Debian Astro Development packages

Le paquet casacore fournit les bibliothèques principales de l'ancien paquet AIPS++/CASA (« Common Astronomy Software Applications »). Cette séparation permet de mieux isoler les bibliothèques principales des applications.

Ce paquet fournit les fichiers pour le développement d'applications.

• Debian Astro Team
• Ole Streicher

• 3.6.1-5 (sid)
• 3.0.0-4 (buster)
• 2.2.0-2 (stretch)
• 3.6.1-4 (trixie)
• 3.5.0-2 (bookworm)
• 3.3.0-4 (bullseye)

• 3 regular users
• 12 recent
• 88 total installations (of 250586 submissions)

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Astro::Fits::Cfitsio est une interface Perl à la bibliothèque de sous-routines cfitsio de William Pence. Pour plus d'information sur cfitsio, consultez la page http://heasarc.gsfc.nasa.gov/fitsio.

Ce module tente de fournir une enveloppe pour à peu près chaque routine cfitsio, tout en restant le plus proche possible du comportement de cfitsio. En tant que tel, il faut être conscient qu'il est encore de bas niveau sous certains aspects, dans le sens que passer un tableau qui n'est pas de la taille correcte à une routine comme fits_write_img() peut provoquer une erreur de segmentation.

Le but est d'utiliser ces routines pour bâtir une interface plus proche de Perl pour beaucoup de tâches communes comme l'écriture et l'écriture d'images ou de tableaux ASCII ou binaires.

• Debian Perl Group
• gregor herrmann

• 1.17-1 (bookworm)
• 1.18-1 (trixie)
• 1.18-1 (sid)
• 1.10-1 (jessie)
• 1.11-2 (stretch)
• 1.12-1 (buster)
• 1.15-1 (bullseye)

devel

lang:perl, library

field

astronomy

• 73 total installations (of 250586 submissions)

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• Git

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• Debian Science Team
• Sébastien Villemot

• 3.10.3-1 (stretch)
• 3.10.2-7 (jessie)

devel

library

role

devel-lib

• 2 regular users
• 111 total installations (of 250586 submissions)

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In Debian Stretch, this package is integrated in wcslib-dev.

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FITS (« Flexible Image Transport System », système flexible de transport d'images) est un format de données utilisé en astronomie. cfitsio est une bibliothèque de routines⋅C ANSI pour la lecture et l'écriture des fichiers de données au format FITS. Un jeu de routines en Fortran a été inclus pour la commodité des programmeurs Fortran.

Ce paquet fournit ce qui est nécessaire pour compiler des sources qui utilisent cette bibliothèque dans leur code.

• Debian Astronomy Maintainers
• Aurelien Jarno

• 3.410-1 (stretch)
• 4.5.0-5 (sid)
• 4.5.0-5 (trixie)
• 4.2.0-3 (bookworm)
• 3.490-3 (bullseye)
• 3.450-3 (buster)
• 3.370-2+deb8u1 (jessie)

• 226 regular users
• 220 recent
• 2236 total installations (of 250586 submissions)

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The Common Pipeline Library (CPL) comprises a set of ISO-C libraries that provide a comprehensive, efficient and robust software toolkit. It forms a basis for the creation of automated astronomical data-reduction tasks (known as "pipelines").

The CPL was developed to standardise the way instrument pipelines are built, to shorten their development cycle and to ease their maintenance. However, it may be more generally applied to any similar application, and the details of the CPL code have been engineered in a way to make the library portable and flexible, as well as minimising external dependencies.

The CPL provides a host of functionality, presented in a clear, generic and uniform manner. Among its many features, the CPL offers:

• many useful low-level data types (images, tables, matrices, strings, property lists, ...),
• many fundamental statistic, arithmetic and conversion operations for these data types.
• medium-level data access methods (e.g. a data abstraction layer for FITS files),
• data table organisation and manipulation,
• keyword/value handling and management,
• a standardised application interface for pipeline recipes, and,
• support for dynamic loading of recipe modules.

Despite the current bias towards instrument pipeline development, the library also provides a variety of general-purpose image- and signal-processing functions, making it an excellent framework for the creation of more generic data-handling packages.

This package contains the static library and the C header files.

