Debian Astro Fedora packages

Dia 是一個圖表、曲線圖、圖形等的編輯器，支援 UML 靜態結構圖表（類別圖）、實體關係 （ER）圖、網路架構圖及其他圖表等，並可匯出成 postscript 及許多格式。

• Philippe SWARTVAGHER

• 0.97.3+git20220525-5 (bookworm)
• 0.98+git20260221-1 (sid)
• 0.98+git20260221-1 (forky)
• 0.98+git20250126-2 (trixie)
• 0.97.3+git20160930-9 (bullseye)

interface

x11

role

program

scope

application

suite

gnu

uitoolkit

gtk

use

editing

works-with

image, image:vector

x11

application

• 478 regular users
• 657 recent
• 5147 total installations (of 281236 submissions)

• Maintainer page
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GIMP is an advanced picture editor. You can use it to edit, enhance, and retouch photos and scans, create drawings, and make your own images. It has a large collection of professional-level editing tools and filters, similar to the ones you might find in Photoshop. Numerous fine-control settings and features like layers, paths, masks, and scripting give you total control over your images.

Many image file formats are supported, including JPEG, Photoshop (.psd), and Paint Shop Pro (.psp) files. It can also be used to scan and print photos.

To open files remotely (like over HTTP), install the gvfs-backends package.

To use a MIDI device (like a musical keyboard) as an input controller in GIMP, install libasound2 and read the how-to at /usr/share/doc/gimp/README.MIDI

• Debian GNOME Extras Maintainers
• Jeremy Bícha

• 2.10.22-4+deb11u2 (bullseye)
• 2.10.22-4+deb11u7 (bullseye-security)
• 2.10.34-1+deb12u5 (bookworm)
• 2.10.34-1+deb12u9 (bookworm-security)
• 2.10.34-1+deb12u9 (bookworm-proposed-updates)
• 3.2.0~RC3-1 (sid)
• 3.2.0~RC3-1 (forky)
• 3.0.4-3+deb13u7 (trixie)
• 3.0.4-3+deb13u7 (trixie-security)
• 3.2.0 (upstream)

field

arts

interface

x11

role

program

scope

application

suite

gimp, gnu

uitoolkit

gtk

use

editing, learning

works-with

image, image:raster, text

works-with-format

gif, jpg, pdf, png, tiff

x11

application

• 9806 regular users
• 32378 recent
• 64343 total installations (of 281236 submissions)

• entangle
• gimp-data
• gimp-data-extras
• gimp-gmic
• gimp-gutenprint
• gimp-help-bg
• gimp-help-ca
• gimp-help-cs
• gimp-help-da
• gimp-help-de
• gimp-help-el
• gimp-help-en
• gimp-help-en-gb
• gimp-help-eo
• gimp-help-es
• gimp-help-fa
• gimp-help-fi
• gimp-help-fr
• gimp-help-hr
• gimp-help-hu
• gimp-help-it
• gimp-help-ja
• gimp-help-ko
• gimp-help-lt
• gimp-help-nl
• gimp-help-nn
• gimp-help-pl
• gimp-help-pt
• gimp-help-pt-br
• gimp-help-ro
• gimp-help-ru
• gimp-help-sk
• gimp-help-sl
• gimp-help-sv
• gimp-help-tr
• gimp-help-uk
• gimp-help-zh-cn
• gimp-plugin-registry

• Maintainer page
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Git is popular version control system designed to handle very large projects with speed and efficiency; it is used for many high profile open source projects, most notably the Linux kernel.

Git falls in the category of distributed source code management tools. Every Git working directory is a full-fledged repository with full revision tracking capabilities, not dependent on network access or a central server.

This package provides the git graphical user interface.

If aspell is installed, it can check the spelling of commit messages as the user types.

If meld is installed, it can be used for displaying diffs and for interactive merge conflict resolution.

