774288c
 conversations held with other people, etc.)
.
774284c
Description-md5: afb1d0b09f3518f36eb67e60d3458096
.
774251,774252c
Description-md5: 1671aecb75f2c53fbe53d9d9521fb13b
Description-en: event logging framework - CLI tool
.
774223c
 conversations held with other people, etc.)
.
774219,774220c
Description-md5: bfd85e20a9015c9d67bbd73b61772545
Description-en: event logging framework - documentation
.
774204c
 conversations held with other people, etc.)
.
774200,774201c
Description-md5: 4f88f9b2286e9deb55f48966cbff894c
Description-en: event logging framework - development files
.
774185c
 conversations held with other people, etc.)
.
774181,774182c
Description-md5: f914ce0b36d6abfe0353b6b9990ff97c
Description-en: event logging framework - shared library
.
774165c
 conversations held with other people, etc.)
.
774161,774162c
Description-md5: f013ed6a20f68a21fc250885036b32f3
Description-en: event logging framework - GObject introspection data
.
752401,752411d
749102,749111d
746810a

Package: python3-veusz
Description-md5: f3373fc1ab5d5ae5dad7460cf7194682
Description-en: 2D and 3D scientific plotting application (Python interface)
 Veusz is a 2D and 3D scientific plotting and graphing package,
 designed to produce publication-ready PDF, SVG, Postscript and bitmap
 output. Veusz provides a GUI, command line and scripting interface
 (based on Python) to its plotting facilities. The plots are built
 using an object-based system to provide a consistent interface.
 .
 This package includes the Python 3 plotting module.

Package: python3-veusz.helpers
Description-md5: cbca14b6ce06f6a99951bc5bd3574016
Description-en: 2D and 3D scientific plotting application (binary modules)
 Veusz is a 2D and 3D scientific plotting and graphing package,
 designed to produce publication-ready PDF, SVG, Postscript and bitmap
 output. Veusz provides a GUI, command line and scripting interface
 (based on Python) to its plotting facilities. The plots are built
 using an object-based system to provide a consistent interface.
 .
 This package includes the architecture-specific parts of the Python 3 plotting
 module.

Package: veusz
Description-md5: 31cb071ef5dd91b209e52551b37fab22
Description-en: 2D and 3D scientific plotting application with graphical interface
 Veusz is a 2D and 3D scientific plotting and graphing package,
 designed to produce publication-ready PDF, SVG, Postscript and bitmap
 output. Veusz provides a GUI, command line and scripting interface
 (based on Python) to its plotting facilities. The plots are built
 using an object-based system to provide a consistent interface.
 .
 This package includes the main executable, documentation and examples.
.
743584,743594d
740099,740104c
Description-md5: b6a2d1f36ec2a243faacd72d92f852ba
Description-en: UKUI desktop panel component
 The ukui-panel is the taskbar component of the UKUI desktop
 environment. It provides a dock window at the screen edge with
 features including application launcher, system tray, task
 management, and system time display. It supports both classic
 and island modes and is based on the ukui-quick-framework
 plugin mechanism.

Package: ukui-panel-widgets
Description-md5: 2eed25e34e2761bd3f2cd2e877078323
Description-en: Default widgets for UKUI panel
 This package contains the default widgets that are loaded by
 the UKUI panel, including the start menu button, calendar,
 search button, separator, show desktop button, task view, and
 task manager plugins.
.
736553a
Package: astrometry-data-tycho2
Description-md5: 99975070eb7f570c758937abe5e63e86
Description-en: Astrometry.net Tycho-2 index files
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package installs all index file from the Tycho-2 catalog.

Package: astrometry-data-tycho2-07
Description-md5: d9f36469d5c10cf7a2ee0c8d789cf81b
Description-en: Astrometry.net Tycho-2 index files (22'-30')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package installs the 4107 index file from the Tycho-2 catalog
 containing skymarks of sizes 22 arcminutes to 30 arcminutes.

Package: astrometry-data-tycho2-07-bigendian
Description-md5: b347384c53cec3dd9baca1491c50bf7d
Description-en: Astrometry.net Tycho-2 big endian index files (22'-30')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the 4107 index file from the Tycho-2 catalog
 containing skymarks of sizes 22 arcminutes to 30 arcminutes. Byte order
 is big endian.

Package: astrometry-data-tycho2-07-littleendian
Description-md5: db22975d2ad3c167a716db4976c5ee5d
Description-en: Astrometry.net Tycho-2 little endian index files (22'-30')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the 4107 index file from the Tycho-2 catalog
 containing skymarks of sizes 22 arcminutes to 30 arcminutes. Byte order
 is litte endian.

Package: astrometry-data-tycho2-08
Description-md5: 6ebf515215de03fb6134b4dbaf6a393a
Description-en: Astrometry.net Tycho-2 index files (30'-44')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package installs the 4108 index file from the Tycho-2 catalog
 containing skymarks of sizes 30 arcminutes to 44 arcminutes.

Package: astrometry-data-tycho2-08-bigendian
Description-md5: 7ddacc3cd1abd6d7af6c3beabf47e436
Description-en: Astrometry.net Tycho-2 big endian index files (30'-44')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the 4108 index file from the Tycho-2 catalog
 containing skymarks of sizes 30 arcminutes to 44 arcminutes. Byte order
 is big endian.

Package: astrometry-data-tycho2-08-littleendian
Description-md5: 42010964994b0a2dfebb1295d83c7dc3
Description-en: Astrometry.net Tycho-2 little endian index files (30'-44')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the 4108 index file from the Tycho-2 catalog
 containing skymarks of sizes 30 arcminutes to 44 arcminutes. Byte order
 is litte endian.

Package: astrometry-data-tycho2-09
Description-md5: bb3384e7a320a9d505e8131c46a66459
Description-en: Astrometry.net Tycho-2 index files (44'-60')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package installs the 4109 index file from the Tycho-2 catalog
 containing skymarks of sizes 44 arcminutes to 60 arcminutes.

Package: astrometry-data-tycho2-09-bigendian
Description-md5: 675943063ea1d46a935b87f521cd00a6
Description-en: Astrometry.net Tycho-2 big endian index files (44'-60')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the 4109 index file from the Tycho-2 catalog
 containing skymarks of sizes 44 arcminutes to 60 arcminutes. Byte order
 is big endian.

Package: astrometry-data-tycho2-09-littleendian
Description-md5: f8cd18d33713b9060780fec8aa32397c
Description-en: Astrometry.net Tycho-2 little endian index files (44'-60')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the 4109 index file from the Tycho-2 catalog
 containing skymarks of sizes 44 arcminutes to 60 arcminutes. Byte order
 is litte endian.

Package: astrometry-data-tycho2-10-19
Description-md5: 4862991080b5b1e2161dc34972e34393
Description-en: Astrometry.net Tycho-2 index files (60'-2000')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package installs the 4110-4119 index file from the Tycho-2 catalog
 containing skymarks of sizes 60 arcminutes to 2000 arcminutes.

Package: astrometry-data-tycho2-10-19-bigendian
Description-md5: fcb60b33260c92717e3b86ec592db671
Description-en: Astrometry.net Tycho-2 big endian index files (60'-2000')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the 4110-4119 index file from the Tycho-2 catalog
 containing skymarks of sizes 60 arcminutes to 2000 arcminutes. Byte order
 is big endian.

Package: astrometry-data-tycho2-10-19-littleendian
Description-md5: 5d7136d5039c87bbe63cff8c6f9c7ea5
Description-en: Astrometry.net Tycho-2 little endian index files (60'-2000')
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the 4110-4119 index file from the Tycho-2 catalog
 containing skymarks of sizes 60 arcminutes to 2000 arcminutes. Byte order
 is litte endian.

.
731952,731968d
703919a
Package: libsynfig-dev
Description-md5: 2a9b378cf611313a54c64ddcec63afaa
Description-en: synfig library development files
 synfig is a vector based 2D animation package. It is designed to be
 capable of producing feature-film quality animation.
 .
 This package contains headers and other files needed to develop
 applications using the shared library and plugin modules.

Package: libsynfig0t64
Description-md5: 954185cac03f0fac6f9abd49cdf51ec9
Description-en: render library and plugins for synfig 2D animation
 synfig is a vector based 2D animation package. It is designed to be
 capable of producing feature-film quality animation.
 .
 This package contains the shared library and plugin modules for it.

Package: synfig
Description-md5: edb4e9874f19866be4284f8f169935d0
Description-en: vector-based 2D animation renderer
 synfig is a vector based 2D animation renderer. It is designed to be
 capable of producing feature-film quality animation.
 .
 This package contains the command-line renderer, for the GUI animation
 editor, please install synfigstudio.

Package: synfig-examples
Description-md5: fa54ce4b55141c30ce1cb2e4ffc7c076
Description-en: synfig animation examples
 synfig is a vector based 2D animation renderer. It is designed to be
 capable of producing feature-film quality animation.
 .
 This package contains several examples of synfig animations and stills.

Package: python3-synphot
Description-md5: 438200a4a33eff401a116d89e10bf351
Description-en: Simulate photometric data and spectra in astronomy
 Synphot simulates photometric data and spectra, observed or otherwise.
 It can incorporate external filters, spectra, and data. One can also use
 a pre-defined standard star (Vega), bandpass, or extinction law.
 Furthermore, it allows one to:
 .
  * Construct complicated composite spectra using different models.
  * Simulate observations.
  * Compute photometric properties such as count rate, effective
    wavelength, and effective stimulus.
  * Manipulate a spectrum; e.g., applying redshift or normalize it to a
    given flux value in a given bandpass.
  * Sample a spectrum at given wavelengths.
  * Plot a quick-view of a spectrum.
  * Perform repetitive operations such as simulating the observations of
    multiple type of sources through multiple bandpasses.

.
703453a
Package: python-symmetrize-doc
Description-md5: 01f3eab10f3c45e0c824159452705b81
Description-en: Symmetrization and centering of 2D pattern - documentation
 Symmetrization of 2D pattern using nonrigid landmark registration
 with symmetry constraints. Implemented registration methods include
 projective transform and thin plate spline. Details are given in the
 publication associated with the package.
 .
 This package contains the documentation.

Package: python3-symmetrize
Description-md5: b5c862dde5f90ee37bed0ce3f7af95a0
Description-en: Symmetrization and centering of 2D pattern
 Symmetrization of 2D pattern using nonrigid landmark registration
 with symmetry constraints. Implemented registration methods include
 projective transform and thin plate spline. Details are given in the
 publication associated with the package.
 .
 This package contains the Python 3 module.

.
697154a
Package: python3-stsci.tools
Description-md5: aa75686ebda40de20b51e2fce402bd84
Description-en: Miscellaneous Python tools from STScI
 This package provides a selection of tools for FITS and WCS handling,
 image handling, and data analysis, used by other STScI packages; mainly
 by Pyraf.

