Debian Astro Scisoft packages

Le système ESO-MIDAS fournit des outils généraux pour le traitement des images et la réduction des données en mettant l'accent sur les applications astronomiques. En outre, il contient des paquets d'applications pour la photométrie stellaire ou d'objets étendus, la décomposition et l'affinage des images, ainsi que des traitements spécifiques pour l'instrumentation de l'ESO à la Silla et le Very Large Telescope (VLT) à Paranal.

• K. Banse, P. Grosbol and D. Baade: MIDAS as a Development Environment. Astronomical Data Analysis Software and Systems I 25:120 (1992)

• Debian Astro Team
• Ole Streicher

• 19.02pl1.0-1 (buster)
• 15.09pl1.0-2 (stretch)
• 13.09pl1.4-1 (jessie)
• 23.02pl1.0-2 (sid)
• 22.02pl1.0-2 (bookworm)
• 19.02pl1.1-6 (bullseye)

• 6 regular users
• 3 recent
• 113 total installations (of 236450 submissions)

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fitsverify est un logiciel qui vérifie soigneusement si un fichier de données FITS (Flexible Image Transport System) se conforme à toutes les exigences décrites dans la version 3.0 de la norme FITS.

• Debian Astro Team
• Ole Streicher

• 4.17-1 (jessie)
• 4.19-1 (buster)
• 4.22-1 (sid)
• 4.22-1 (trixie)
• 4.20-4 (bookworm)
• 4.20-3 (bullseye)
• 4.18-1 (stretch)

field

astronomy

role

program

use

checking

works-with

file

• 5 regular users
• 1 recent
• 125 total installations (of 236450 submissions)

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Funtools, is a "minimal buy-in" FITS library and utility package developed at the High Energy Astrophysics Division of SAO. The Funtools library provides simplified access to a wide array of file types: standard astronomical FITS images and binary tables, raw arrays and binary event lists, and even tables of ASCII column data. A sophisticated region filtering library (compatible with ds9) filters images and tables using boolean operations between geometric shapes, support world coordinates, etc. Funtools also supports advanced capabilities such as optimized data searching using index files.

This package contains the tools.

• E. Mandel, S.S. Murray and J.B. Roll: Funtools: An Experiment with Minimal Buy-in Software. Astronomical Data Analysis Software and Systems X 238:225 (2001)

• Debian Astro Team
• Michael Hudson-Doyle

• 1.4.4+dfsg2-1 (jessie)
• 1.4.7-1 (stretch)
• 1.4.7-4 (buster)
• 1.4.7-4 (bullseye)
• 1.4.8-1 (bookworm)
• 1.4.8-1.1 (trixie)
• 1.4.8-1.1 (sid)

• 4 regular users
• 7 recent
• 116 total installations (of 236450 submissions)

• Maintainer page
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Grace est un outil de pointage-cliquage permettant à l’utilisateur de dessiner des graphiques X-Y. Il s’agit du programme précédemment connu comme Xmgr.

Quelques-unes de ses caractéristiques sont : mise à l’échelle définie par l’utilisateur, marques de graduation, étiquettes, symboles, styles de ligne, couleurs, régression polynomiale, cerces (spline), moyenne mobile, transformation de Fourier discrète et rapide, corrélation croisée ou automatique, traitement par lots pour un tracé automatique et prise en charge de l’impression pour PostScript, FrameMaker et plusieurs formats d’image.

• Nicholas Breen

• 5.1.25-13 (trixie)
• 5.1.25-13 (bookworm)
• 5.1.25-14 (sid)
• 5.1.24-3 (jessie)
• 5.1.25-3 (stretch)
• 5.1.25-6 (buster)
• 5.1.25-9 (bullseye)

field

mathematics

interface

x11

role

program

scope

application

uitoolkit

motif

use

editing, learning, printing

works-with

image, image:vector, text

works-with-format

postscript

x11

application

• 121 regular users
• 39 recent
• 1051 total installations (of 236450 submissions)

• Maintainer page
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IPython can be used as a replacement for the standard Python shell, or it can be used as a complete working environment for scientific computing (like Matlab or Mathematica) when paired with the standard Python scientific and numerical tools. It supports dynamic object introspections, numbered input/output prompts, a macro system, session logging, session restoring, complete system shell access, verbose and colored traceback reports, auto-parentheses, auto-quoting, and is embeddable in other Python programs.