• K. Banse, P. Ballester, C. Izzo, Y. Jung, L. K. Lundin, D. J. McKay, A. Modigliani, R. M. Palsa, M. Kiesgen and C. Sabet: The Common Pipeline Library - a silver bullet for standardising pipelines?. Astronomical Data Analysis Software and Systems (ADASS) XIII 314:392 (2004) (eprint)

• Debian Astronomy Maintainers
• Ole Streicher

• 7.1-3 (buster)
• 6.5-1 (jessie)
• 7.0-3 (stretch)
• 7.1.3-1 (bullseye)
• 7.2.3+ds-1 (bookworm)
• 7.3.2+ds-1~bpo12+1 (bookworm-backports)
• 7.3.2+ds-1 (trixie)
• 7.3.2+ds-1 (sid)

devel

lang:c, library

field

astronomy

role

devel-lib

science

calculation

works-with

image, image:raster

• 2 regular users
• 8 recent
• 63 total installations (of 250586 submissions)

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La bibliothèque FFTW calcule les transformées de Fourier rapides (FFT) en une ou plusieurs dimensions. Elle est très rapide. Ce paquet fournit la bibliothèque statique liée, les fichiers d'en-tête et les programmes de test.

Ce paquet fournit les fichiers d'en-tête et les bibliothèques statiques. Pour la documentation, consultez libfftw3-doc.

• Matteo Frigo and Steven G. Johnson: The Design and Implementation of FFTW3. 93(2):216–231 (2005) (eprint)

• Debian Science Maintainers
• Gianfranco Costamagna

• 3.3.5-3 (stretch)
• 3.3.4-2 (jessie)
• 3.3.8-2 (buster)
• 3.3.8-2 (bullseye)
• 3.3.10-1 (bookworm)
• 3.3.10-2 (trixie)
• 3.3.10-2 (sid)

devel

library

role

devel-lib

• 425 regular users
• 427 recent
• 6667 total installations (of 250586 submissions)

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In Debian Stretch, this package is integrated in wcslib-dev.

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The GNU Scientific Library (GSL) is a collection of routines for numerical analysis. The routines are written from scratch by the GSL team in C, and present a modern API for C programmers, while allowing wrappers to be written for very high level languages.

This package contains the header files, static libraries and symbolic links that developers using GNU GSL will need.

URL: http://www.gnu.org/software/gsl/

• Dirk Eddelbuettel

• 2.7.1+dfsg-5+deb12u1 (bookworm)
• 2.3+dfsg-1 (stretch)
• 2.5+dfsg-6 (buster)
• 2.5+dfsg-6+deb10u1 (buster-security)
• 2.8+dfsg-5 (sid)
• 2.8+dfsg-5 (trixie)
• 2.6+dfsg-2 (bullseye)
• 2.6+dfsg-2+deb11u1 (bullseye-security)

• 268 regular users
• 1405 recent
• 2901 total installations (of 250586 submissions)

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In Debian Stretch, this package is integrated in wcslib-dev.

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Hierarchical Data Format 5 (HDF5) is a file format and library for storing scientific data. HDF5 was designed and implemented to address the deficiencies of HDF4.x. It has a more powerful and flexible data model, supports files larger than 2 GB, and supports parallel I/O.

This package contains development files for serial platforms.

• Gilles Filippini

• 1.10.0-patch1+docs-3+deb9u1 (stretch)
• 1.10.4+repack-10+deb10u1 (buster-security)
• 1.10.8+repack1-1 (bookworm)
• 1.10.6+repack-4+deb11u1 (bullseye)
• 1.14.5+repack-3 (sid)
• 1.14.5+repack-3 (trixie)
• 1.10.4+repack-10 (buster)
• 1.8.13+docs-15+deb8u1 (jessie-security)
• 1.8.13+docs-15+deb8u1 (jessie)
• 1.14.6 (upstream)

devel

library

role

devel-lib

• 358 regular users
• 411 recent
• 4263 total installations (of 250586 submissions)

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HEALPix is an acronym for Hierarchical Equal Area isoLatitude Pixelization of a sphere. As suggested in the name, this pixelization produces a subdivision of a spherical surface in which each pixel covers the same surface area as every other pixel. It is commonly used to store all-sky astronomical images, most famously maps of the cosmic microwave background.

This package provides .mod files for the Fortran language implementation of HEALPix.

• Debian Astro Team
• Leo Singer

• 3.60+ds-1 (sid)
• 3.60+ds-1 (bookworm)
• 3.60+ds-1 (bullseye)
• 3.60+ds-1 (trixie)
• 3.83 (upstream)

• 47 total installations (of 250586 submissions)

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LORENE is a set of C++ classes to solve various problems arising in numerical relativity, and more generally in computational astrophysics. It provides tools to solve partial differential equations by means of multi-domain spectral methods.

This package contains the static libraries and include files necessary to build LORENE codes or applications using LORENE.

Compiling LORENE codes (including some that are shipped in the lorene-codes-src package) often requires a Fortran compiler. LORENE is configured to use gfortran.