.
696189c
Package: libstopt7
.
688993c
 This utility allows you to use the Speedtest.net service from the
 command line.
.
688986,688991c
Description-md5: 888d0651505664258c3520e3dca98297
Description-en: Command line interface for testing internet bandwidth using speedtest.net
 Speedtest.net is a webservice that allows you to test your broadband
 connection by downloading a file from one of many Speedtest.net
 servers from around the world.
.
688983c
 Allows you to use the Speedtest.net service via pure Go APIs.
.
688976,688981c
Description-md5: 00e9174b5e219d3669c9c46b18c77ede
Description-en: Go APIs to Test Internet Speed using speedtest.net
 Speedtest.net is a webservice that allows you to test your broadband
 connection by downloading a file from one of many Speedtest.net
 servers from around the world.
.
686777,686810d
685230a
Package: python3-sncosmo
Description-md5: 699544ee184aea05245dcad2dcb8824c
Description-en: Python library for high-level supernova cosmology analysis
 SNCosmo synthesizes supernova spectra and photometry from SN models,
 and has functions for fitting and sampling SN model parameters given
 photometric light curve data. It offers fast implementations of
 several commonly used extinction laws and can be used to construct SN
 models that include dust. The SNCosmo library includes supernova
 models such as SALT2, MLCS2k2, Hsiao, Nugent, PSNID, SNANA and Whalen
 models, as well as a variety of built-in bandpasses and magnitude
 systems, and provides convenience functions for reading and writing
 peculiar data formats used in other packages. The library is
 extensible, allowing new models, bandpasses, and magnitude systems to
 be defined using an object-oriented interface.

.
682179a
Package: python3-skyfield
Description-md5: 2e86bad342fb03842886e36155c95614
Description-en: Elegant astronomy for Python
 Skyfield is a pure-Python astronomy package that is compatible with
 both Python 3 and makes it easy to generate high precision
 research-grade positions for planets and Earth satellites.
 .
 Skyfield computes positions for the stars, planets, and satellites in
 orbit around the Earth. Its results should agree with the positions
 generated by the United States Naval Observatory and their
 Astronomical Almanac to within 0.0005 arcseconds (which equals half a
 “mas” or milliarcsecond).

.
679043a
Package: shutter
Description-md5: 02af88a8a1ab9d18f357823a2612e22a
Description-en: feature-rich screenshot program
 Shutter is a feature-rich screenshot program. You can take a
 screenshot of a specific area, window, your whole screen, or even of
 a website - apply different effects to it, draw on it to highlight
 points, and then upload to an image hosting site, all within one
 window.
 .
 Features:
    * take a screenshot of your complete desktop, a rectangular area
    * take screenshot directly or with a specified delay time
    * save the screenshots to a specified directory and name them in a
      convenient way (using special wild-cards)
    * Shutter is fully integrated into the GNOME Desktop (TrayIcon etc.)
    * generate thumbnails directly when you are taking a screenshot
      and set a size level in %
    * Shutter session collection
          o keep track of all screenshots during session
          o copy screeners to clipboard
          o print screenshots
          o delete screenshots
          o rename your file
    * upload your files directly to Image-Hosters (e.g. imgur.com), retrieve
      all the needed links and share them with others
    * edit your screenshots directly using the embedded drawing tool

.
676610a
Package: libsep-dev
Description-md5: e58880dbef1fb83bec57783260797039
Description-en: C library for source extraction and photometry (development files)
 SEP makes the core algorithms of Source Extractor available as a
 library of stand-alone functions and classes. These operate
 directly on in-memory arrays (no FITS files or configuration files).
 The code is derived from the Source Extractor code base (written in
 C) and aims to produce results compatible with Source Extractor
 whenever possible.

Package: libsep0
Description-md5: 605beb4fc7345849f097c7ce95815d09
Description-en: C library for source extraction and photometry
 SEP makes the core algorithms of Source Extractor available as a
 library of stand-alone functions and classes. These operate
 directly on in-memory arrays (no FITS files or configuration files).
 The code is derived from the Source Extractor code base (written in
 C) and aims to produce results compatible with Source Extractor
 whenever possible.
 .
 This package contains the shared library.

Package: python3-sep
Description-md5: dff988dde1cb0cc9c27bb37659b6662d
Description-en: Python library for source extraction and photometry
 SEP makes the core algorithms of Source Extractor available as a
 library of stand-alone functions and classes. These operate
 directly on in-memory arrays (no FITS files or configuration files).
 The code is derived from the Source Extractor code base (written in
 C) and aims to produce results compatible with Source Extractor
 whenever possible.
 .
 This Python module that wraps the C library in a Pythonic API. The
 Python wrapper operates on NumPy arrays.

.
674488,674499d
670421,670426d
668249,668250c
 Source code for Debianized Rust crate "write-json"
.
668247c
Description-md5: ca29a291d514ae4cc20674747cbab03b
.
667660,667661c
 Source code for Debianized Rust crate "vm-superio"
.
667658c
Description-md5: dd4646e0f6c492e8c58cc19ca159c2db
.
667598a
Package: librust-virtio-vsock-dev
Description-md5: b134c88d58aaf75490bf4c251d5c864e
Description-en: Virtio vsock device implementation - Rust source code
 Source code for Debianized Rust crate "virtio-vsock"

.
666667,666668c
 Source code for Debianized Rust crate "ucd-util"
.
666665c
Description-md5: 8f8d5405d17f0ef2e7875c17baae54d5
.
666656,666657c
 Source code for Debianized Rust crate "ucd-parse"
.
666654c
Description-md5: da2bddbe546683b5520952f93aa63b8d
.
666633a
Package: u8loc
Description-md5: 935be2578be42e93144be3f15fa48371
Description-en: Run child processes in a UTF-8-capable locale
 This package contains the following binaries built from the Rust crate
 "u8loc":
  - u8loc

.
660215,660216c
 quanta is a high-speed timing library,
 useful for getting the current time very quickly,
.
660213c
Description-md5: 44c93041b45afd47720d663a104add73
.
659460,659461c
 Source code for Debianized Rust crate "predicates-core"
.
659458c
Description-md5: d37c3c1f214bd40103fa286a45178dc0
.
658399,658400c
 Source code for Debianized Rust crate "partition-identity"
.
658397c
Description-md5: fb7b9cd1e368d42886137587724cbd74
.
658174a

Package: librust-p9-wire-format-derive-dev
Description-md5: 7b1c8ceb630a1ca66c3daf7878c7be69
Description-en: Supporting proc-macro for the `p9` crate - Rust source code
 Source code for Debianized Rust crate "p9_wire_format_derive"
.
656884,656885c
 Source code for Debianized Rust crate "mutate_once"
.
656882c
Description-md5: 84ef419e944830d472c8484ab51ea4b1
.
653441a
Package: librust-icu-provider-registry-dev
Description-md5: 56f1dc3d8657895ec8fb4041fc1a94ed
Description-en: Registry of all ICU4X data markers - Rust source code
 Source code for Debianized Rust crate "icu_provider_registry"

.
653436a
Package: librust-icu-provider-export-dev
Description-md5: 4bbc58a7ce7f54d72e1b13d9a043aace
Description-en: Generate data for ICU4X DataProvider - Rust source code
 Source code for Debianized Rust crate "icu_provider_export"

.
653431a
Package: librust-icu-provider-baked-dev
Description-md5: 54c36e5e6e6a2c7092f4f65f1dcd483e
Description-en: Tooling for the ICU4X baked data provider - Rust source code
 Source code for Debianized Rust crate "icu_provider_baked"

.
650892,650893c
 Source code for Debianized Rust crate "fragile"
.
650890c
Description-md5: 406934aa316e9d4001f22f773516f44a
.
649346a
Package: librust-dtor-dev
Description-md5: 3e83b78af8757bae11dca6d59ea5a76b
Description-en: Global, no_std-compatible destructors for all platforms that run after main (like C/C++ __attribute__((destructor))) - Rust source code
 Source code for Debianized Rust crate "dtor"

.
648692,648693c
 Source code for Debianized Rust crate "deser-hjson"
.
648690c
Description-md5: 2544abb43b18efd0ad00c4c8ea6400d4
.
648270,648271c
 Source code for Debianized Rust crate "data-encoding-macro-internal"
.
648268c
Description-md5: 1649644f0ef1eaddb3c82fec98ba488b
.
648264,648265c
 Source code for Debianized Rust crate "data-encoding-macro"
.
648262c
Description-md5: b98643cec097de4c1f2b55e46ec13327
.
647876,647879c
Description-md5: 329cdcd390bc497d932299cb292327c0
Description-en: Constant-time base64, base32, and hex codecs reimplemented in Rust - Rust source code
 Source code for Debianized Rust crate "ct-codecs"
.
646624,646625c
Description-md5: f222211d3e79f6d47a6bdc627fea89d3
Description-en: Character encoding decoding for email - Rust source code
.
644108a
Package: librust-askama-parser-dev
Description-md5: f8908298bd0ed0d7bdb3fafc343eae18
Description-en: Parser for Askama templates - Rust source code
 Source code for Debianized Rust crate "askama_parser"

.
639459a
Package: ruby-rake-compiler-dock
Description-md5: 916a71dcb9ef3d28d7442e4dcea7a039
Description-en: cross compiler environment for building binary gems
 Use rake-compiler-dock to enter an interactive shell session or add a task to
 your Rakefile to automate your cross build.

.
639003a
Package: ruby-protocol-multipart
Description-md5: 0fdaa0fe7a291a2ff2b3c95230cdf966
Description-en: Provides abstractions to handle the multipart format
 This Ruby gem provides abstractions to handle the multipart format.

.
634648,634838d
620344,620357d
615937,615969d
615163a
Package: python3-radio-beam
Description-md5: a6b84072dec849b373864b05a0874a71
Description-en: Python Tools for Radio Beam IO and Manipulation
 Radio Beam is a simple toolkit for reading beam information from FITS
 headers and manipulating beams. Some example applications include
 Convolution/deconvolution and Unit conversion (Jy to/from K).

.
614870,614904d
613864,613865c
Description-md5: 43243c34459c64b022d09f8e2f7d4efe
Description-en: 'SVG' Graphics Device
.
610262,610263c
 and 'attributes'.
.
610253,610260c
Description-md5: 7aab09d6552fd8aa436c635f383613b4
Description-en: Straightforward 'NetCDF' Metadata
 Extract metadata from 'NetCDF' data sources, these can be files, file handles
 or servers. This package leverages and extends the lower level functions
 of the 'RNetCDF' package providing a consistent set of functions that all
 return data frames. We introduce named concepts of 'grid', 'axis' and 'source'
 which are all meaningful entities without formal definition in the 'NetCDF'
 library <https://www.unidata.ucar.edu/software/netcdf>. 'RNetCDF' matches the
.
610125,610132c
Description-md5: 6ad755243ffe870e292283c652235589
Description-en: Visualizations of Paired Comparisons
 Convert a logical vector or a vector of p-values or a correlation, difference,
 or distance matrix into a display identifying the pairs for which the
 differences were not significantly different. Designed for use in conjunction
 with the output of functions like TukeyHSD, dist (stats), simint, simtest,
 csimint, csimtest (multcomp), friedmanmc, kruskalmc (pgirmess).
.
607924,607925c
 Generalized Estimation Equation solver.
.
607922c
Description-md5: ba153622ee7243047e3623954026ac2e
.
592803a
Package: python3-pyvkfft
Description-md5: 31fc396bb54935aaf6e49e8057357fdf
Description-en: Binding to the OpenCL backends of VkFFT - Python3
 pyvkfft offers a simple python interface to the CUDA and OpenCL
 backends of VkFFT, compatible with pyCUDA, CuPy and pyOpenCL.
 .
 This package installs the library for Python 3 and includes the
 OpenCL backend. The CUDA backend is available in the
 python3-pyvkfft-cuda package.

Package: python3-pyvkfft-doc
Description-md5: 392d23be90a8b78de4ed29455731c673
Description-en: Binding to the backends of VkFFT - Documentation
 pyvkfft offers a simple python interface to the CUDA and OpenCL
 backends of VkFFT, compatible with pyCUDA, CuPy and pyOpenCL.
 .
 This is the common documentation package.