This package contains the actual terminal shell for Python 3.

• Debian Python Team
• Stefano Rivera

• 5.1.0-3+deb9u1 (stretch-security)
• 5.8.0-1+deb10u1 (buster-security)
• 7.20.0-1+deb11u1 (bullseye)
• 7.20.0-1+deb11u1 (bullseye-security)
• 8.5.0-4 (bookworm)
• 8.20.0-1 (trixie)
• 8.20.0-1 (sid)
• 2.3.0-2 (jessie)
• 5.1.0-3 (stretch)
• 5.8.0-1+deb10u1 (buster)
• 8.24.0 (upstream)

• 1203 regular users
• 256 recent
• 7144 total installations (of 236450 submissions)

• isympy3
• python3-matplotlib
• python3-sympy

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Several tasks to operate of FITS files and extensions from within IRAF, like copying, extension extraction, conversion etc.

The following tasks are available:

• fgread: Read a FITS file with FOREIGN extensions
• fgwrite: Create a FITS file with FOREIGN extensions
• funpack: Uncompress a FITS file
• fxconvert: Convert between IRAF image types.
• fxcopy: Copy FITS files or FITS extension to an output FITS file
• fxdelete: Delete FITS extensions in place
• fxdummyh: Create a dataless single FITS file
• fxextract: Extract a FITS extension
• fxheader: List one line of header description per FITS unit
• fxinsert: Insert FITS files or extensions into another FITS file
• fxplf: Converts a pixel list file into a BINTABLE extension
• fxsplit: Split a multiple extension FITS file into single FITS files
• ricepack: Rice compress a FITS file
• sum32: Compute the 32-bit FITS 1's complement checksum

• Nelson Zarate, Rob Seaman and Doug Tody: FITS Foreign File Encapsulation Convention. (2012) (eprint)

• Debian Astro Team
• Ole Streicher

• 2018.07.06-8 (sid)
• 2018.07.06-8 (trixie)
• 2018.07.06-4 (bookworm)
• 2018.07.06-4 (bullseye)
• 2018.07.06-3 (buster)

• 2 regular users
• 6 recent
• 53 total installations (of 236450 submissions)

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This package obtains radial velocities and velocity dispersions using cross-correlation methods or emission line fits. It consists of several SPP tasks:

• XCSAO and PXCSAO: cross-correlate spectra,
• EMSAO and PEMSAO: find emission lines in spectra,
• BCVCORR: solar system barycentric velocity correction,
• SUMSPEC: add and/or modify spectra,
• LINESPEC: synthetic emission line templates,
• EQWIDTH: equivalent widths of lines in spectra,
• WLRANGE: wavelength overlap range for a list of spectra,
• LISTSPEC: list pixel, wavelength, delta wavelength, and/or pixel value for spectrum image,
• PIX2WL: wavelength at a given pixel in a spectrum,
• WL2PIX: pixel at a given wavelength in a spectrum,
• VELSET Artificially change the redshift of (log-wavelength) spectra

• M. J. Kurtz and D. J. Mink: RVSAO 2.0: Digital Redshifts and Radial Velocities. Publications of the Astronomical Society of the Pacific 110:934 - 977 (1998) (eprint)

• Debian Astro Team
• Ole Streicher

• 2.8.5-1 (bookworm)
• 2.8.3-1 (buster)
• 2.8.5-2 (trixie)
• 2.8.5-2 (sid)
• 2.8.3-1 (bullseye)

• 1 recent
• 48 total installations (of 236450 submissions)

• Maintainer page
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ATLAS est une approche de la génération automatique et de l'optimisation de logiciel de calcul numérique. Actuellement, ATLAS fournit des versions optimisées de l'ensemble complet de noyaux d'algèbre linéaire connu sous le nom de « Basic Linear Algebra Subroutines » (BLAS), et d'un sous-ensemble de routines d'algèbre linéaire de la bibliothèque LAPACK.

