c193c4f11c8ecc75
swarp_2.38.0+dfsg.orig.tar.gz 603.1 KiB 779aece5f5b9f3cac1ad79b3fdf7458c13cfb4e3961e6c2e18e8f04befb46634
swarp_2.38.0+dfsg-2.debian.tar.xz 4.4 KiB 584af90f414007465cf790920bbce9d954616521eb7ff45113ba94f8537df00e

Available diffs

No changes file available.

Binary packages built by this source

swarp: 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.

swarp-dbgsym: debug symbols for package swarp

 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.