.
592289a
Package: idle-python3.15
Description-md5: fd104146cc6fcd2fe1edfc565a758b51
Description-en: IDE for Python (v3.15) using Tkinter
 IDLE is an Integrated Development Environment for Python (v3.15).
 IDLE is written using Tkinter and therefore quite platform-independent.

Package: libpython3.15
Description-md5: 084f7a1bef0aa849039081e3d46630b9
Description-en: Shared Python runtime library (version 3.15)
 Python is a high-level, interactive, object-oriented language. Its 3.15 version
 includes an extensive class library with lots of goodies for
 network programming, system administration, sounds and graphics.
 .
 This package contains the shared runtime library, normally not needed
 for programs using the statically linked interpreter.

Package: libpython3.15-dbg
Description-md5: e89d795e45255a3405310f25da06a9a6
Description-en: Debug Build of the Python Interpreter (version 3.15)
 The package holds two things:
 .
 - Extensions for a Python interpreter configured with --pydebug.
 - Debug information for standard python extensions.
 .
 See the README.debug for more information.

Package: libpython3.15-dev
Description-md5: 3455ac777950eb14a7b3526105189993
Description-en: Header files and a static library for Python (v3.15)
 Header files, a static library and development tools for building
 Python (v3.15) modules, extending the Python interpreter or embedding
 Python (v3.15) in applications.
 .
 Maintainers of Python packages should read README.maintainers.
 .
 This package contains development files. It is normally not
 used on it's own, but as a dependency of python3.15-dev.

Package: libpython3.15-minimal
Description-md5: 74f98817c8d94cc66acd9a098a2a5327
Description-en: Minimal subset of the Python language (version 3.15)
 This package contains some essential modules. It is normally not
 used on it's own, but as a dependency of python3.15-minimal.

Package: libpython3.15-stdlib
Description-md5: 61bba94b532ebcfd90fd3d3f5d30894e
Description-en: Interactive high-level object-oriented language (standard library, version 3.15)
 Python is a high-level, interactive, object-oriented language. Its 3.15 version
 includes an extensive class library with lots of goodies for
 network programming, system administration, sounds and graphics.
 .
 This package contains Python 3.15's standard library. It is normally not
 used on its own, but as a dependency of python3.15.

Package: libpython3.15-testsuite
Description-md5: d0d2e45a2e0edae7b84504406cb3043c
Description-en: Testsuite for the Python standard library (v3.15)
 The complete testsuite for the Python standard library.  Note that
 a subset is found in the libpython3.15-stdlib package, which should
 be enough for other packages to use (please do not build-depend
 on this package, but file a bug report to include additional
 testsuite files in the libpython3.15-stdlib package).

Package: python3.15
Description-md5: d89554b8c849a68718387e3138457adc
Description-en: Interactive high-level object-oriented language (version 3.15)
 Python is a high-level, interactive, object-oriented language. Its 3.15 version
 includes an extensive class library with lots of goodies for
 network programming, system administration, sounds and graphics.

Package: python3.15-dbg
Description-md5: baf192472435916b3c4356cd66ce8859
Description-en: Debug Build of the Python Interpreter (version 3.15)
 The package holds two things:
 .
 - A Python interpreter configured with --pydebug. Dynamically loaded modules
   are searched as <foo>_d.so first. Third party extensions need a separate
   build to be used by this interpreter.
 - Debug information for standard python interpreter and extensions.
 .
 See the README.debug for more information.

Package: python3.15-dev
Description-md5: 733fb20f8dc5d0cc8dd1e3b14c96066e
Description-en: Header files and a static library for Python (v3.15)
 Header files, a static library and development tools for building
 Python (v3.15) modules, extending the Python interpreter or embedding
 Python (v3.15) in applications.
 .
 Maintainers of Python packages should read README.maintainers.

Package: python3.15-doc
Description-md5: 2e70d35e8ab10821a8def59a146b6250
Description-en: Documentation for the high-level object-oriented language Python (v3.15)
 These is the official set of documentation for the interactive high-level
 object-oriented language Python (v3.15). All documents are provided
 in HTML format. The package consists of ten documents:
 .
   * What's New in Python3.15
   * Tutorial
   * Python Library Reference
   * Macintosh Module Reference
   * Python Language Reference
   * Extending and Embedding Python
   * Python/C API Reference
   * Installing Python Modules
   * Documenting Python
   * Distributing Python Modules

Package: python3.15-examples
Description-md5: be13d3b15820fe9b7d4e07269a147ff8
Description-en: Examples for the Python language (v3.15)
 Examples, Demos and Tools for Python (v3.15). These are files included in
 the upstream Python distribution (v3.15).

Package: python3.15-full
Description-md5: 5f5ed9ebb20d93c6d8522371f0130fb2
Description-en: Python Interpreter with complete class library (version 3.15)
 Python, the high-level, interactive object oriented language,
 includes an extensive class library with lots of goodies for
 network programming, system administration, sounds and graphics.
 .
 This package is a dependency package, which depends on the full
 standard library of Python for Python developers. Including modules
 used only at build-time, such as venv, and modules with complex
 dependencies, such as tk and IDLE. All batteries included.
 .
 According to the Debian Python policy, this package must not be used in
 build dependencies, dependencies and recommendations.

Package: python3.15-gdbm
Description-md5: ee57cf402d581b29e8b29cfc8a6d8d64
Description-en: GNU dbm database support for Python (v3.15)
 GNU dbm database module for Python. Install this if you want to
 create or read GNU dbm database files with Python.

Package: python3.15-minimal
Description-md5: 36686d9ab3881a32b0eeaf3eda8c5a9b
Description-en: Minimal subset of the Python language (version 3.15)
 This package contains the interpreter and some essential modules.  It can
 be used in the boot process for some basic tasks.
 See /usr/share/doc/python3.15-minimal/README.Debian for a list of the modules
 contained in this package.

Package: python3.15-nopie
Description-md5: 716ac16f4a608c9ef1e918419ab6fb3b
Description-en: Python interpreter linked without PIE (version 3.15)
 This package contains the interpreter not built as position independent
 executable. This interpreter is diverting the python3.15 executable, and making
 the interpreter built with PIE available as python3.15-pie.

Package: python3.15-tk
Description-md5: c7f872430fda3141b3001d69be719498
Description-en: Tkinter - Writing Tk applications with Python (v3.15)
 A module for writing portable GUI applications with Python (v3.15) using Tk.
 Also known as Tkinter.

Package: python3.15-venv
Description-md5: 4d3a2f5687f028e9a46d068f6ac7899c
Description-en: Interactive high-level object-oriented language (pyvenv binary, version 3.15)
 Python is a high-level, interactive, object-oriented language. Its 3.15 version
 includes an extensive class library with lots of goodies for
 network programming, system administration, sounds and graphics.
 .
 This package contains the pyvenv-3.15 binary.

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Package: python-salib-doc
Description-md5: a5b185a453af71063cdd058fbf1b8a1f
Description-en: Sensitivity Analysis Library (Documentation)
 SALib is an open source library written in Python for performing sensitivity
 analyses. SALib provides a decoupled workflow, meaning it does not directly
 interface with the mathematical or computational model. Instead, SALib is
 responsible for generating the model inputs, using one of the sample
 functions, and computing the sensitivity indices from the model outputs, using
 one of the analyze functions. SALib provides several sensitivity analysis
 methods, such as Sobol, Morris, and FAST.
 .
 This package contains the documentation.

Package: python3-salib
Description-md5: f26df6a6b9142385dbe2509fa611b2ed
Description-en: Sensitivity Analysis Library (Python3 version)
 SALib is an open source library written in Python for performing sensitivity
 analyses. SALib provides a decoupled workflow, meaning it does not directly
 interface with the mathematical or computational model. Instead, SALib is
 responsible for generating the model inputs, using one of the sample
 functions, and computing the sensitivity indices from the model outputs, using
 one of the analyze functions. SALib provides several sensitivity analysis
 methods, such as Sobol, Morris, and FAST.
 .
 This package contains the Python 3 version of the library.

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Package: python3-pyvips
Description-md5: 6b5157365e9741f688f6577d406c96ec
Description-en: Python binding for the libvips image processing library
 pyvips is a Python binding for libvips, a demand-driven image processing
 library designed for speed and low memory use.
 .
 This package provides the Python 3 module.

Package: python3-pyvips-doc
Description-md5: 535eebe69649242a4f2117c415a535c0
Description-en: Python binding for the libvips image processing library (doc)
 pyvips is a Python binding for libvips, a demand-driven image processing
 library designed for speed and low memory use.
 .
 This package contains the HTML documentation for pyvips.

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Package: python3-opentelemetry-configuration
Description-md5: 90c76ff82a098ad0ec853ab4056120c4
Description-en: OpenTelemetry Python Declarative Configuration
 OpenTelemetry is an observability framework – an API, SDK, and tools that are
 designed to aid in the generation and collection of application telemetry
 data such as metrics, logs, and traces.
 .
 This package implements the OpenTelemetry declarative configuration
 specification <https://opentelemetry.io/docs/specs/otel/configuration/> for
 the Python SDK. It parses a YAML or JSON configuration file (or
 programmatically-constructed configuration model) into typed dataclasses and
 applies the result to the global SDK providers.
 .
 Note that this libarary is marked by upstream as *experimental*! The API
 surface, type names, and behaviour may change between minor versions. Pin
 a specific version in production.

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Package: python3-mistral-common
Description-md5: f996e7f5bca564a671df37d45328c49e
Description-en: Official inference library for pre-processing of Mistral models
 Mistral-common is a library of common utilities for Mistral AI. It is notably
 used to convert LLMs in Mistral-specific format to the GGUF file format used
 for inference by llama.cpp.

Package: python3-mistral-common-doc
Description-md5: 5e3be831fa95717fd0ed6263da63cfce
Description-en: Official inference library for pre-processing of Mistral models (docs)
 Mistral-common is a library of common utilities for Mistral AI. It is notably
 used to convert LLMs in Mistral-specific format to the GGUF file format used
 for inference by llama.cpp.
 .
 This package provides the documentation of the Python module.

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Package: python-drizzle-doc
Description-md5: 3c110b47e3e3368fbff093fdfa4e132a
Description-en: Dithered image combination for Python (API documentation)
 The drizzle library is a Python package for combining dithered images
 into a single image. This library is derived from code used in
 drizzlepac. Like drizzlepac, most of the code is implemented in the C
 language. The biggest change from drizzlepac is that this code passes
 an array that maps the input to output image into the C code, while
 the drizzlepac code computes the mapping by using a Python
 callback. Switching to using an array allowed the code to be greatly
 simplified.
 .
 This package contains the API documentation.

Package: python-drizzle-testdata
Description-md5: 84c1e740cf54086ef87d64b82bb1eea5
Description-en: Dithered image combination for Python (Test data)
 The drizzle library is a Python package for combining dithered images
 into a single image. This library is derived from code used in
 drizzlepac. Like drizzlepac, most of the code is implemented in the C
 language. The biggest change from drizzlepac is that this code passes
 an array that maps the input to output image into the C code, while
 the drizzlepac code computes the mapping by using a Python
 callback. Switching to using an array allowed the code to be greatly
 simplified.
 .
 This package contains the data required for the unit tests.