• Debian Astronomy Maintainers
• Alexandre Detiste

• 0.0.0~cvs20161116+dfsg-1 (stretch)
• 0.0.0~cvs20161116+dfsg-2 (trixie)
• 0.0.0~cvs20161116+dfsg-2 (sid)
• 0.0.0~cvs20161116+dfsg-1 (buster)
• 0.0.0~cvs20161116+dfsg-1 (bookworm)
• 0.0.0~cvs20161116+dfsg-1 (bullseye)

• 4 regular users
• 11 recent
• 95 total installations (of 250586 submissions)

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libnova is a general purpose, double precision, Celestial Mechanics, Astrometry and Astrodynamics library.

This package contains the development files.

• Debian Qt/KDE Maintainers
• Benjamin Drung

• 0.16-5 (bullseye)
• 0.16-5.1 (trixie)
• 0.16-5.1 (sid)
• 0.16-4 (buster)
• 0.16-2 (stretch)
• 0.16-5 (bookworm)
• 0.14.0-2.1 (jessie)

devel

lang:c, lang:c++, library

field

astronomy

role

devel-lib

• 8 regular users
• 8 recent
• 118 total installations (of 250586 submissions)

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Header files and a static library that are the basis of tools in the pluto-jpl-eph package.

The package is a build requirement of the pluto-lunar tools.

• Steffen Moeller
• Adrian Bunk

• 0.0~git20180228-1.1 (buster)
• 0.0~git20180228-1.1 (bullseye)
• 0.0~git20180228-1.1 (bookworm)
• 0.0~git20180228-1.1 (trixie)
• 0.0~git20180228-1.1 (sid)

• 5 regular users
• 6 recent
• 49 total installations (of 250586 submissions)

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PURIFY is a collection of routines written in C that implements different tools for radio interferometric imaging including file handling (for both visibilities and fits files), implementation of the measurement operator and set-up of the different optimization problems used for image deconvolution. The code calls the generic Sparse OPTimization (SOPT) package to solve the imaging optimization problems.

This package contains the development files.

• Luke Pratley, Jason D. McEwen, Mayeul d'Avezac, Rafael E. Carrillo, Alexandru Onose and Yves Wiaux: Robust sparse image reconstruction of radio interferometric observations with PURIFY. Mon. Not. Roy. Astron. Soc., submitted (2016) (eprint)

• Debian Astro Team
• Ole Streicher

• 2.0.0-4 (buster)
• 4.1.0-1 (sid)
• 2.0.0-5 (bullseye)
• 2.0.0-1 (stretch)
• 5.0.0 (upstream)

• 49 total installations (of 250586 submissions)

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SOPT is a C package to perform Sparse OPTimisation. It solves a variety of sparse regularisation problems, including the SARA algorithm.

SOPT is largely provided to support the PURIFY package, a companion open-source code to perform radio interferometric imaging, also written by the authors of SOPT.

This package contains the development files.

• L. Pratley, J. D. McEwen, M. d'Avezac, R. E. Carrillo, A. Onose and Y. Wiaux: Robust sparse image reconstruction of radio interferometric observations with PURIFY. Mon. Not. Roy. Astron. Soc., submitted (2016) (eprint)

• Debian Astro Team
• Ole Streicher

• 2.0.0-5 (buster)
• 2.0.0-2 (stretch)
• 3.0.1-11 (bullseye)
• 4.2.0+dfsg-2 (trixie)
• 4.2.0+dfsg-2 (sid)
• 3.0.1+dfsg-1 (bookworm)
• 5.0.0 (upstream)

• 2 regular users
• 10 recent
• 87 total installations (of 250586 submissions)

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This library is a collection of code designed to aid in replacing the SLA library with code from NOVAS and ERFA.

Where possible the API is similar to the C SLA API except for the use of a "pal" prefix.

This package contains the development files.

• T. Jenness and D. S. Berry: PAL: A Positional Astronomy Library. Astronomical Data Analysis Software and Systems XXII 475:307 (2013) (eprint)

• Debian Astronomy Team
• Phil Wyett

• 0.5.0-1 (jessie)
• 0.9.10-3 (trixie)
• 0.9.10-1 (bookworm)
• 0.9.8-1 (bullseye)
• 0.9.8-1 (buster)
• 0.9.10-3 (sid)
• 0.5.0-4 (stretch)

devel

library

role

devel-lib

• 2 regular users
• 6 recent
• 54 total installations (of 250586 submissions)

• Maintainer page
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• Git

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PgSphere, an extension for PostgreSQL, aims at providing uniform access to spherical data. It allows for a fast search and analysis for objects with spherical attributes in geographical, astronomical, or other applications using PostgreSQL.