• Jonathan Nieder

• 2.30.2-1+deb11u5 (bullseye-security)
• 2.39.5-0+deb12u2 (bookworm-security)
• 2.53.0-1 (sid)
• 2.30.2-1+deb11u2 (bullseye)
• 2.47.3-0+deb13u1 (trixie)
• 2.39.5-0+deb12u3 (bookworm)
• 2.53.0-1 (forky)
• 2.51.0+next.20250825-1 (experimental)
• 2.53.0+next.20260227-1 (experimental)

devel

rcs

interface

x11

role

program

uitoolkit

tk

use

downloading, editing, storing, synchronizing, viewing

works-with

file, software:source, vcs

x11

application

• 395 regular users
• 474 recent
• 5153 total installations (of 281236 submissions)

• Maintainer page
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• Git

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• Matthias Klose

• 3.9.2-3 (bullseye)
• 3.11.2-1 (bookworm)
• 3.14.3 (upstream)

• 549 total installations (of 281236 submissions)

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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 the INDI server, the drivers for the supported astronomical instrumentation, and other INDI tools.

• Debian KDE Extras Team
• Aurélien COUDERC

• 1.9.9+dfsg-3 (trixie)
• 1.8.8+dfsg-1 (bullseye)
• 1.9.9+dfsg-2 (bookworm)
• 1.9.9+dfsg-6 (forky)
• 1.9.9+dfsg-6 (sid)
• 2.1.9+dfsg-1 (experimental)
• 2.1.9 (upstream)

field

astronomy

interface

commandline

network

service

role

program

• 159 regular users
• 103 recent
• 1177 total installations (of 281236 submissions)

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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
• Gordon Ball

• 9.8.0-4 (forky)
• 8.35.0-1 (trixie)
• 7.20.0-1+deb11u1 (bullseye-security)
• 7.20.0-1+deb11u1 (bullseye)
• 8.5.0-4 (bookworm)
• 9.11.0-1 (sid)

• 1131 regular users
• 888 recent
• 7616 total installations (of 281236 submissions)

• isympy3
• python3-matplotlib
• python3-sympy

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• Git

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• Git

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Kst is a fast real-time large-dataset viewing and plotting tool. It has basic data analysis functionality, contains many powerful built-in features and is expandable with plugins and extensions.

• Debian QA Group
• Syed-Shahrukh Hussain

• 2.0.8-6 (trixie)
• 2.0.8-7 (forky)
• 2.0.8-5 (bookworm)
• 2.0.8-7 (sid)
• 2.0.8-4 (bullseye)
• plot-3.0.0 (upstream)

field

chemistry, physics

interface

commandline, x11

role

program

suite

kde

uitoolkit

qt

use

viewing

x11

application

• 25 regular users
• 115 recent
• 397 total installations (of 281236 submissions)

• Maintainer page
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• Git

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The Debian package includes the FITS reader that is a separate package on Fedora.

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KStars is a scientifically accurate desktop planetarium, visualising a graphical simulation of the night sky from any location on Earth, at any date and time. The display includes 130,000 stars, 13,000 deep-sky objects, all 8 planets, the Sun and Moon, and thousands of comets and asteroids. KStars addresses students and amateur astronomers of all levels.

The database of known objects can be extended and updated from local or remote databases, which is prepared for in a user-extendable interface. KStars suggests observations of particular interest like conjunctions with respect to the location of the user. And for user-selected targets it proposes the ones that are best-observable.

The software may be used for planning experiments around the globe, e.g. for remote controlled commercial services. But KStars also features an INDI interface to control local telescopes and cameras. Users with programming experience can script it via the KDE desktop bus.

• Debian KDE Extras Team
• Pino Toscano

• 3.4.3-1 (bullseye)
• 3.6.2-2 (bookworm)
• 3.6.2-2 (trixie)
• 3.6.2-2 (forky)
• 3.6.2-2 (sid)
• 3.8.1-2 (experimental)

field

astronomy

interface

x11

role

program

suite

kde

uitoolkit

qt

use

learning

x11

application

• 112 regular users
• 56 recent
• 1236 total installations (of 281236 submissions)

• kstars-data-extra-tycho2

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• Debian Astronomy Maintainers
• Aurelien Jarno

• 4.6.3-1 (sid)
• 4.6.3-1 (forky)
• 4.6.2-2 (trixie)
• 3.490-3 (bullseye)
• 4.2.0-3 (bookworm)

• 122 regular users
• 71 recent
• 1220 total installations (of 281236 submissions)

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Extract models of the Point Spread Function (PSF) from FITS images processed with SExtractor, and measures the quality of images. The generated PSF models can be used for model-fitting photometry or morphological analyses.