Package: python3-drizzle
Description-md5: d641a747bf69c9589b161bdb2dc9b59d
Description-en: Dithered image combination for Python
 The drizzle library is a Python package for combining dithered images
 into a single image. This library is derived from code used in
 drizzlepac. Like drizzlepac, most of the code is implemented in the C
 language. The biggest change from drizzlepac is that this code passes
 an array that maps the input to output image into the C code, while
 the drizzlepac code computes the mapping by using a Python
 callback. Switching to using an array allowed the code to be greatly
 simplified.

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Package: python3-cpl
Description-md5: 6b7b644022ad3042621e17acb7ab2833
Description-en: Control pipeline recipes from the ESO (Python3)
 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 astropy fits 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.

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Package: python3-calendra
Description-md5: 740cb9d4b6e1c61ebed23c15a3d8766c
Description-en: Worldwide holidays and workdays computational toolkit (Python3 version)
 Calendra is a Python module that offers classes able to handle calendars, list
 legal / religious holidays and gives working-day-related computation functions.
 It is a fork of Workalendar designed to be more extensible and introspectable,
 adding interfaces where Workalendar is philosophically opposed for the sake of
 simplicity.
 .
 What can Calendra do that Workalendar cannot?
  * Provides descriptions for holidays for the "day indicated" for each Holiday
    (such as '3rd Monday in August').
  * Keeps distinct the indicated and observed dates for Holidays, such that it's
    possible to determine on what day a given holiday is observed.
  * Allows the number of Holidays in a calendar year to be counted.
    Consolidates observance logic in the core code rather than requiring each
    calendar implementation to implement its own.
 .
 This package contains the Python 3 version of the library.

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Package: python3-astropy-affiliated
Description-md5: fc39334b803eef0601d9c0232d24195b
Description-en: Collection of all astropy affiliated packages
 A major part of the Astropy project is the concept of “Affiliated
 Packages”. An affiliated package is an astronomy-related Python
 package that is not part of the astropy core package, but has
 requested to be included as part of the Astropy project’s
 community. These packages are expressing an interest in Astropy’s
 goals of improving reuse, interoperability, and interface standards
 for Python astronomy and astrophysics packages.
 .
 This metapackage installs all affiliated packages.

Package: python3-astropy-coordinated
Description-md5: a871322ec79ff25fe0904dd15b6a0e2b
Description-en: Collection of all astropy coordinated packages
 Coordinated packages are Astropy enhancing packages that are
 maintained by the Astropy Project as a whole. In practice this means
 the Astropy coordination committee has administrative control of a
 coordinated package repository (delegated to the maintainers), and
 that maintainers of these packages have formal roles in the Astropy
 Project. In some cases these are packages identified by the core team
 as needing development separate from the core (either they are
 experimental or problem space-focused), while others started as
 affiliated packages but have become so important to the ecosystem
 that they grew to become coordinated.
 .
 This metapackage installs all coordinated packages.

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Package: asdftool
Description-md5: eb66e08346889fcd227d11ac2648fa8d
Description-en: Command line tool to manipulate ASDF scientific data files
 ASDF (Advanced Scientific Data Format) is a proposed
 next generation interchange format for scientific data. ASDF aims to
 exist in the same middle ground that made FITS so successful, by
 being a hybrid text and binary format: containing human editable
 metadata for interchange, and raw binary data that is fast to load
 and use. Unlike FITS, the metadata is highly structured and is
 designed up-front for extensibility.
 .
 This package contains the asdf command line tool.

Package: python-asdf-doc
Description-md5: e9d5c1f1266604458dbade9c436a7efc
Description-en: Python library for the Advanced Scientific Data Format (documentation)
 ASDF (Advanced Scientific Data Format) is a proposed
 next generation interchange format for scientific data. ASDF aims to
 exist in the same middle ground that made FITS so successful, by
 being a hybrid text and binary format: containing human editable
 metadata for interchange, and raw binary data that is fast to load
 and use. Unlike FITS, the metadata is highly structured and is
 designed up-front for extensibility.
 .
 This package contains the API documentation.

Package: python3-asdf
Description-md5: 5de6519bea5b5e62a795a426d96b1ab8
Description-en: Python 3 library for the Advanced Scientific Data Format
 ASDF (Advanced Scientific Data Format) is a proposed
 next generation interchange format for scientific data. ASDF aims to
 exist in the same middle ground that made FITS so successful, by
 being a hybrid text and binary format: containing human editable
 metadata for interchange, and raw binary data that is fast to load
 and use. Unlike FITS, the metadata is highly structured and is
 designed up-front for extensibility.
 .
 This is the Python 3 package.

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Package: python3-amcrest
Description-md5: fbc934fbf5587e25c9ed789204d9fe51
Description-en: interface to Amcrest and Dahua camera HTTP APIs
 This library provides access to the HTTP SDK API exposed by Amcrest cameras
 and related Dahua firmware devices.
 .
 It talks directly to network cameras and network video recorders over their
 HTTP endpoints. It can query device and software information, retrieve
 snapshots, capture audio, record real-time video streams, and send pan, tilt,
 and zoom control commands where the device offers those functions.
 .
 The package also includes command-line and text user interface tools for
 working with configured cameras.

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Package: python3-pytest-asdf-plugin
Description-md5: 029495645390811da7631dfd8f5b3725
Description-en: Pytest plugin for testing ASDF schemas
 ASDF (Advanced Scientific Data Format) is a proposed
 next generation interchange format for scientific data. ASDF aims to
 exist in the same middle ground that made FITS so successful, by
 being a hybrid text and binary format: containing human editable
 metadata for interchange, and raw binary data that is fast to load
 and use. Unlike FITS, the metadata is highly structured and is
 designed up-front for extensibility.
 .
 This package provides a Pytest plugin for testing these schemas.

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Package: python3-pysynphot
Description-md5: 083a8874d24f3f5c160cd0b1103fabbf
Description-en: Python Synthetic Photometry Utilities
 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.

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Package: pyscanfcs
Description-md5: a77c372599720e7642e3f34c61aec6d5
Description-en: scientific tool for perpendicular line scanning FCS
 When a membrane is scanned perpendicularly to its surface,
 the fluorescence signal originating from the membrane itself
 must be separated from the signal of the surrounding medium for
 an FCS analysis. PyScanFCS interactively extracts the fluctuating
 fluorescence signal from such measurements and applies a multiple-tau
 algorithm. The obtained correlation curves can be evaluated using PyCorrFit.
 .
 Package provides the Python module pyscanfcs and its graphical user interface.
 The graphical user interface is written in wxPython.

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Package: python-pyregion-doc
Description-md5: 887ecffb0191281da87320dd0e914e28
Description-en: Python module to parse ds9 region files (documentation)
 Pyregion is a Python module to parse ds9 region files. It also supports ciao
 region files.
 .
 This is the common documentation package.

Package: python3-pyregion
Description-md5: 45e7a0d549baa48683cca5702aeb422d
Description-en: Python module to parse ds9 region files (Python 3)
 Pyregion is a Python module to parse ds9 region files. It also supports ciao
 region files.
 .
 This is the Python 3 version of the package.

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Package: python3-pyraf
Description-md5: f7421082fca06089d04b1a287a5eca5d
Description-en: Python interface for IRAF
 PyRAF is a command language for running IRAF tasks in a Python like
 environment. It works very similar to IRAF CL, but has been updated
 to allow such things as importing Python modules, GUI parameter
 editing and help. It can be imported into Python allowing you to run
 IRAF commands from within a larger script.

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Package: python-pyopencl-doc
Description-md5: 0b1f9cb9c27d466dca495ad8192d962e
Description-en: module to access OpenCL parallel computation API (documentation)
 PyOpenCL lets you access the OpenCL parallel computation API from
 Python. Here's what sets PyOpenCL apart:
  * Object cleanup tied to lifetime of objects. This idiom, often called
    RAII in C++, makes it much easier to write correct, leak- and
    crash-free code.
  * Completeness. PyOpenCL puts the full power of OpenCL’s API at your
    disposal, if you wish.
  * Convenience. While PyOpenCL's primary focus is to make all of OpenCL
    accessible, it tries hard to make your life less complicated as it
    does so--without taking any shortcuts.
  * Automatic Error Checking. All OpenCL errors are automatically
    translated into Python exceptions.
  * Speed. PyOpenCL’s base layer is written in C++, so all the niceties
    above are virtually free.
  * Helpful, complete documentation and a wiki.
  * Liberal licensing (MIT).
 .
 This package contains HTML documentation and example scripts.

Package: python3-pyopencl
Description-md5: 7a31e9ce8f06c38705703f009d69b248
Description-en: Python 3 module to access OpenCL parallel computation API
 PyOpenCL lets you access the OpenCL parallel computation API from
 Python. Here's what sets PyOpenCL apart:
  * Object cleanup tied to lifetime of objects. This idiom, often called
    RAII in C++, makes it much easier to write correct, leak- and
    crash-free code.
  * Completeness. PyOpenCL puts the full power of OpenCL’s API at your
    disposal, if you wish.
  * Convenience. While PyOpenCL's primary focus is to make all of OpenCL
    accessible, it tries hard to make your life less complicated as it
    does so--without taking any shortcuts.
  * Automatic Error Checking. All OpenCL errors are automatically
    translated into Python exceptions.
  * Speed. PyOpenCL’s base layer is written in C++, so all the niceties
    above are virtually free.
  * Helpful, complete documentation and a wiki.
  * Liberal licensing (MIT).
 .
 This package contains Python 3 modules.

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Package: pymoctool
Description-md5: 0daaa74532b1d5c29ed351c4d41979bb
Description-en: Python Multi-Order Coverage maps tool for Virtual Observatory
 'pymoctool' is a command-line Python-based library for manipulating
 Multi-Order Coverage maps (MOCs).
 .
 Frequently astronomical survey catalogues or images are sparse and
 cover only a small part of the sky.  In a Multi-Order Coverage map
 the extent of data in a particular dataset is cached as a
 pre-calculated mask image.  The hierarchical nature enables fast
 boolean operations in image space, without needing to perform complex
 geometrical calculations.  Services such as VizieR generally offer the
 MOC masks, allowing a faster experience in graphical applications
 such as Aladin, or for researchers quickly needing to locate which
 datasets may contain overlapping coverage.
 .
 The MOC mask image itself is tessellated and stored in NASA HealPix
 format, encoded inside a FITS image container.  Using the HealPix
 (Hierarchical Equal Area isoLatitude Pixelization) tessellation
 method ensures that more precision (pixels) in the mask are available
 when describing complex shapes such as approximating survey or
 polygon edges, while only needing to store a single big cell/pixel
 when an coverage is either completely inside, or outside of the mask.
 Catalogues can be rendered on the mask as circles.
 .
 It is written in Python and uses the PyMOC library.

Package: python3-pymoc
Description-md5: dd08809f5fe35817a256e4e1bd2a51ca
Description-en: Python Multi-Order Coverage maps for Virtual Observatory
 PyMOC provides a Python compatible library for handling MOCs.
 .
 Frequently astronomical survey catalogues or images are sparse and
 cover only a small part of the sky.  In a Multi-Order Coverage map
 the extent of data in a particular dataset is cached as a
 pre-calculated mask image.  The hierarchical nature enables fast
 boolean operations in image space, without needing to perform complex
 geometrical calculations.  Services such as VizieR generally offer the
 MOC masks, allowing a faster experience in graphical applications
 such as Aladin, or for researchers quickly needing to locate which
 datasets may contain overlapping coverage.
 .
 The MOC mask image itself is tessellated and stored in NASA HealPix
 format, encoded inside a FITS image container.  Using the HealPix
 (Hierarchical Equal Area isoLatitude Pixelization) tessellation
 method ensures that more precision (pixels) in the mask are available
 when describing complex shapes such as approximating survey or
 polygon edges, while only needing to store a single big cell/pixel
 when an coverage is either completely inside, or outside of the mask.
 Catalogues can be rendered on the mask as circles.