Ce paquet fournit les en-têtes nécessaires à la compilation avec les bibliothèques que procure ATLAS.

• Debian Science Team
• Sébastien Villemot

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

devel

library

role

devel-lib

• 4 regular users
• 156 total installations (of 236450 submissions)

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• Git

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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 des programmes utilitaires, basés sur CFITSIO, à savoir fitscopy, fpack et funpack.

• Debian Astronomy Maintainers
• Benjamin Drung

• 4.2.0-3 (bookworm)
• 3.410-1 (stretch)
• 3.370-2+deb8u1 (jessie)
• 4.3.1-1 (trixie)
• 4.3.1-1.1 (sid)
• 3.450-3 (buster)
• 3.490-3 (bullseye)
• 4.4.0 (upstream)

• 89 regular users
• 76 recent
• 1154 total installations (of 236450 submissions)

• Maintainer page
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• Git

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

• 259 regular users
• 132 recent
• 2878 total installations (of 236450 submissions)

• Maintainer page
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• Git

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PLplot is relatively small, portable, freely distributable, and is rich enough to satisfy most users. It has a wide range of plot types including line (linear, log), contour, 3D, fill, and almost 1000 characters (including Greek and mathematical) in its extended font set. The package is designed to make it easy to quickly get graphical output; only a handful of function calls is typically required. For more advanced use, virtually all aspects of plotting are configurable.

This package contains all that is needed for doing development in C, C++ and Fortran with PLplot. For development in Tcl/Tk, Python and Java, install the plplot-tcl-dev, python3-plplot and libplplot-java packages, respectively. This package also includes the OCaml and Lua examples. To use one of these languages you will also need to install the libplplot-xxx package for that language.

• Debian Science Team
• Rafael Laboissière

• 5.10.0+dfsg2-0.4 (stretch)
• 5.15.0+dfsg2-7+deb13u1 (trixie)
• 5.15.0+dfsg-19 (bullseye)
• 5.15.0+dfsg2-6 (bookworm)
• 5.15.0+dfsg2-9 (sid)
• 5.10.0+dfsg-1 (jessie)
• 5.14.0+dfsg-3 (buster)

devel

library

role

devel-lib

• 7 regular users
• 15 recent
• 239 total installations (of 236450 submissions)

• Maintainer page
• Bugs
• Git

• Home page
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WCSTools est un ensemble d’utilitaires, écrits en C, qui crée, affiche et manipule le système de coordonnées mondiales (WCS) d’une image FITS ou IRAF, en utilisant des mots clés dans l’en-tête d’image qui relie la position de pixel dans l’image à une position dans le ciel. Des programmes auxiliaires recherche dans les catalogues d’étoiles et manipulent des images.

Ce paquet fournit les fichiers nécessaires au développement.

• Mink, Douglas J.: WCSTools: an Image Astrometry Toolkit. Astronomical Data Analysis Software and Systems VIII 172:498 (1999)

• Debian Astro Team
• Steve Langasek

• 3.9.7-1 (bookworm)
• 3.9.5-3 (buster)
• 3.9.4-2 (stretch)
• 3.9.0+dfsg-1 (jessie)
• 3.9.7-1.1 (sid)
• 3.9.7-1.1 (trixie)
• 3.9.6-1 (bullseye)

devel

library

role

devel-lib

• 2 regular users
• 4 recent
• 60 total installations (of 236450 submissions)

• Maintainer page
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• Git

• Home page

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Pmw est une boîte à outils pour assembler des composants graphiques Python de haut niveau en utilisant l'interface Tkinter des bibliothèques graphiques Tk. Elle se compose d'un ensemble de classes de base et d'une bibliothèque de mégawidgets flexibles et extensibles construits à partir de ces classes.

Ce paquet fournit les modules pmw.