• Bertin, Emmanuel: Automated Morphometry with SExtractor and PSFEx. 442:435 (2011) (eprint)

• Debian Astronomy Maintainers
• Ole Streicher

• 3.24.2-2 (forky)
• 3.21.1-1 (bookworm)
• 3.24.2-2 (trixie)
• 3.24.2-2 (sid)
• 3.17.1+dfsg-6 (bullseye)

• 6 regular users
• 12 recent
• 116 total installations (of 281236 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

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APLpy is a Python module aimed at producing publication-quality plots of astronomical imaging data in FITS format. The module uses Matplotlib, a powerful and interactive plotting package. It is capable of creating output files in several graphical formats, including EPS, PDF, PS, PNG, and SVG.

• Debian Astronomy Team
• Ole Streicher

• 2.0.3-2 (bullseye)
• 2.2.0-2 (sid)
• 2.2.0-2 (forky)
• 2.2.0-1 (trixie)
• 2.1.0-1 (bookworm)

• 13 regular users
• 12 recent
• 183 total installations (of 281236 submissions)

• Maintainer page
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• Git

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• Git

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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

• 7.2.0-1 (sid)
• 5.2.1-2 (bookworm)
• 7.2.0-1 (forky)
• 4.2-6 (bullseye)
• 7.0.1-3 (trixie)
• 8.0.0 (upstream)

• 338 regular users
• 122 recent
• 1573 total installations (of 281236 submissions)

• Maintainer page
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• Git

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The ccdproc package provides many of the necessary tools for processing of ccd images built on a framework to provide error propagation and bad pixel tracking throughout the reduction process.

• Debian Astronomy Team
• Ole Streicher

• 2.5.1-3 (forky)
• 2.1.0-4 (bullseye)
• 2.4.0-1 (bookworm)
• 2.4.3-1 (trixie)
• 2.5.1-3 (sid)

• 14 regular users
• 12 recent
• 186 total installations (of 281236 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

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NetworkX is a Python-based package for the creation, manipulation, and study of the structure, dynamics, and functions of complex networks.

The structure of a graph or network is encoded in the edges (connections, links, ties, arcs, bonds) between nodes (vertices, sites, actors). If unqualified, by graph it's meant a simple undirected graph, i.e. no self-loops and no multiple edges are allowed. By a network it's usually meant a graph with weights (fields, properties) on nodes and/or edges.

The potential audience for NetworkX includes: mathematicians, physicists, biologists, computer scientists, social scientists.

This package contains the Python 3 version of NetworkX.

• Debian OpenStack
• Thomas Goirand

• 3.2.1-5 (trixie)
• 2.8.8-1 (bookworm)
• 3.4.2-4 (forky)
• 3.4.2-4 (sid)
• 2.5+ds-2 (bullseye)
• 3.6.1 (upstream)

• 967 regular users
• 530 recent
• 6122 total installations (of 281236 submissions)

• Maintainer page
• Bugs
• Git

• Home page
• Bugs
• Git

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pandas is a Python package providing fast, flexible, and expressive data structures designed to make working with "relational" or "labeled" data both easy and intuitive. It aims to be the fundamental high-level building block for doing practical, real world data analysis in Python. pandas is well suited for many different kinds of data:

• Tabular data with heterogeneously-typed columns, as in an SQL table or Excel spreadsheet
• Ordered and unordered (not necessarily fixed-frequency) time series data.
• Arbitrary matrix data (homogeneously typed or heterogeneous) with row and column labels
• Any other form of observational / statistical data sets. The data actually need not be labeled at all to be placed into a pandas data structure

This package contains the Python 3 version.

