Debian Science Astronomy-dev packages

Pakken casacore indeholder basisbibliotekerne for den gamle pakke AIPS++/CASA (Common Astronomy Software Applications). Denne opdeling blev lavet for at få en bedre separation af basisbibliotekerne og programmer.

Denne pakke indeholder filerne for programudvikling.

Astro::Fits::Cfitsio is a Perl interface to William Pence's cfitsio subroutine library. For more information on cfitsio, see http://heasarc.gsfc.nasa.gov/fitsio.

This module attempts to provide a wrapper for nearly every cfitsio routine, while retaining as much cfitsio behavior as possible. As such, one should be aware that it is still somewhat low-level, in the sense that handing an array which is not the correct size to a routine like fits_write_img() may cause SIGSEGVs.

The goal is to eventually use these routines to build a more Perl-like interface to many common tasks such as reading and writing of images and ASCII and binary tables.

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) is a data format most used in astronomy. cfitsio is a library of ANSI C routines for reading and writing FITS format data files. A set of Fortran-callable wrapper routines are also included for the convenience of Fortran programmers.

This package contains what you need for compiling sources that use this library in your own 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) er standarden for dataformatet i astronomi brugt for transport, analyse og arkivlagring af videnskabelige datasæt.

Dette bibliotek tilbyder effektiv I/O for FITS-billeder og binære tabeller. Alle grundlæggende FITS-formater og gzip-komprimerede filer er understøttet.

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) er en distribueret XML-baseret kontrolprotokol designet til at styre astronomiske instrumenter. INDI er lille, fleksible, nem at fortolke, skalerbar og tilstandsløs. Den understøtter gængse DCS-funktioner såsom fjernkontrol, dataindhentelse, overvågning og meget mere.

Denne pakke indeholder udviklingsteksthoveder og biblioteker for INDI-biblioteket.

Libnova er et alment bibliotek for dobbeltpræcision, himmelmekanik, astrometri og astrodynamik.

Denne pakke indeholder udviklingsfilerne.

Denne pakke indeholder hovedfilerne og statisk bibliotek krævet for at kompilere programmer som bruger 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.

Dette bibliotek er en kodesamling designet til at hjælpe med at erstatte SLA-biblioteket med kode fra NOVAS og ERFA.

Hvor muligt ligner API'en C SLA API'en med undtagelse af brugen af et »pal-præfiks«.

Denne pakke indeholder udviklingsfilerne.

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.

Dette modul kan vise, konfigurere og køre CPL-baserede opskrifter fra Python3. Inddata, kalibrering og uddata kan specificeres som FITS-filer eller som pyfits-objekter i hukommelsen.

Common Pipeline Library (CPL) består af et sæt af ISO-C-biblioteker, som tilbyder et omfattende, effektivt og robust programværktøjssæt. Den udfører et grundlag for oprettelsen af automatiserede astronomiske datareduktionsopgaver.

En af funktionerne tilbudt af CPL'en er muligheden for at oprette algoritmer for datareduktion, som kører som udvidelsesmoduler (dynamiske biblioteker). Disse kaldes for »opskrifter« og er et af hovedaspekterne til udviklingsmiljøet for CPL-datareduktion.

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.

Dette er et tyndt omslag omkring de høje og mellemniveau grænseflader for Dr. Mark Calabrettas WCSLIB for håndtering af World Coordinate System.

Derudover er der udvidelser (skrevet i C) til at understøtte Spitzer Simple Imaging Polynomial (SIP)-konventionsnøgleord og Paper IV-tabelopslagsforstyrrelse.

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 er en udvidelse af Tcl-sproget, der tilbyder simpel adgang til astronomiske data gemt i FITS-filformatet. fitsTcl implementerer en Tcl- grænseflade til biblioteket cfitsio, udviklet af HEASARC (High Energy Astrophysics Science Archive Research Center) på NASA Goddard Space Flight Center.

WCSLIB er et C-bibliotek, udrustet med et fuld sæt af Fortran-omslag, som implementerer standarden »World Coordinate System« (WCS) i FITS (Flexible Image Transport System).

PGSBOX tegner og etiketterer et krumt koordinatsystem. Kalderen skal tilbyde en separat ekstern funktion, NLFUNC, til at definere den ikkelineære koordinattransformation.

Denne pakke indeholder det statiske bibliotek og C-teksthovedfilerne.

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).