• Carlo Segre

• 1.3.2-6 (buster)
• 1.3.2-6 (jessie)
• 1.3.2-6 (stretch)

devel

lang:python, library

role

shared-lib

uitoolkit

tk

• 12 regular users
• 131 total installations (of 236450 submissions)

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The astropy package contains core functionality and some common tools needed for performing astronomy and astrophysics research with Python. It can be extended by a number of "affiliated packages" that are intended to work with the core package.

• The Astropy Collaboration, A. M. Price-Whelan, B. M. Sipőcz, H. M. Günther, P. L. Lim, S. M. Crawford, S. Conseil, D. L. Shupe, M. W. Craig, N. Dencheva, A. Ginsburg, J. T. VanderPlas, L. D. Bradley, D. Pérez-Suárez, M. de Val-Borro, T. L. Aldcroft, K. L. Cruz, T. P. Robitaille, E. J. Tollerud, C. Ardelean, T. Babej, Y. P. Bach, M. Bachetti, A. V. Bakanov, S. P. Bamford, G. Barentsen, P. Barmby, A. Baumbach, K. L. Berry, F. Biscani, M. Boquien, K. A. Bostroem, L. G. Bouma, G. B. Brammer, E. M. Bray, H. Breytenbach, H. Buddelmeijer, D. J. Burke, G. Calderone, J. L. Cano Rodríguez, M. Cara, J. V. M. Cardoso, S. Cheedella, Y. Copin, L. Corrales, D. Crichton, D. D’Avella, C. Deil, É. Depagne, J. P. Dietrich, A. Donath, M. Droettboom, N. Earl, T. Erben, S. Fabbro, L. A. Ferreira, T. Finethy, R. T. Fox, L. H. Garrison, S. L. J. Gibbons, D. A. Goldstein, R. Gommers, J. P. Greco, P. Greenfield, A. M. Groener, F. Grollier, A. Hagen, P. Hirst, D. Homeier, A. J. Horton, G. Hosseinzadeh, L. Hu, J. S. Hunkeler, Ž. Ivezić, A. Jain, T. Jenness, G. Kanarek, S. Kendrew, N. S. Kern, W. E. Kerzendorf, A. Khvalko, J. King, D. Kirkby, A. M. Kulkarni, A. Kumar, A. Lee, D. Lenz, S. P. Littlefair, Z. Ma, D. M. Macleod, M. Mastropietro, C. McCully, S. Montagnac, B. M. Morris, M. Mueller, S. J. Mumford, D. Muna, N. A. Murphy, S. Nelson, G. H. Nguyen, J. P. Ninan, M. Nöthe, S. Ogaz, S. Oh, J. K. Parejko, N. Parley, S. Pascual, R. Patil, A. A. Patil, A. L. Plunkett, J. X. Prochaska, T. Rastogi, V. Reddy Janga, J. Sabater, P. Sakurikar, M. Seifert, L. E. Sherbert, H. Sherwood-Taylor, A. Y. Shih, J. Sick, M. T. Silbiger, S. Singanamalla, L. P. Singer, P. H. Sladen, K. A. Sooley, S. Sornarajah, O. Streicher, P. Teuben, S. W. Thomas, G. R. Tremblay, J. E. H. Turner, V. Terrón, M. H. van Kerkwijk, A. de la Vega, L. L. Watkins, B. A. Weaver, J. B. Whitmore, J. Woillez and V. Zabalza: The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package. The Astronomical Journal 156(3):123 (2018) (eprint)

• Debian Astronomy Maintainers
• Ole Streicher

• 4.2-6 (bullseye)
• 5.2.1-2 (bookworm)
• 0.4.2-2 (jessie)
• 6.0.0-1 (trixie)
• 6.0.1-4 (sid)
• 3.1.2-2 (buster)
• 1.3-8 (stretch)
• 6.1.0~rc1 (upstream)

• 254 regular users
• 119 recent
• 1345 total installations (of 236450 submissions)

• Maintainer page
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• Git

• Home page
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• Git

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Gnuplot.py est un module Python qui s'interface avec Gnuplot, le programme de tracé de courbes populaire. Il vous permet d'utiliser gnuplot depuis Python sur des tableaux de données situés en mémoire, des fichiers de données ou des fonctions mathématiques. Si vous utilisez Python pour effectuer des calculs ou comme « colle » pour les programmes numériques, vous pouvez utiliser ce module pour dessiner des données au fur et à mesure de leur calcul. Et la combinaison avec Python rend facile l'automatisation des choses, y compris la création « d'animations » brutes en dessinant les différents jeux de données les uns après les autres.

