Debian Science Astronomy-dev 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.

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.

CCfits is an object oriented interface to the cfitsio library. It is designed to make the capabilities of cfitsio available to programmers working in C++. It is written in ANSI C++ and implemented using the C++ Standard Library with namespaces, exception handling, and member template functions.

This package contains what you need for compiling sources that use this library in your own code.

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.

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 the static library and headers for the C language implementation of HEALPix. The C library provides basic input/output of HEALPix maps as well as basic spatial operations like conversion between spherical coordinates and HEALPix pixels.

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.

ERFA is a C library containing key algorithms for astronomy, and is based on the SOFA library published by the International Astronomical Union (IAU).

It is intended to replicate the functionality of SOFA (aside from possible bugfixes in ERFA that have not yet been included in SOFA), but is licensed under a three-clause BSD license to enable its compatibility with a wide range of open source licenses. Permission for this release has been obtained from the SOFA board.

This package contains the header files and the static library.

FITS (Flexible Image Transport System) is the standard data format in astronomy used for the transport, analysis, and archival storage of scientific data sets.

This library provides efficient I/O for FITS images and binary tables. All basic FITS formats and gzip compressed files are supported.

Gyoto aims at providing a framework for computing orbits and ray-traced images in General relativity.

This package provides the files necessary to compile Gyoto plugins and codes using the libgyoto library.

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 the static library and headers for the C++ language implementation of HEALPix. The C++ library provides input/output, basic spatial operations such as conversion between spherical coordinates and HEALPix pixels, and also sophisticated spatial operations such as querying cones or polygons, as well as upsampling/downsampling, smoothing, and fast spherical harmonic transforms.

INDI (Instrument-Neutral Device Interface) is a distributed XML-based control protocol designed to operate astronomical instrumentation. INDI is small, flexible, easy to parse, scalable, and stateless. It supports common DCS functions such as remote control, data acquisition, monitoring, and a lot more.

This package contains development headers and libraries for the INDI library.

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

This package contains the development files.

This package contains the header files and static library needed to compile applications that use qfits.

AST implements an object oriented model for describing physical coordinate systems, and the transformations that exist between them.

It provides a comprehensive range of facilities for attaching world coordinate systems (WCS) to astronomical data and for retrieving and manipulating that information.

It has built-in intelligence for identifying types of celestial, spectral, time and other coordinate systems (including compound systems that combine axes of different types) and determining how to transform between them. This allows general purpose code to be written that makes no assumptions about the nature of the coordinate systems.

This package contains the files needed for development.

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.

WCSTools is a set of software utilities, written in C, which create, display and manipulate the world coordinate system of a FITS or IRAF image, using specific keywords in the image header which relate pixel position within the image to position on the sky. Auxiliary programs search star catalogs and manipulate images.

This package contains the files needed for development.

This module can list, configure and execute CPL-based recipes from Python3. The input, calibration and output data can be specified as FITS files or as pyfits objects in memory.

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.

One of the features provided by the CPL is the ability to create data-reduction algorithms that run as plugins (dynamic libraries). These are called "recipes" and are one of the main aspects of the CPL data-reduction development environment.

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 a Python wrapper around the C++ implementation of HEALPix.

FITS (Flexible Image Transport System) is a data format most used in astronomy. PyFITS is a Python module for reading, writing, and manipulating FITS files. The module uses Python's object-oriented features to provide quick, easy, and efficient access to FITS files. The use of Python's array syntax enables immediate access to any FITS extension, header cards, or data items.

Note that the development of PyFITS has been stopped and will not see any new upstream version. It is superseded by the module astropy.io which is almost a drop-in replacement. PyFITS should therefore only be used for compatibility reasons, astropy should be used instead for new developments.

This package provides PyFITS on the Python 2 module path. It is complemented by python3-pyfits.

This is a thin wrapper around the high- and mid-level interfaces of Dr. Mark Calabretta's WCSLIB for handling the World Coordinate System.

In addition, there are extensions (written in C) to support Spitzer Simple Imaging Polynomial (SIP) convention keywords and Paper IV table lookup distortion.

The CFITSIO library consists of a set of functions for reading and writing FITS (Flexible Image Transport System) files. The S-Lang CFITSIO module wraps many of the functions of the CFITSIO library and permits one to easily manipulate FITS files from the S-Lang interpreter.

fitsTcl is an extension to the Tcl language, providing simple access to astronomical data stored in FITS file format. fitsTcl implements a Tcl interface to the cfitsio library, developed by the HEASARC (High Energy Astrophysics Science Archive Research Center) at the NASA Goddard Space Flight Center.

WCSLIB is a C library, supplied with a full set of Fortran wrappers, that implements the "World Coordinate System" (WCS) standard in FITS (Flexible Image Transport System).

PGSBOX draws and labels a curvilinear coordinate grid. The caller must provide a separate external function, NLFUNC, to define the non-linear coordinate transformation.

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

World Wind allows any user to zoom from satellite altitude into any place on Earth, leveraging high resolution LandSat imagery and SRTM elevation data to experience Earth in visually rich 3D, just as if they were really there.

This package contains the worldwind library.

The ivoafits package consists of a set of classes which can be used by any Java application to load and view images available in the widespread FITS (Flexible Image Transport System) data format.

The package is a software tool of the Virtual Observatory (VO) providing an astronomical research environment. It is used by several VO applications, e.g. TOPCAT or VO Enabled Mirage. The library depends on Thomas McGlynn's nom.tam.fits package ("libfits-java" in Debian).