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Package: python-pydl-doc
Description-md5: ac56203e2bb8640660252fa4efb09fcd
Description-en: Library of IDL astronomy routines converted to Python (doc)
 PyDL consists of Python replacements for functions that are part of the IDL
 built-in library or part of astronomical IDL libraries.
 The emphasis is on reproducing results of the astronomical library
 functions.
 Only the bare minimum of IDL built-in functions are implemented to support
 this.
 .
 There are four astronomical libraries targeted:
 .
   * idlutils: a general suite of tools heavily used by SDSS.
   * Goddard utilities: The IDL Astronomy User's Library, maintained by
 Wayne Landsman and distributed with idlutils.
   * idlspec2d: tools for working with SDSS, BOSS and eBOSS spectroscopic
 data.
   * photoop: tools for working with SDSS imaging data.
 .
 This is the common documentation package.

Package: python3-pydl
Description-md5: bff08e5c0fd301b0aa1c5abb2e7e887a
Description-en: Library of IDL astronomy routines converted to Python 3
 PyDL consists of Python replacements for functions that are part of the IDL
 built-in library or part of astronomical IDL libraries.
 The emphasis is on reproducing results of the astronomical library
 functions.
 Only the bare minimum of IDL built-in functions are implemented to support
 this.
 .
 There are four astronomical libraries targeted:
 .
   * idlutils: a general suite of tools heavily used by SDSS.
   * Goddard utilities: The IDL Astronomy User's Library, maintained by
 Wayne Landsman and distributed with idlutils.
   * idlspec2d: tools for working with SDSS, BOSS and eBOSS spectroscopic
 data.
   * photoop: tools for working with SDSS imaging data.
 .
 This is the Python 3 version of the package.

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Package: python3-pyavm
Description-md5: f83d9eb40d8e8e135948e3655dfa40f6
Description-en: Python3 module to handle Astronomy Visualization Metadata Standard
 PyAVM is a module to represent, read, and write metadata following the
 Astronomy Visualization Metadata (AVM) standard.
 With pyavm you can:
 .
  * Parse AVM meta-data from an existing image.
  * Access and Set the metadata.
  * Create an AVM object from scratch.
  * Convert to a WCS object.
  * Initialize from a FITS header.
  * Initialize from a WCS object.
 .
 This is the Python 3 Version of the package.

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Package: libpoppler162
Description-md5: 74b6b371a9886bca4fc2c2761b5a2fec
Description-en: PDF rendering library
 Poppler is a PDF rendering library based on Xpdf PDF viewer.
 .
 This package contains the shared core library.

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Package: libpocl-dev
Description-md5: e354c66ecd7fac208f624d728c125be4
Description-en: development files for the PoCL library
 Portable Computing Language is an open source implementation of the OpenCL
 standard which can be easily adapted for new targets. One of the goals of the
 project is improving performance portability of OpenCL programs, avoiding the
 need for target-dependent manual optimizations.
 .
 This package provides the development files for the PoCL library. Unless very
 specific needs, this package is useless. This package is only required to link
 directly and explicitly with PoCL.
 .
 To develop OpenCL programs (that can be run with PoCL), the opencl-dev virtual
 package (provided by ocl-icd-opencl-dev for example) is required, not this one.

Package: libpocl-devices-level0
Description-md5: 9851a2c5fad1e6c605ec77ab44111700
Description-en: Portable Computing Language library - Level Zero device library
 Portable Computing Language is an open source implementation of the OpenCL
 standard which can be easily adapted for new targets. One of the goals of the
 project is improving performance portability of OpenCL programs, avoiding the
 need for target-dependent manual optimizations.
 .
 This package provides the Level Zero device library.

Package: libpocl2-common
Description-md5: 78bb8a43cbfd220175471920d25274ed
Description-en: common files for the PoCL library
 Portable Computing Language is an open source implementation of the OpenCL
 standard which can be easily adapted for new targets. One of the goals of the
 project is improving performance portability of OpenCL programs, avoiding the
 need for target-dependent manual optimizations.
 .
 This package provides the architecture independent files of the PoCL library.

Package: libpocl2t64
Description-md5: 610b47f08150bddaa4674d5a7911773f
Description-en: Portable Computing Language library
 Portable Computing Language is an open source implementation of the OpenCL
 standard which can be easily adapted for new targets. One of the goals of the
 project is improving performance portability of OpenCL programs, avoiding the
 need for target-dependent manual optimizations. A "native" target is included,
 which allows running OpenCL kernels on the host (CPU).
 .
 This package provides the core of PoCL.

Package: pocl-doc
Description-md5: 90921ef1c6cdf53ad65969ed754f50fc
Description-en: documentation for the PoCL library
 Portable Computing Language is an open source implementation of the OpenCL
 standard which can be easily adapted for new targets. One of the goals of the
 project is improving performance portability of OpenCL programs, avoiding the
 need for target-dependent manual optimizations.
 .
 This package provides the documentation for the PoCL library.

Package: pocl-opencl-icd
Description-md5: a2a9ed5c155c582d02308f5380e633cd
Description-en: PoCL ICD
 Portable Computing Language is an open source implementation of the OpenCL
 standard which can be easily adapted for new targets. One of the goals of the
 project is improving performance portability of OpenCL programs, avoiding the
 need for target-dependent manual optimizations. A "native" target is included,
 which allows running OpenCL kernels on the host (CPU).
 .
 This package allows one to use PoCL as an installable client driver (ICD) for
 OpenCL.

Package: pocl-source
Description-md5: 69e55c652ad234a993b70519db800689
Description-en: PoCL source code
 Portable Computing Language is an open source implementation of the OpenCL
 standard which can be easily adapted for new targets. One of the goals of the
 project is improving performance portability of OpenCL programs, avoiding the
 need for target-dependent manual optimizations.
 .
 This package provides original Debian (with Debian patches already applied)
 sources of PoCL shipped in a tarball. This can be used for building the
 device libraries for additional targets.

Package: pocl-tests
Description-md5: 598e05d38250b9a6f31635e04cdb7119
Description-en: PoCL testsuite
 Portable Computing Language is an open source implementation of the OpenCL
 standard which can be easily adapted for new targets. One of the goals of the
 project is improving performance portability of OpenCL programs, avoiding the
 need for target-dependent manual optimizations.
 .
 This package contains the source code of the PoCL test suite.

Package: pocld
Description-md5: 54d60007f5639a126449a7637a89ff55
Description-en: dummy pocld for PoCL-R
 Dummy package, will contain pocld from PoCL 6.1.

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533666a
Package: planetary-system-stacker
Description-md5: 01c01a0d62579a6eecd430400639609f
Description-en: create a sharp image of a planetary system object (moon, sun, planets)
 This package contrains software to produce a sharp image of a planetary
 system object (moon, sun, planets) from many seeing-affected frames using
 the "lucky imaging" technique._
 .
 The program is mainly targeted at extended objects (moon, sun), but it
 works as well for planets. Results obtained in many tests show at least
 the same image quality as with the established software AutoStakkert!3.
 .
 Input to the program can be either video files or directories containing
 still images. The following algorithmic steps are performed:
 .
  * First, all frames are ranked by their overall image quality.
  * On the best frame, a rectangular patch with the most pronounced structure
    in x and y is identified automatically. (Alternatively, the user can
    select the patch manually as well.)
  * Using this patch, all frames are aligned globally with each other.
  * A mean image is computed by averaging the best frames.
  * An alignment point mesh covering the object is constructed automatically.
    Points, where the image is too dim, or has too little contrast or structure,
    are discarded. The user can modify the alignment points, or set them all
    by hand as well.
  * For each alignment point, all frames are ranked by their local contrast
    in a surrounding image patch.
  * The best frames up to a given number are selected for stacking.
    Note that this list can be different for different points.
  * For all frames, local shifts are computed at all alignment points.
  * Using those shifts, the alignment point patches of all contributing
    frames are stacked into a single average image patch.
  * Finally, all stacked patches are blended into a global image, using the
    background image in places without alignment points.
  * After stacking is completed, the stacked image can be postprocessed
    (sharpened) either in a final step of the stacking workflow, or in a
    separate postprocessing job.

.
531771a

Package: python3-pillow-jpegxl-plugin
Description-md5: be598b2466ee4a53d57986eb55915d20
Description-en: Pillow plugin for JPEG-XL, using Rust for bindings
 Features:
  - JPEG-XL Plugin for Pillow
  - Encoder/Decoder to work with JPEG-XL using safe wrapper
  - Support EXIF metadata encoding
.
530500a
Package: phpmyadmin
Description-md5: b9abac2fce7719799e194516b6640871
Description-en: MySQL web administration tool
 This package allows administering of MySQL or MariaDB with a web interface.
 .
 It allows administrators to:
  - browse through databases and tables;
  - create, copy, rename, alter and drop databases;
  - create, copy, rename, alter and drop tables;
  - perform table maintenance;
  - add, edit and drop fields;
  - execute any SQL-statement, even multiple queries;
  - create, alter and drop indexes;
  - load text files into tables;
  - create and read dumps of tables or databases;
  - export data to SQL, CSV, XML, Word, Excel, PDF and LaTeX formats;
  - administer multiple servers;
  - manage MySQL users and privileges;
  - check server settings and runtime information with configuration hints;
  - check referential integrity in MyISAM tables;
  - create complex queries using Query-by-example (QBE), automatically
    connecting required tables;
  - create PDF graphics of database layout;
  - search globally in a database or a subset of it;
  - transform stored data into any format using a set of predefined
    functions, such as displaying BLOB-data as image or download-link;
  - manage InnoDB tables and foreign keys;
 and is fully internationalized and localized in dozens of languages.

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525819a
Package: python3-photutils
Description-md5: e1b13169e615ce5c2e06eb9aa197f15e
Description-en: Astropy affiliated package for image photometry (Python 3)
 Photutils contains functions for:
 .
  * estimating the background and background rms in astronomical images
  * detecting sources in astronomical images
  * estimating morphological parameters of those sources (e.g., centroid
    and shape parameters)
  * performing aperture and PSF photometry
 .
 This package contains the Python 3 version of the package.

.
508832,508842d
508149,508177d
499877,499895d
495548a
Package: liblru-ocaml
Description-md5: a47664f90cfdcea97295efdf97fca90d
Description-en: scalable LRU caches (runtime)
 Lru provides weight-bounded finite maps that can remove the
 least-recently-used (LRU) bindings in order to maintain a weight
 constraint.
 .
 This package contains runtime files.

Package: liblru-ocaml-dev
Description-md5: af962e8fcd95df69fe96bfdc39682762
Description-en: scalable LRU caches (development)
 Lru provides weight-bounded finite maps that can remove the
 least-recently-used (LRU) bindings in order to maintain a weight
 constraint.
 .
 This package contains development files.

.
494900a
Package: libezjsonm-lwt-ocaml
Description-md5: 1487655961aab8c880f2100797c18507
Description-en: simple Lwt-based interface to the Jsonm JSON library (runtime)
 Ezjsonm provides more convenient (but far less flexible) input and
 output functions that go to and from string values. This avoids the
 need to write signal code, which is useful for quick scripts that
 manipulate JSON.
 .
 More advanced users should go straight to the Jsonm library and use
 it directly, rather than be saddled with the Ezjsonm interface.
 .
 This simple interface over the Jsonm library provides an Lwt variant
 of the serialisation functions.
 .
 This package contains runtime files.