• Debian Science Maintainers
• Josue Ortega

• 1.8-8 (bookworm)
• 1.8-8 (bullseye)
• 1.8-8 (trixie)
• 1.8-8 (sid)

• 55 regular users
• 3 recent
• 164 total installations (of 236450 submissions)

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NumPy (Numerical Python) fournit un puissant objet de tableau à n dimensions, des fonctions sophistiquées (dispersion), des outils pour intégrer du code Fortran et C/C++, des outils pratiques pour l'algèbre linéaire, la transformation de Fourier et la génération de nombres aléatoires.

Ce paquet installe NumPy pour Python 3.

• Debian Python Team
• Timo Röhling

• 1.12.1-3 (stretch)
• 1.8.2-2 (jessie)
• 1.26.4+ds-8 (sid)
• 1.16.2-1 (buster)
• 1.19.5-1 (bullseye)
• 1.24.2-1 (bookworm)
• 1.24.2-2 (trixie)

• 25318 regular users
• 2519 recent
• 43037 total installations (of 236450 submissions)

• python3-shapely

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The XPA messaging system provides seamless communication between many kinds of Unix programs, including Tcl/Tk programs such as ds9. The pyds9 module uses a Python interface to XPA to communicate with ds9. It supports communication with all of ds9’s XPA access points.

• Debian Astronomy Team
• Ole Streicher

• 1.8.1-1 (stretch)
• 1.8.1-5 (sid)
• 1.8.1-5 (trixie)
• 1.8.1-5 (bookworm)
• 1.8.1-5 (bullseye)
• 1.8.1-5 (buster)

• 56 regular users
• 1 recent
• 133 total installations (of 236450 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

Last version of python-numdisplay was 1.5.6 from 2009. Use python3-pyds9 instead.

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pysynphot simulates photometric data and spectra as they are observed with the Hubble Space Telescope (HST). Passbands for standard photometric systems are available, and users can incorporate their own filters, spectra, and data. pysynphot user interface allows you to:

• Construct complicated composite spectra from various grids of model atmosphere spectra, parameterized spectrum models, and atlases of stellar spectrophotometry.
• Simulate observations.
• Query the resulting structures for quantities of interest, such as countrate, effective wavelength, effective stimulus, as well as the wavelength and flux arrays.
• Plot HST sensitivity curves and calibration target spectra.
• Compute photometric calibration parameters for any HST instrument mode.

pysynphot can help HST observers to perform cross-instrument simulations, to examine the transmission curve of the HST Optical Telescope Assembly (OTA), and spectra of HST calibration targets. Expert users can take advantage of the control and data structures available in Python to easily perform repetitive operations such as simulate the observation of multiple type of sources through multiple observing modes.

• P. L. Lim, R. I. Diaz and V. Laidler: PySynphot User’s Guide. (2015)

• Debian Astronomy Team
• Ole Streicher

• 0.9.12+dfsg-3 (buster)
• 2.0.0+dfsg-1 (bookworm)
• 1.0.0+dfsg-1 (bullseye)
• 2.0.0+dfsg-1 (sid)
• 0.9.8.5+dfsg-1 (stretch)

• 7 regular users
• 1 recent
• 116 total installations (of 236450 submissions)

• Maintainer page
• Bugs
• Git

• Home page
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Il s'agit d'un module pour écrire des applications GUI portables avec Python⋅3.x en utilisant Tk. Il est aussi connu sous le nom Tkinter.

