swarp 2.41.2-1build1 source package in Ubuntu


swarp (2.41.2-1build1) groovy; urgency=medium

  * No change rebuild against new cfitsio ABI.

 -- Dimitri John Ledkov <email address hidden>  Thu, 27 Aug 2020 23:46:35 +0100

Upload details

Uploaded by:
Dimitri John Ledkov
Uploaded to:
Original maintainer:
Ubuntu Developers
Medium Urgency

See full publishing history Publishing

Series Pocket Published Component Section
Groovy release universe misc


File Size SHA-256 Checksum
swarp_2.41.2.orig.tar.gz 433.3 KiB 618c079eb2a1ddc1bad472cea36706ae8b9cca13b03e7f7da8a49ff7b6018f05
swarp_2.41.2-1build1.debian.tar.xz 6.8 KiB f5e536db9ecd9efc8d4974db6a6a80e80e4334c5c5ff0de48e75de300ae38048
swarp_2.41.2-1build1.dsc 2.0 KiB 09f48373267c4a1374c96b1a49e59f3906179bf8767b9fcbe7089f468ab6f89c

View changes file

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
  * 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
  * Selectable high-order interpolation method (up to 8-tap filters) in any
  * 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
  * XML VOTable-compliant output of meta-data.

swarp-dbgsym: debug symbols for swarp