Package: libezjsonm-lwt-ocaml-dev
Description-md5: 210ac61a42288257d431b4b24e7437c5
Description-en: simple Lwt-based interface to the Jsonm JSON library (development)
 Ezjsonm provides more convenient (but far less flexible) input and
 output functions that go to and from string values. This avoids the
 need to write signal code, which is useful for quick scripts that
 manipulate JSON.
 .
 More advanced users should go straight to the Jsonm library and use
 it directly, rather than be saddled with the Ezjsonm interface.
 .
 This simple interface over the Jsonm library provides an Lwt variant
 of the serialisation functions.
 .
 This package contains development files.

Package: libezjsonm-ocaml
Description-md5: ec954fd1b1b949f40be7a07671b3998c
Description-en: simple interface on top of the Jsonm JSON library (runtime)
 Ezjsonm provides more convenient (but far less flexible) input and
 output functions that go to and from string values. This avoids the
 need to write signal code, which is useful for quick scripts that
 manipulate JSON.
 .
 More advanced users should go straight to the Jsonm library and use
 it directly, rather than be saddled with the Ezjsonm interface.
 .
 This package contains runtime files.

Package: libezjsonm-ocaml-dev
Description-md5: edcbc2b811e0e5b0e6cac5479828a97f
Description-en: simple interface on top of the Jsonm JSON library (development)
 Ezjsonm provides more convenient (but far less flexible) input and
 output functions that go to and from string values. This avoids the
 need to write signal code, which is useful for quick scripts that
 manipulate JSON.
 .
 More advanced users should go straight to the Jsonm library and use
 it directly, rather than be saddled with the Ezjsonm interface.
 .
 This package contains development files.

.
468095,468106d
465778,465790d
455511,455528d
453940a
Package: python3-mpl-animators
Description-md5: 08cfe88f7ae333cde8c824ddd1d871be
Description-en: Interative animation framework for matplotlib
 Set of classes which allow the easy construction of interactive
 matplotlib widget based animations.  “Out of the box” classes are
 provided for making line or image plots from numpy arrays, with
 sliders to control the animation automatically added for all
 dimensions not on the axes of the plot.

.
452355a
Package: moraine
Description-md5: 6c455119bd99bb326c615fdc25468b62
Description-en: snapshot backup over SSH/rsync and rclone (CLI + GTK desktop app)
 Moraine creates timestamped, hard-linked snapshots: each backup run looks like
 a complete tree, but unchanged files share disk via hard links, so history
 costs almost nothing. It restores individual files or whole trees, prunes old
 snapshots with a GFS retention policy, and keeps a run log.
 .
 Backends: rsync over SSH, and rclone (cloud, SFTP, SMB, WebDAV, S3, ...).
 .
 This package provides both the command-line client (moraine) and the GTK 4
 desktop application (moraine-gui) — run whichever you prefer.

.
448559,448573d
447810a
Package: mint-sticky
Description-md5: 98642a333f7b3ad1447e846fa09894ea
Description-en: Desktop Sticky Notes app for Linux
 This package contains the Sticky Notes app, which allows the quick creation of
 notes through an xapp status icon.

.
446594,446603d
437716,437726d
436646,436659d
436632c
Package: libmapnik4.3
.
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424821,424829d
410948,410956d
410889a
Package: libwignernj-dev
Description-md5: 13e9216570aad6f36b1aac20f96f302c
Description-en: Exact evaluation of Wigner symbols (development files)
 libwignernj is a scientific library that does exact evaluation of Wigner 3j,
 6j, and 9j symbols, Clebsch-Gordan coefficients, Racah W-coefficients, Fano
 X-coefficients, and Gaunt coefficients. All intermediate arithmetic is exact
 integer arithmetic using a prime-factorization representation; floating-point
 conversion happens only at the final step. Results are accurate to the last
 bit of the chosen output precision.
 .
 This package contains the header files and other development support.

Package: libwignernj0
Description-md5: f6bd06a635229bf617a1b31437cc41f0
Description-en: Exact evaluation of Wigner symbols
 libwignernj is a scientific library that does exact evaluation of Wigner 3j,
 6j, and 9j symbols, Clebsch-Gordan coefficients, Racah W-coefficients, Fano
 X-coefficients, and Gaunt coefficients. All intermediate arithmetic is exact
 integer arithmetic using a prime-factorization representation; floating-point
 conversion happens only at the final step. Results are accurate to the last
 bit of the chosen output precision.

.
410691a
Package: libwebservice-dropbox-perl
Description-md5: 2efb4b309cb3870587c7894cc2fa6013
Description-en: interface to Dropbox API for Perl
 WebService::Dropbox is a Perl interface to the Dropbox service using their
 API.
 .
  - Support Dropbox v2 REST API
  - Support Furl (Fast!!!)
  - Streaming IO (Low Memory)

.
410402a
Package: libweb-api-perl
Description-md5: 0b053a5fa6f4c14131ebd019017c8474
Description-en: simple base module for implementing RESTful APIs
 Web::API is a simple base module to implement almost any RESTful API with just
 a few lines of configuration. Implement the RESTful API of your choice in 10
 minutes, roughly.

.
373730a
Package: libnet-twitter-lite-perl
Description-md5: 586b461994d84b41297447257798a10a
Description-en: interface to the Twitter API
 Net::Twitter::Lite is a lightweight Perl implementation of the Twitter API.
 It uses the same definitions as Net::Twitter (see libnet-twitter-perl), but
 without the extra bells and whistles. Same great taste, less filling.
 .
 This module is related to, but is not part of, Net::Twitter. Its API methods
 and documentation are derived from Net::Twitter's internals. It exists for
 those who cannot, or prefer not to install Moose and its dependencies.
 .
 If you need additional functionality, finer-grained control over features,
 backwards compatibility with older versions and additional error handling
 options, you should using Net::Twitter instead.

Package: libnet-twitter-perl
Description-md5: 4fdf8de458eb19f8a6f3b3ca1f9ee799
Description-en: Perl interface to the Twitter social network
 Net::Twitter is a Perl module that provides an interface to the Twitter.com
 social networking site. This module allows you to set your status message
 as well as review the messages from those you follow.
 .
 This package also provides Net::Identica, an API for the Twitter-inspired
 StatusNet social networking software, <URL:http://status.net/>.
 .
 DEPRECATION NOTICE: According to the upstream author, Net::Twitter has
 been superseded by Twitter::API and will no longer be supported in the future.

.
373068a
Package: libnet-oauth-perl
Description-md5: 229e57533790e7a628ca66292bde593c
Description-en: implementation of the OAuth 1.0 protocol
 Net::OAuth implements OAuth, which is "An open protocol to allow secure API
 authentication in a simple and standard method from desktop and web
 applications."
 .
 In practical terms, OAuth is a mechanism for a Consumer to request protected
 resources from a Service Provider on behalf of a user.

.
372435a
Package: libnet-dropbox-api-perl
Description-md5: fd59235b8d517ad490cbe06de9ef7940
Description-en: Perl module providing a dropbox API interface
 Net::Dropbox::API is a perl interface to the Dropbox API. The Dropbox
 API is a OAuth based API.

.
364698a
Package: libmail-chimp3-perl
Description-md5: 75d05be786dc8200eb6cffbf0adf858b
Description-en: interface to mailchimp.com's RESTful Web API v3
 Mail::Chimp3 is a Perl package for interacting with The Rocket Science Group's
 MailChimp service via its RESTful Web API v3.0. The package makes use of
 WEB::API.

.
359284,359303d
358842,358878d
352819a
Package: libhmsbeagle-dev
Description-md5: e2cf134283793dc53c4584f6ab2c2591
Description-en: High-performance lib for Bayesian and Maximum Likelihood phylogenetics (devel)
 BEAGLE is a high-performance library that can perform the core calculations at
 the heart of most Bayesian and Maximum Likelihood phylogenetics packages. It
 can make use of highly-parallel processors such as those in graphics cards
 (GPUs) found in many PCs.
 .
 The project involves an open API and fast implementations of a library for
 evaluating phylogenetic likelihoods (continuous time Markov processes) of
 biomolecular sequence evolution.
 .
 The aim is to provide high performance evaluation 'services' to a wide range
 of phylogenetic software, both Bayesian samplers and Maximum Likelihood
 optimizers.  This allows these packages to make use of implementations that
 make use of optimized hardware such as graphics processing units.
 .
 This package contains development files needed to build against Beagle library.

Package: libhmsbeagle-java
Description-md5: 19e3721dbbb7bb8a6b2e6402430b80ec
Description-en: High-performance lib for Bayesian and Maximum Likelihood phylogenetics (java)
 BEAGLE is a high-performance library that can perform the core calculations at
 the heart of most Bayesian and Maximum Likelihood phylogenetics packages. It
 can make use of highly-parallel processors such as those in graphics cards
 (GPUs) found in many PCs.
 .
 The project involves an open API and fast implementations of a library for
 evaluating phylogenetic likelihoods (continuous time Markov processes) of
 biomolecular sequence evolution.
 .
 The aim is to provide high performance evaluation 'services' to a wide range
 of phylogenetic software, both Bayesian samplers and Maximum Likelihood
 optimizers.  This allows these packages to make use of implementations that
 make use of optimized hardware such as graphics processing units.
 .
 This package contains the Java interface.

Package: libhmsbeagle1v5
Description-md5: d1ca6965facda724668a6194b79a4004
Description-en: High-performance lib for Bayesian and Maximum Likelihood phylogenetics
 BEAGLE is a high-performance library that can perform the core calculations at
 the heart of most Bayesian and Maximum Likelihood phylogenetics packages. It
 can make use of highly-parallel processors such as those in graphics cards
 (GPUs) found in many PCs.
 .
 The project involves an open API and fast implementations of a library for
 evaluating phylogenetic likelihoods (continuous time Markov processes) of
 biomolecular sequence evolution.
 .
 The aim is to provide high performance evaluation 'services' to a wide range
 of phylogenetic software, both Bayesian samplers and Maximum Likelihood
 optimizers.  This allows these packages to make use of implementations that
 make use of optimized hardware such as graphics processing units.

.
349974,350024d
346337a
Package: libflickr-api-perl
Description-md5: 0b9f0e66a8d6b5d5a28b40b519e5d204
Description-en: Perl interface to the Flickr API
 Flickr::API is a simple interface for using the Flickr API in Perl. It is a
 subclass of LWP::UserAgent, so all of the various proxy, request limit, cache
 and other options are available.

Package: libflickr-upload-perl
Description-md5: d350a815844ceb128a486fcee1605a3e
Description-en: module for uploading images to flickr.com
 flickr_upload is a completely functional batch uploading tool which
 uses Perl module Flickr::Upload as its back-end. It is flickr.com
 image uploading made easy and quick from the command line; it also
 helps you tagging, choosing access control, defining content type,
 setting safety level, etc., while uploading your images.
 .
 flickr_upload may also be useful for generating authentication tokens
 against other API keys/secrets (i.e. for embedding in scripts).

.
340296a
Package: libdist-zilla-plugin-twitter-perl
Description-md5: 657549f2669ed0a775b3279203da3367
Description-en: Twitter when you release with Dist::Zilla
 Dist::Zilla::Plugin::Twitter module will use Net::Twitter to send a
 release notice to Twitter. By default, it will include a short link to
 the release page of your module on http://metacpan.org.