• Matthias Klose

• 3.4.2-1 (jessie)
• 3.7.3-1 (buster)
• 3.12.3-1 (sid)
• 3.11.5-1 (trixie)
• 3.11.2-3 (bookworm)
• 3.9.2-1 (bullseye)
• 3.5.3-1 (stretch)

• 16275 regular users
• 1806 recent
• 33047 total installations (of 236450 submissions)

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SAOImage DS9 est application d’imagerie et de visualisation pour l’astronomie. DS9 gère les images FITS et les tables binaires, plusieurs tampons de trame, la manipulation de région et plusieurs algorithmes d’échelle et de cartes de couleurs. Il permet une communication facile avec des tâches d’analyse externes et est hautement configurable et extensible à l’aide de XPA et SAMP.

Toutes les versions et plateformes prennent en charge un ensemble cohérent de capacités graphiques fonctionnelles.

DS9 prend en charge des fonctions modernes telles que les tampons de trame 2D, 3D et RVB, les images en mosaïque, le pavage, le clignotement, les repères géométriques, la manipulation de carte de couleur, le changement d’échelle, l’agrandissement arbitraire, le recadrage, la rotation, le panorama et une variété de systèmes de coordonnées.

L’interface graphique pour DS9 est personnalisable par l’utilisateur. Les éléments graphiques tels que l’affichage des coordonnées, le panorama (panner), la loupe, les graphes horizontaux et verticaux, la barre de boutons et la barre de couleurs peuvent être configurés à l’aide de menus ou la ligne de commande.

• W. A. Joye and E. Mandel: New Features of SAOImage DS9. Astronomical Data Analysis Software and Systems XII 295:489 (2003)

• Debian Astronomy Maintainers
• Ole Streicher

• 8.0.1+repack-2 (buster)
• 7.3.2+repack-1 (jessie)
• 7.5+repack1-2 (stretch)
• 8.2+repack-2 (bullseye)
• 8.4.1+repack-3 (bookworm)
• 8.5+repack-1 (trixie)
• 8.5+repack-1 (sid)
• 8.6~b1 (upstream)

field

astronomy

interface

x11

role

program

science

visualisation

uitoolkit

tk

use

viewing

x11

application

• 33 regular users
• 5 recent
• 351 total installations (of 236450 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

saoimage is outdated; use saods9

The ESO/Starlink Skycat tool combines the image display capabilities of the RTD (Real-Time Display) with a set of classes for accessing astronomical catalogs locally and over the network using HTTP. The tool allows you to view FITS images from files or from the Digitized Sky Survey (DSS).

• M.A. Albrecht, A. Brighton, T. Herlin, P. Biereichel and D. Durand: Access to Data Sources and the ESO SkyCat Tool. Astronomical Data Analysis Software and Systems VI 125:333 (1997)

• Debian Astronomy Maintainers
• Ole Streicher

• 3.1.2+starlink1~b+dfsg-5 (buster)
• 3.1.2+starlink1~b+dfsg-7 (sid)
• 3.1.2+starlink1~b+dfsg-5 (bullseye)
• 3.1.2+starlink1~b+dfsg-7 (trixie)
• 3.1.2+starlink1~b+dfsg-7 (bookworm)
• 3.1.2+starlink1~b-8 (jessie)
• 3.1.2+starlink1~b+dfsg-2 (stretch)

field

astronomy

interface

x11

role

program

science

visualisation

uitoolkit

tk

use

viewing

x11

application

• 10 regular users
• 3 recent
• 147 total installations (of 236450 submissions)

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THELI est un outil puissant pour réduire les images d’astronomie dans l’infrarouge proche et l’infrarouge moyen, prenant en charge plus de cent instruments, ayant une ou plusieurs puces, d’observatoires professionnels tout autour du globe. L’interface graphique et le modèle de données interne permettent à l’utilisateur de se concentrer sur le processus de traitement de données hautement automatisé sans être perturbé par la complexité et les caractères spécifiques des instruments d’optique dans l’infrarouge. THELI est complètement adaptable sur les machines à plusieurs processeurs avec mémoire partagée, permettant un traitement rapide de grands ensembles de données. Le visualisateur intégré des données permet l’accès à n’importe quel produit de périphérique ou en mémoire. Des instruments personnels peuvent être ajoutés, rendant aussi THELI intéressant pour les astronomes amateurs.