• McKinney, Wes: pandas: a Foundational Python Library for Data Analysis and Statistics. (2011) (eprint)

• Debian Science Maintainers
• Graham Inggs

• 1.5.3+dfsg-2 (bookworm)
• 2.3.3+dfsg-3 (sid)
• 2.3.3+dfsg-3 (forky)
• 1.1.5+dfsg-2 (bullseye)
• 2.2.3+dfsg-9 (trixie)
• 3.0.1 (upstream)

• 796 regular users
• 611 recent
• 7439 total installations (of 281236 submissions)

• python3-bottleneck
• python3-sklearn-pandas

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SciPy supplements the popular NumPy module (python-numpy package), gathering a variety of high level science and engineering modules together as a single package.

SciPy is a set of Open Source scientific and numeric tools for Python. It currently supports special functions, integration, ordinary differential equation (ODE) solvers, gradient optimization, genetic algorithms, parallel programming tools, an expression-to-C++ compiler for fast execution, and others.

• Debian Python Team
• Drew Parsons

• 1.17.1-1exp1 (experimental)
• 1.15.3-1 (trixie)
• 1.6.0-2 (bullseye)
• 1.16.3-4 (forky)
• 1.10.1-2 (bookworm)
• 1.16.3-4 (sid)
• 1.17.1 (upstream)

• 3409 regular users
• 2728 recent
• 29765 total installations (of 281236 submissions)

• Maintainer page
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• Git

• Home page
• Bugs
• Git

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SymPy is a Python library for symbolic mathematics (manipulation). It aims to become a full-featured computer algebra system (CAS) while keeping the code as simple as possible in order to be comprehensible and easily extensible. SymPy is written entirely in Python and does not require any external libraries, except optionally for plotting support.

This package contains the Python 3 version of sympy.

• Debian Science Maintainers
• Georges Khaznadar

• 1.14.0-2 (forky)
• 1.7.1-3 (bullseye)
• 1.11.1-1 (bookworm)
• 1.14.0-2 (sid)
• 1.13.3-5 (trixie)

• 11918 regular users
• 6128 recent
• 28442 total installations (of 281236 submissions)

• texmacs-bin

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SAOImage DS9 is an astronomical imaging and data visualization application. DS9 supports FITS images and binary tables, multiple frame buffers, region manipulation, and many scale algorithms and colormaps. It provides for easy communication with external analysis tasks and is highly configurable and extensible via XPA and SAMP.

All versions and platforms support a consistent set of GUI and functional capabilities.

DS9 supports advanced features such as 2-D, 3-D and RGB frame buffers, mosaic images, tiling, blinking, geometric markers, colormap manipulation, scaling, arbitrary zoom, cropping, rotation, pan, and a variety of coordinate systems.

The GUI for DS9 is user configurable. GUI elements such as the coordinate display, panner, magnifier, horizontal and vertical graphs, button bar, and color bar can be configured via menus or the command line.

• 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

• 8.6+repack-6 (sid)
• 8.4.1+repack-3 (bookworm)
• 8.6+repack-5 (trixie)
• 8.2+repack-2 (bullseye)
• 8.6+repack-6 (forky)
• 8.7 (upstream)

field

astronomy

interface

x11

role

program

science

visualisation

uitoolkit

tk

use

viewing

x11

application

• 40 regular users
• 15 recent
• 349 total installations (of 281236 submissions)

• Maintainer page
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• Git

• Home page
• Bugs
• Git

Fedora includes the predessor saoimage instead.

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GNU Screen is a terminal multiplexer that runs several separate "screens" on a single physical character-based terminal. Each virtual terminal emulates a DEC VT100 plus several ANSI X3.64 and ISO 2022 functions. Screen sessions can be detached and resumed later on a different terminal.

Screen also supports a whole slew of other features, including configurable input and output translation, serial port support, configurable logging, and multi-user support.

