How to Install and Uninstall swarp Package on Ubuntu 21.10 (Impish Indri)

Last updated: December 24,2024

1. Install "swarp" package

Please follow the guidelines below to install swarp on Ubuntu 21.10 (Impish Indri)

$ sudo apt update $ sudo apt install swarp

2. Uninstall "swarp" package

This is a short guide on how to uninstall swarp on Ubuntu 21.10 (Impish Indri):

$ sudo apt remove swarp $ sudo apt autoclean && sudo apt autoremove

3. Information about the swarp package on Ubuntu 21.10 (Impish Indri)

Package: swarp
Architecture: amd64
Version: 2.41.4-2
Priority: optional
Section: universe/science
Origin: Ubuntu
Maintainer: Ubuntu Developers
Original-Maintainer: Debian Astronomy Maintainers
Bugs: https://bugs.launchpad.net/ubuntu/+filebug
Installed-Size: 494
Depends: libc6 (>= 2.29), libcfitsio9 (>= 3.480~)
Filename: pool/universe/s/swarp/swarp_2.41.4-2_amd64.deb
Size: 159396
MD5sum: 93bc5321df77461ac9ddb80899350ea0
SHA1: 383d543364aecc911e2e5ba262edf1dc2935eb91
SHA256: 44215e249e011324319ba03de80042ced7c74cf8bb003fd65280e8d36a1717b0
SHA512: 0a910d8c5b580d3fc3c6c6ba7318058da397821212c85c7594ad8d3e3f1587f833d3d4fbeb745c7d01c22cef2ebaf2f4ce53b07cc593b073d9313566730cc202
Homepage: https://www.astromatic.net/software/swarp
Description-en: 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.
Description-md5: 131adc05cd3745d738a183ebc92e1137