• Mischa Schirmer: THELI: Convenient Reduction of Optical, Near-infrared, and Mid-infrared Imaging Data. The Astrophysical Journal Supplement 209(2):16 (2013) (eprint)

• Debian Astro Team
• Kay Thriemer

• 3.1.4-1 (sid)
• 3.0.5-2 (bullseye)
• 3.1.4-1 (bookworm)

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WCSTools est un ensemble d’utilitaires, écrits en C, qui crée, affiche et manipule le système de coordonnées mondiales (WCS) d’une image FITS ou IRAF, en utilisant des mots clés dans l’en-tête d’image qui relie la position de pixel dans l’image à une position dans le ciel. Des programmes auxiliaires recherche dans les catalogues d’étoiles et manipulent des images.

Ce paquet fournit les outils exécutables.

• Mink, Douglas J.: WCSTools: an Image Astrometry Toolkit. Astronomical Data Analysis Software and Systems VIII 172:498 (1999)

• Debian Astro Team
• Steve Langasek

• 3.9.7-1.1 (sid)
• 3.9.7-1.1 (trixie)
• 3.9.7-1 (bookworm)
• 3.9.6-1 (bullseye)
• 3.9.5-3 (buster)
• 3.9.4-2 (stretch)
• 3.9.0+dfsg-1 (jessie)

• 8 regular users
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Ximtool provides an image display capability to remote client applications for IRAF using the standard imtool/iis image display protocol. The image display server allows a number of image frame buffers to be created and displayed. The client can read and write data in these frame buffers. Any frame or combination of frames can be displayed. Various display options are provided, e.g., zoom and pan, flip about either axis, frame blink, windowing of the display, and colortable enhancement.

• Tody, Doug: A Portable GUI Development System---The IRAF Widget Server. ASP Conference Series 77 (1995) (eprint)

• Debian Astro Team
• Ole Streicher

• 2.0+2020.06.15+dfsg-1 (bullseye)
• 2.1+dfsg-2 (sid)
• 2.1+dfsg-1 (trixie)
• 2.1+dfsg-1 (bookworm)
• 2.0+2020.06.15+dfsg-1~bpo10+1 (buster-backports)

• 3 regular users
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Whatever this is

• Debian Astro Team
• Ole Streicher

• 1994.02.17-1 (VCS)

• Git

Xephem is an interactive astronomical ephemeris program for X Windows systems with Motif. It provides many graphical views as well as quantitative heliocentric, geocentric and topocentric information for Earth satellites, solar system and celestial objects.

• Debian Astronomy Maintainers
• Lukasz Sanocki

• 4.2.0+ds-1 (VCS)

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Not DFSG-Free.

Written in ANSI C, eclipse is a library offering numerous services related to astronomical image processing: FITS data access, various image and cube loading methods, binary image handling and filtering (including convolution and morphological filters), 2-D cross- correlation, connected components, cube and image arithmetic, dead pixel detection and correction, object detection, data extraction, flat- fielding with robust fit, image generation, statistics, photometry, image-space resampling, image combination, and cube stacking. It also contains support for mathematical tools like random number generation, FFT, curve fitting, matrices, fast median computation, and point-pattern matching. The main feature of this library is its ability to handle large amounts of input data (up to 2GB in the current version) regardless of the amount of memory and swap available on the local machine. Another feature is the very high speed allowed by optimized C, making it an ideal base tool for programming efficient number-crunching applications, e.g., on parallel (Beowulf) systems.

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Latest version: 5.0-0 released 23 Sept 2005

A prototype IRAF color image display package, COLOR, is now available. Currently this package provides conversion of 3 bandpass IRAF images to a Sun 24-bit RGB rasterfile format, a 24-bit to 8-bit compression algorithm and Floyd-Steinberg dithering, and an RGB 8-bit pixel dithering algorithm. The Sun rasterfiles are displayed using non-IRAF tools and the others use only IRAF images and SAOimage or IMTOOL. These tasks are usable with the currently common 8-bit color workstations and are provided for those users which don't have more capable hardware such as 24-bit workstations, IIS displays, and 24-bit addon cards.