• Axel Beckert
• Adrian Bunk

• 4.9.1-3 (trixie)
• 4.8.0-6 (bullseye)
• 4.9.1-3.1 (forky)
• 4.9.1-3.1 (sid)
• 4.9.0-4 (bookworm)
• 5.0.1 (upstream)

hardware

input:keyboard

interface

text-mode

role

program

scope

utility

suite

gnu

uitoolkit

ncurses

works-with

software:running

• 15190 regular users
• 2099 recent
• 56211 total installations (of 281236 submissions)

• byobu
• iselect
• liquidprompt

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Find sources, such as stars and galaxies, in astronomical images. The input data files are in FITS file format, and are analyzed to compute the locations of sources, with the ability to distinguish between galaxies and stars using a neural-network technique.

• E. Bertin and S. Arnouts: SExtractor: Software for source extraction. Astronomy and Astrophysics Supplement 117:393-404 (1996) (eprint)

• Debian Astronomy Maintainers
• Ole Streicher

• 2.28.2+ds-1 (trixie)
• 2.28.2+ds-1 (forky)
• 2.28.2+ds-1 (sid)
• 2.25.0+ds-3 (bullseye)
• 2.25.0+ds-3 (bookworm)

• 90 regular users
• 63 recent
• 1094 total installations (of 281236 submissions)

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Stellarium renders 3D photo-realistic skies in real-time. With Stellarium, you really see what you can see with your eyes, binoculars or a small telescope.

Some features:

• default star catalogue with over 600 thousand stars,
• information about the brightest stars (spectral type, distance, etc.),
• downloadable star catalogue extensions, for up to 210 million stars,
• all New General Catalogue (NGC) objects,
• images of almost all Messier objects and the Milky Way,
• real time positions of the planets and their satellites,
• 13 different cultures with their constellations,
• artistic illustrations of the 88 Western constellations,
• very realistic atmosphere, sunrise and sunset,
• 7 panoramic landscapes (more can be made or downloaded from the website),
• scripting with ECMAScript,
• plug-in support: Stellarium comes with 8 plug-ins by default, including:
• artificial satellites plug-in (updated from an on-line TLE database),
• ocular simulation plug-in (shows how objects look like in a given ocular),
• Solar System editor plug-in (imports comet and asteroid data from the MPC),
• telescope control plug-in (Meade LX200 and Celestron NexStar compatible).

Stellarium should not be used for very high accurate calculation or ephemerids like eclipse predictions. However, it is the ideal program to prepare an observation evening with naked eye, binocular, or small telescope.

• Debian Astro Maintainers
• Tomasz Buchert

• 24.3-1 (trixie)
• 0.20.4-3 (bullseye)
• 0.22.2-1 (bookworm)
• 25.4-1 (forky)
• 25.4-1 (sid)

field

astronomy

hardware

opengl

interface

x11

role

program

scope

application

uitoolkit

sdl

use

learning, viewing

x11

application

• 329 regular users
• 222 recent
• 2696 total installations (of 281236 submissions)

• Maintainer page
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• Git

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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.

• E. Bertin, Y. Mellier, M. Radovich, G. Missonnier, P. Didelon and B. Morin: The TERAPIX Pipeline. 281:228 (2002)

• Debian Astronomy Maintainers
• Nilesh Patra

• 2.41.5-3 (forky)
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• 2.41.5-1 (trixie)
• 2.41.5-3 (sid)
• 2.41.4-2 (bullseye)

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ATpy is a high-level Python package providing a way to manipulate tables of astronomical data in a uniform way. It provides built-in support for NumPy recarrays and common astronomical file/database formats (FITS, VO, HDF5, and ASCII tables) with a very simple API.

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Much of ATpy’s functionality has now been incorporated into Astropy, and there is no longer active development of new features in ATpy, instead focusing efforts on Astropy.

This program enables you to draw sky charts, making use of the data in 16 catalogs of stars and nebulae. In addition the position of planets, asteroids and comets are shown.

The purpose of this program is to prepare different sky maps for a particular observation. A large number of parameters help you to choose specifically or automatically which catalogs to use, the colour and the dimension of stars and nebulae, the representation of planets, the display of labels and coordinate grids, the superposition of pictures, the condition of visibility and more. All these features make this celestial atlas more complete than a conventional planetarium.

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