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324736c
Package: libbluray4
.
318013a
Package: libless-awful-ssl-clojure
Description-md5: be77c5ffc1c5cdb0f98dafb04612ac8a
Description-en: ssl wrapper for clojure around java crypto libraries
 This library tries to make it less complicated to build simple SSL-enabled
 applications: given a CA certificate and a signed key and cert, it can give
 you an SSLContext suitable for creating TCPSockets directly, or handing off
 to Netty.

.
317556,317705d
317548a
Package: lemonade-desktop
Description-md5: a94a7d856fc975b051cc978be777596d
Description-en: Local LLM serving with GPU and NPU acceleration web application
 Lemonade helps users run local LLMs with the highest performance by
 configuring state-of-the-art inference engines for their NPUs and GPUs.
 .
 Lemonade works with model providers such as huggingface.
 This package provides the web application.

Package: lemonade-server
Description-md5: 349decff01e89fd9d44997e375798eea
Description-en: Local LLM serving with GPU and NPU acceleration server
 Lemonade helps users run local LLMs with the highest performance by
 configuring state-of-the-art inference engines for their NPUs and GPUs.
 .
 Lemonade works with model providers such as huggingface.
 This package provides the server.

.
317497a
Package: lefse
Description-md5: 99a95edfdd51afd5bb9d222117f5342b
Description-en: determine features of organisms, clades, taxonomic units, genes
 LEfSe (Linear discriminant analysis Effect Size) determines the features
 (organisms, clades, operational taxonomic units, genes, or functions)
 most likely to explain differences between classes by coupling standard
 tests for statistical significance with additional tests encoding
 biological consistency and effect relevance.

.
314554a
Package: laniakea-mailgun
Description-md5: 73ca45a30bdb1223e9641970dd3cf363
Description-en: Management suite for Debian-based OSes - E-Mail Sender
 Laniakea is a software suite to manage Debian derivatives. It provides
 tooling to maintain an APT archive (and multiple individual package
 repositories), perform QA on it, autobuild packages, sync packages,
 etc. It also provides various tools for better insight into the archive.
 .
 This package contains a service that listens on the Laniakea ZeroMQ
 message stream and sends e-mails to users or mailinglist if the events
 fulfill certain criteria.

Package: laniakea-mirk
Description-md5: f40ad6e36ddc7c0c883f06e02885777d
Description-en: Management suite for Debian-based OSes - Matrix Bot
 Laniakea is a software suite to manage Debian derivatives. It provides
 tooling to maintain an APT archive (and multiple individual package
 repositories), perform QA on it, autobuild packages, sync packages,
 etc. It also provides various tools for better insight into the archive.
 .
 This package contains a Matrix bot that listens on the Laniakea ZeroMQ
 message stream and posts messages to Matrix chat rooms if the fulfill
 certain criteria.

Package: laniakea-server
Description-md5: e10a8e497164a9d8cb7f160221c06553
Description-en: Management suite for Debian-based OSes - Privileged Server
 Laniakea is a software suite to manage Debian derivatives. It provides
 tooling to maintain an APT archive (and multiple individual package
 repositories), perform QA on it, autobuild packages, sync packages,
 etc. It also provides various tools for better insight into the archive.
 .
 This package contains many of the privileged server components that require
 write-access to the Postgres database of Laniakea.
 .
 Laniakea requires to be manually configured for the respective environment
 before this package will do anything.
 Refer to the documentation on how to set up the database and environment.

Package: laniakea-webdash
Description-md5: 64b02ba9ded57b3168ab658449fd2a5f
Description-en: Management suite for Debian-based OSes - Web Dashboard
 Laniakea is a software suite to manage Debian derivatives. It provides
 tooling to maintain an APT archive (and multiple individual package
 repositories), perform QA on it, autobuild packages, sync packages,
 etc. It also provides various tools for better insight into the archive.
 .
 This package contains a web dashboard application that displays the
 status of the archive suites as well as various developer information.

Package: laniakea-webswview
Description-md5: fab3fd30a1855deeaa9d9af679697570
Description-en: Management suite for Debian-based OSes - Web Software Index
 Laniakea is a software suite to manage Debian derivatives. It provides
 tooling to maintain an APT archive (and multiple individual package
 repositories), perform QA on it, autobuild packages, sync packages,
 etc. It also provides various tools for better insight into the archive.
 .
 This package contains a web application that allows searching for
 applications and packages in the software archive.

Package: laniakea-webupload
Description-md5: 9b33de5db751e8c5350cb7a6e099661e
Description-en: Management suite for Debian-based OSes - HTTP Upload Receiver
 Laniakea is a software suite to manage Debian derivatives. It provides
 tooling to maintain an APT archive (and multiple individual package
 repositories), perform QA on it, autobuild packages, sync packages,
 etc. It also provides various tools for better insight into the archive.
 .
 This package contains a small webserver application that accepts uploads
 that were pushed using dput(1) and places them in a safe location for
 Rubicon to check.

Package: python3-laniakea
Description-md5: 4e021c2fcd0cb188b67958a44d53a50c
Description-en: Management suite for Debian-based OSes - Python module
 Laniakea is a software suite to manage Debian derivatives. It provides
 tooling to maintain an APT archive (and multiple individual package
 repositories), perform QA on it, autobuild packages, sync packages,
 etc. It also provides various tools for better insight into the archive.
 .
 This package contains the shared Python module which provides the database
 schema, message schema and common archive actions.

.
285344,285355d
277650a
Package: icingaweb2-module-fileshipper
Description-md5: ecd91f8356d960f2f6d28acd04bd010d
Description-en: This Module offers to deploy config files through the Director
 Icinga Web 2 is a very modular, fast and simple web interface for your Icinga
 monitoring environment.
 .
 This module offers the possibility to deploy hand-crafted Icinga 2 config files
 through the Icinga Director based on Import Source able to deal with CSV, JSON,
 YAML and XML files.

.
277641a
Package: icingaweb2-module-director
Description-md5: a788c6f09090c096fb6b877cd994d700
Description-en: simple and responsive web interface for Icinga - director module
 Icinga Web 2 is a very modular, fast and simple web interface for your Icinga
 monitoring environment.
 .
 The software will give you a web frontend for your monitoring solution, and
 can run additional modules, extending monitoring data, or even supplying
 something new to the webinterface.
 .
 Icinga Director is a configuration tool that has been designed to make Icinga 2
 configuration easy and understandable.

.
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Package: icingaweb2-module-businessprocess
Description-md5: 15dd2bf75459ff2d4815c71fcf0c2114
Description-en: simple and responsive web interface for Icinga - businessprocess module
 Icinga Web 2 is a very modular, fast and simple web interface for your Icinga
 monitoring environment.
 .
 The software will give you a web frontend for your monitoring solution, and
 can run additional modules, extending monitoring data, or even supplying
 something new to the webinterface.
 .
 Business Process viewer and modeler provides a web-based process modeler. It
 integrates as a module into Icinga Web 2 and provides a plugin check command
 for Icinga. Tile and tree views can be shown inline, as dashlets or fullscreen.
 All of those for whole processes or just parts of them.

.
272461,272500d
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Package: python3-hickle
Description-md5: f5d0eaa1b47b5943c7d97f9ff2c9c7b1
Description-en: HDF5 based version of pickle
 An HDF5 based clone of 'pickle', with a twist: instead of serializing to a
 pickle file, Hickle dumps to an HDF5 file (Hierarchical Data Format). It is
 designed to be a "drop-in" replacement for pickle (for common data objects),
 but is really an amalgam of 'h5py' and 'pickle' with extended functionality.
 .
 That is: 'hickle' is a neat little way of dumping Python variables to HDF5
 files that can be read in most programming languages, not just Python. Hickle
 is fast, and allows for transparent compression of your data (LZF / GZIP).

.
268879,268887d
268653a
Package: healpy-data
Description-md5: c4ee58a35b8a2b11453f31bb679a1262
Description-en: HEALPix representation of spherical data - Python data
 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 platform-independent data and test files for the Python
 wrapper around the C++ implementation of HEALPix.

Package: python3-healpy
Description-md5: 0bf0c1a24964e5387d62f4b693d05b4f
Description-en: HEALPix representation of spherical data - Python3 interface
 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 Python3 wrapper around the C++ implementation of
 HEALPix.

.
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Package: python-gwcs-doc
Description-md5: 1c0a35bbb4ec5034b5723027291cb469
Description-en: Tools for managing the WCS of astronomical data (documentation)
 GWCS takes a general approach to WCS. It supports a data model which includes
 the entire transformation pipeline from input coordinates (detector by
 default) to world coordinates.  The goal is to provide a flexible toolkit
 which is easily extendible by adding new transforms and frames.
 .
 This is the common documentation package.

Package: python3-gwcs
Description-md5: 849090319f2f4fc3412d1f7616a20729
Description-en: Tools for managing the WCS of astronomical data (Python 3)
 GWCS takes a general approach to WCS. It supports a data model which includes
 the entire transformation pipeline from input coordinates (detector by
 default) to world coordinates.  The goal is to provide a flexible toolkit
 which is easily extendible by adding new transforms and frames.
 .
 This package contains the Python 3 version of the package.

.
216807,216814d
216256,216264d
214348,214361d
214258,214264d
214001,214006d
213612,213614c
Description-md5: b7f711932e725d67dbf0ebe30d871de4
Description-en: Go terminal and console support library
 This library provides the following terminal and console support
 functionality:
 .
  * Putting a terminal into raw mode
  * Reading a line of input from a terminal without local echo
  * Setting Bracketed Paste Mode (if supported)
  * Setting the terminal prompt
  * Determining whether a given file descriptor is a terminal
  * Restoring the terminal connected to a given file descriptor
    to a previous state
.
211697,211712d
210951,210957d
210636a
Package: golang-github-tonistiigi-go-archvariant-dev
Description-md5: 5929fa0755406e38e0311b5c6b296d61
Description-en: Go package to detect compatibility version of the current system
 go-archvariant is a Go package for determining the maximum compatibility
 version of the current system. The main use case is to use this value in
 container platform definitions.
 .
 On x86-64 platforms this package returns the maximum current
 microarchitecture level as defined in (https://en.wikipedia.org/wiki/X86-
 64#Microarchitecture_levels).

.
209879,209886d
209857,209864d
206149,206154d
203583,203590d
200622,200627d
191790,191796d
189765,189774d
189753,189759d
177800a
Package: python3-glue
Description-md5: cda164a782a94826c5b0f862140869d8
Description-en: Python 3 library for data interaction
 python3-glue is a Python library for data interaction, it blurs the boundary
 between GUI-centric and code-centric data exploration.
 There are many ways to leverage Glue from Python. Among other things, you can
 write code to do the following:
 .
  * Send data in the form of NumPy arrays or Pandas DataFrames to Glue for
    exploration.
  * Write startup scripts that automatically load and clean data,
    before starting Glue.
  * Write custom functions to parse files, and plug these functions into the
    Glue GUI.
  * Write custom functions to link datasets, and plug these into the Glue GUI.
  * Create your own visualization modules.

.
177745a
Package: glueviz
Description-md5: bf1c4b982292f3fff4aa9fcaf248dced
Description-en: Linked data visualization
 Glue is a Python project to link visualizations of scientific datasets across
 many files. Some of its features are:
 .
  * Interactive, linked statistical graphics of multiple files.
  * Support for many file formats including common image formats,
    ascii tables, astronomical image and table formats (fits, vot, ipac), and
    HDF5. Custom data loaders can also be easily added.
  * Highly scriptable and extendable.
 .
 This package also provides the default "glue" command.