By using an SQL interface, PgSphere's users can conveniently manage data of geographical objects around the world and astronomical data collections like star and other catalogues.

• Debian PostgreSQL Maintainers
• Christoph Berg

• 1.1.1+2018.10.13-1 (buster)

• 1 regular users
• 10 total installations (of 250586 submissions)

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Voro++ is a software library for carrying out three-dimensional computations of the Voronoi tessellation. A distinguishing feature of the Voro++ library is that it carries out cell-based calculations, computing the Voronoi cell for each particle individually. It is particularly well-suited for applications that rely on cell-based statistics, where features of Voronoi cells (eg. volume, centroid, number of faces) can be used to analyze a system of particles.

This package contains the static library and header file to compile programs against the library.

• Rycroft, C.H.: Voro++: A three-dimensional Voronoi cell library in C++. Chaos 19:41111 (2009) (eprint)

• Debian Astronomy Team
• Roger Wesson

• 0.4.6+dfsg1-3 (buster)
• 0.5+revert-to-0.4.6+dfsg1-1 (sid)
• 0.5+revert-to-0.4.6+dfsg1-1 (bullseye)
• 0.5+revert-to-0.4.6+dfsg1-1 (bookworm)
• 0.5+revert-to-0.4.6+dfsg1-1 (trixie)

• 65 total installations (of 250586 submissions)

• Maintainer page
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• Git

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• Git

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WSClean (w-stacking clean) is a fast generic widefield imager. It uses the w-stacking algorithm and can make use of the w-snapshot algorithm. As of Feb 2014, it is 2-12 times faster than CASA's w-projection, depending on the array configuration. It supports full-sky imaging and proper beam correction for homogeneous dipole arrays such as the MWA.

WSClean allows Hogbom and Cotton-Schwab cleaning, and can clean polarizations joinedly. All operations are performed on the CPU (it is not specialized for GPUs).

This package contains the static library and the header file to compile own programs against the library.

• A. R. Offringa, B. McKinley, N. Hurley-Walker, F. H. Briggs, R. B. Wayth, D. L. Kaplan, M. E. Bell, L. Feng, A. R. Neben, J. D. Hughes, J. Rhee, T. Murphy, N. D. R. Bhat, G. Bernardi, J. D. Bowman, R. J. Cappallo, B. E. Corey, A. A. Deshpande, D. Emrich, A. Ewall-Wice, B. M. Gaensler, R. Goeke, L. J. Greenhill, B. J. Hazelton, L. Hindson, M. Johnston-Hollitt, D. C. Jacobs, J. C. Kasper, E. Kratzenberg, E. Lenc, C. J. Lonsdale, M. J. Lynch, S. R. McWhirter, D. A. Mitchell, M. F. Morales, E. Morgan, N. Kudryavtseva, D. Oberoi, S. M. Ord, B. Pindor, P. Procopio, T. Prabu, J. Riding, D. A. Roshi, N. U. Shankar, K. S. Srivani, R. Subrahmanyan, S. J. Tingay, M. Waterson, R. L. Webster, A. R. Whitney, A. Williams and C. L. Williams: WSCLEAN: an implementation of a fast, generic wide-field imager for radio astronomy. Monthly Notices of the Royal Astronomical Society 444:606 - 619 (2014) (eprint)

• Debian Astro Team
• Ole Streicher

• 3.4-3 (sid)
• 2.6-1 (buster)
• 2.10.1-1 (bullseye)
• 3.1-3 (bookworm)
• 2.2.1-1 (stretch)
• 3.4-3 (trixie)

• 2 regular users
• 10 recent
• 82 total installations (of 250586 submissions)

• Maintainer page
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• Git

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Many routines are included in pgplot for viewing scientific data. Many (about 70) output devices are supported. 2-D, 3-D, contour, image manipulation, etc. are well supported. Interactive routines are included. Both a C and a FORTRAN library are present.

• Carlo Segre
• Andreas Beckmann

• 5.2.2-19.5 (non-free) (bookworm)
• 5.2.2-19+deb8u1 (non-free) (jessie)
• 5.2.2-19.3 (non-free) (stretch)
• 5.2.2-19.3 (non-free) (buster)
• 5.2.2-19.4 (non-free) (bullseye)
• 5.2.2-19.7 (non-free) (trixie)
• 5.2.2-19.7 (non-free) (sid)

devel

library

field

mathematics

role

devel-lib, shared-lib

• 51 regular users
• 7 recent
• 206 total installations (of 250586 submissions)

• Maintainer page
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Giza-dev is a DFSG-free replacement for pgplot5.