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MXTOOLS is an IRAF package providing tools for image matching and image coordinate manipulation.

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TABLES provides support for tabular data for STSDAS and other packages. Many types of data are stored in tabular format, such as catalogs of astronomical objects, spectral data (e.g. columns of wavelength and flux), and coefficients of fit to data. TABLES provides a programming interface for accessing tables, and it includes a collection of utility programs for working with tables. FITS tables, STSDAS format, and simple text tables are supported. The programming interface is used for the utility programs in TABLES, by tasks in STSDAS, and by other external packages. The utility programs are used for such tasks as plotting, selecting rows based on an expression involving column values, sorting rows in a table, joining tables, and performing arithmetic operations on column values.

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PLASTIC is a protocol for communication between client-side astronomy applications. It is very simple for application developers to adopt and is easily extended. Through PLASTIC applications can do tasks such as instruct each other to load VOTables, highlight a subset of rows or load an image of a particular area of sky. Although such operations are quite simple, they enable powerful collaborations between tools. The philosophy is that the astronomer should have a suite of interoperating tools at his disposal, each of which does one thing well and which can be composed according to his particular needs.

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The IVOA Applications Working Group has now produced a specification for SAMP, the successor protocol to PLASTIC. It is recommended to use SAMP rather than PLASTIC.

AstroAsciiData is a Python module to handle ASCII tables. Features:

• Imports all reasonably well-formed Ascii tables
• Column-first access
• Easy creation and manipulation of tables, columns, rows and attached comments
• Retains formatting of data values
• Support for SExtractor style headers
• Column sorting
• Interchangeable comment character, column delimiter and null value
• Exports data to Ascii, Numpy/Numarray, FITS table, HTML table, LaTeX table

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Python-asciidata and pyfits are obsoleted by python3-astropy.

Numeric is a Python module for high-performance, numeric computing. It provides much of the functionality and performance of commercial numeric software such as Matlab; in some cases, it provides more functionality than commercial software.

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Python-numeric is not maintained anymore, outdated by python3-numpy

Specview is a tool for 1-D spectral visualization and analysis of astronomical spectrograms. Written in Java, it is capable of reading all the Hubble Space Telescope spectral data formats as well as data from several other instruments (such as IUE, FUSE, ISO, FORS and SDSS), preview spectra from MAST, and data from generic FITS and ASCII tables. It can read data from Virtual Observatory servers, and read and write spectrogram data in Virtual Observatory SED format. It can also read files in the SPC Galactic format used in the chemistry field. Once ingested, data can be plotted and examined with a large selection of custom settings. Specview supports instrument-specific data quality handling, flexible spectral units conversions, custom plotting attributes, plot annotations, tiled plots, hardcopy to JPEG files and PostScript file or printer, etc. Specview can be used to build wide-band SEDs, overplotting or combining data from the same astronomical source taken with different instruments and/or spectral bands. Data can be further processed with averaging, splicing, detrending, and Fourier filtering tools. Specview has a spectral model fitting capability that enables the user to work with multi-component models (including user- defined models) and fit models to data.

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Tiny Tim generates simulated Hubble Space Telescope point spread functions (PSFs). It is written in C and distributed as source code and runs on a wide variety of UNIX and VMS systems. Tiny Tim includes mirror zonal errors, time dependent aberrations (for the pre-repair instruments), field dependent obscuration patterns (for WF/PC-1 and WFPC2), and filter passband effects. It can produce a normally sampled or subsampled PSF. Output is a FITS image file.

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Unknown, unspecified license

VOPlot is a tool for visualizing astronomical data. It was developed in Java and acts on data available in VOTABLE, ASCII and FITS formats. VOPlot is available as a stand alone version, which is to be installed on the user's machine, or as a web-based version fully integrated with the VizieR database.

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