Package: python3-glue-qt
Description-md5: a3154830e19624fed9277b0de36a9829
Description-en: Qt-based user interface package for glueviz
 Glue is a Python project to link visualizations of scientific datasets
 within and among files. This package provides the Qt-based graphical
 user interface components. and viewers for the glue ecosystem.
 .
 Some of its features are:
 .
  * Interactive, linked statistical graphics of multiple files.
  * Support for many file formats including common image formats,
    ascii tables, astronomical image and table formats (fits, vot,
    ipac), and HDF5. Custom data loaders can also be easily added.
  * Highly scriptable and extendable.

.
177617,177629d
172439a
Package: ginga
Description-md5: 972fb915e6622a9c7b415eaaef76f0f9
Description-en: Astronomical image viewer
 Ginga is a toolkit designed for building viewers for scientific image
 data in Python, visualizing 2D pixel data in numpy arrays.
 It can view astronomical data such as contained in files based on the
 FITS (Flexible Image Transport System) file format.  It is written and
 is maintained by software engineers at the Subaru Telescope, National
 Astronomical Observatory of Japan.
 .
 The Ginga toolkit centers around an image display object which supports
 zooming and panning, color and intensity mapping, a choice of several
 automatic cut levels algorithms and canvases for plotting scalable
 geometric forms.  In addition to this widget, a general purpose
 "reference" FITS viewer is provided, based on a plugin framework.
 A fairly complete set of standard plugins are provided for features
 that is expected from a modern FITS viewer: panning and zooming windows,
 star catalog access, cuts, star pick/fwhm, thumbnails, etc.
 .
 This package contains the image viewer based on Python 3.

Package: python3-ginga
Description-md5: d731bb4342e78bd6d6d942e6aaf91c8c
Description-en: Astronomical image toolkit for Python
 Ginga is a toolkit designed for building viewers for scientific image
 data in Python, visualizing 2D pixel data in numpy arrays.
 It can view astronomical data such as contained in files based on the
 FITS (Flexible Image Transport System) file format.  It is written and
 is maintained by software engineers at the Subaru Telescope, National
 Astronomical Observatory of Japan.
 .
 The Ginga toolkit centers around an image display object which supports
 zooming and panning, color and intensity mapping, a choice of several
 automatic cut levels algorithms and canvases for plotting scalable
 geometric forms.  In addition to this widget, a general purpose
 "reference" FITS viewer is provided, based on a plugin framework.
 A fairly complete set of standard plugins are provided for features
 that is expected from a modern FITS viewer: panning and zooming windows,
 star catalog access, cuts, star pick/fwhm, thumbnails, etc.

.
157422,157426c
  - quoting pertinent source code (with a cache)
  - underlining points and ranges in the source code, possibly with labels
  - emitting fix-it hints
  - generating patches from fix-it hints
  - SARIF output
.
157419c
Description-md5: 3b982c26f4b6aa3b430c9b0e3fbf47cd
.
137176a
Package: gavodachs2-server
Description-md5: 36391efd1065f86dfafb16b4f7e89cda
Description-en: server package of the Virtual Observatory data center suite
 This package sets up a ready-to use VO data center using GAVO's Data
 Center Helper Suite (DaCHS), in particular by configuring a postgres
 database backend.  The DaCHS server lets data center operators ingest
 their astronomical data into structured repositories and publish
 those to the Virtual Observatory.

Package: python3-gavo
Description-md5: 1c634877326cf502048f42bdccfac82d
Description-en: Virtual Observatory data center publishing suite
 The Data Center Helper Suite (DaCHS) is a collection of Python modules
 (with some exceptions) to help you in setting up and running a VO-compliant
 data center. Moreover, some parts of this code are useful for client-side
 applications.
 .
 Currently, DaCHS supports most DAL protocols (SIAP, SCS, TAP), form-based
 interfaces, a publishing registry, ADQL and some other (less prominent)
 VO standards, and data management for various kinds of input.

Package: python3-gavo-stc
Description-md5: 270bd0999c4874471ee63f8166c8729c
Description-en: IVOA Space-Time-Coordinate (STC) library
 This library handles space-time information within the Virtual
 Observatory (VO) according to the IVOA (International Virtual
 Observatory Alliance) STC recommendation.
 .
 The VO knows two implementations for STC metadata, one in XML
 called STC-X and a linear string implementation called STC-S.
 This library provides support for the generating and parsing of
 STC-S expressions and STC-X documents. Moreover, it contains various
 helper functions for the transformation between Earth coordinate
 systems, for dealing with sky coordinates, for time parsing and time
 conversions, and for the definition and conversion of units in STC.

Package: python3-gavo-utils
Description-md5: 61e4a499504252b650d4f02f2b653b3b
Description-en: support library for the Virtual Observatory
 The "python3-gavoutils" library is a collection of helper functions and
 classes used by various VO libraries and applications.
 .
 Among other things, this collection provides support for memoisation,
 for formatting and text manipulation. It contains bindings for the
 pgsphere postgres extension, utility functions to deal with
 FITS files and math-related helper functions.

Package: python3-gavo-votable
Description-md5: 82d7e91c302fe182587ef0d4adc5345a
Description-en: library for the reading and writing of VOTables
 The VOTable format is defined by the International Virtual Observatory
 Alliance (IVOA) to facilitate data exchange in astronomy. This library
 implements most of the specification and offers simple and advanced,
 streaming interfaces.  Also included is a simple client to query TAP
 servers.

.
94473,94484d
93603a
Package: python3-einsteinpy
Description-md5: 3177305117e8eee627b5bdb745fe9b7b
Description-en: General Relativity in Python
 EinsteinPy is an open source pure Python package
 dedicated to problems arising in General Relativity
 and relativistic physics, such as goedesics plotting
 for schwarzschild space-time model, calculation of
 schwarzschild radius for any mass given, symbolic
 calculation of various functions related to GR such
 as christoffel symbols. Features like visualization
 of geodesics of curved black holes and 3D visualizations
 are some of the features which are planned.
 It is released under the MIT license.

.
76049,76139d
73574,73584d
68542a
Package: dde-qtplatform-plugins
Description-md5: d26d10dfde2f6e517c4bfabb59036d31
Description-en: Qt platform theme integration plugin for DDE
 Deepin's dde-qtplatform-plugins is the Qt platform integration plugin for
 Deepin Desktop Environment. It provides an abstract interface between Deepin
 applications and the Qt toolkit for further application theme customization.
 .
 This package provides the Qt 6 (DTK6) xcb platform plugin.
 .
 This package is part of DDE (Deepin Desktop Environment).

.
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Package: python3-compyle
Description-md5: 2f80dc2cdc6fc3bed5fe6f505745722b
Description-en: Execute a subset of Python on HPC platforms
 ComPyle allows users to execute a restricted subset of Python (almost
 similar to C) on a variety of HPC platforms. Currently it supports
 multi-core execution using Cython, and OpenCL and CUDA for GPU devices.
 .
 Users start with code implemented in a very restricted Python syntax,
 this code is then automatically transpiled, compiled and executed to run
 on either one CPU core, or multiple CPU cores (via OpenMP_) or on a GPU.
 CPy offers source-to-source transpilation, making it a very convenient
 tool for writing HPC libraries.
 .
 Some simple yet powerful parallel utilities are provided which can allow
 you to solve a remarkably large number of interesting HPC problems.
 .
 ComPyle also features JIT transpilation if you wish making it easy to use.

.
51005,51013d
40332,40339d
28265,28273d
24162a
Package: beast-mcmc
Description-md5: 347f87629165216c55313b0035e8c195
Description-en: Bayesian MCMC phylogenetic inference
 BEAST is a cross-platform program for Bayesian MCMC analysis of molecular
 sequences. It is entirely orientated towards rooted, time-measured
 phylogenies inferred using strict or relaxed molecular clock models. It
 can be used as a method of reconstructing phylogenies but is also a
 framework for testing evolutionary hypotheses without conditioning on a
 single tree topology. BEAST uses MCMC to average over tree space, so that
 each tree is weighted proportional to its posterior probability. Included
 is a simple to use user-interface program for setting up standard
 analyses and a suit of programs for analysing the results.

Package: beast-mcmc-examples
Description-md5: c63bad5feea098eb39bb86db8b6f8d33
Description-en: Bayesian MCMC phylogenetic inference - example data
 BEAST is a cross-platform program for Bayesian MCMC analysis of molecular
 sequences. It is entirely orientated towards rooted, time-measured
 phylogenies inferred using strict or relaxed molecular clock models. It
 can be used as a method of reconstructing phylogenies but is also a
 framework for testing evolutionary hypotheses without conditioning on a
 single tree topology. BEAST uses MCMC to average over tree space, so that
 each tree is weighted proportional to its posterior probability. Included
 is a simple to use user-interface program for setting up standard
 analyses and a suit of programs for analysing the results.
 .
 This package contains the example data.

Package: libnucleotidelikelihoodcore0
Description-md5: 2beeba75259cb25079c34eef520b0bde
Description-en: implementation of LikelihoodCore for nucleotides used by beast-mcmc
 BEAST is a cross-platform program for Bayesian MCMC analysis of molecular
 sequences. It is entirely orientated towards rooted, time-measured
 phylogenies inferred using strict or relaxed molecular clock models. It
 can be used as a method of reconstructing phylogenies but is also a
 framework for testing evolutionary hypotheses without conditioning on a
 single tree topology. BEAST uses MCMC to average over tree space, so that
 each tree is weighted proportional to its posterior probability. Included
 is a simple to use user-interface program for setting up standard
 analyses and a suit of programs for analysing the results.
 .
 This package provides an implementation of LikelihoodCore for nucleotides
 that calls native methods for maximum speed.

.
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22725a
Package: barnowl
Description-md5: 433996a434a354683f4eb690c5630cfb
Description-en: A curses-based tty Jabber, IRC, AIM  and Zephyr client
 A curses-based instant-messaging client supporting the Jabber, IRC, AIM
 and Zephyr  protocols.  Much of the functionality is written in
 Perl, which is supported as an extension language.
 .
 This is a fork of ktools software's owl Zephyr/AIM client.

.
16840a
Package: python3-astroscrappy
Description-md5: 3de22ef6cfb247c9a8ef0d2625289d81
Description-en: Optimized Cosmic Ray Annihilation in Python
 Astro-SCRAPPY is designed to detect cosmic rays in images (numpy arrays),
 based on Pieter van Dokkum's L.A.Cosmic algorithm. Parallelization is
 achieved using OpenMP.

.
16831a
Package: python3-regions
Description-md5: f8ac057da2e217bd82b761264140aac9
Description-en: Python astronomy package for region handling
 The regions package provides (or plans to provide) classes to
 represent regions defined using pixel or celestial coordinates or on
 the celestial sphere.

.
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Package: python-astroplan-doc
Description-md5: 537438698779b9600c1a32398a64bf63
Description-en: Observation planning package for astronomers (documentation)
 Astroplan is an observation planning package for astronomers that can help
 you plan for everything but the clouds.
 .
 It is an Astropy affiliated package that seeks to make your life as an
 observational astronomer a little less infuriating.
 .
 This is the common documentation package.

Package: python3-astroplan
Description-md5: c7c7af5113ce1fc8cd984c41e83ca73c
Description-en: Observation planning package for astronomers (Python 3)
 Astroplan is an observation planning package for astronomers that can help
 you plan for everything but the clouds.
 .
 It is an Astropy affiliated package that seeks to make your life as an
 observational astronomer a little less infuriating.
 .
 This is the Python 3 version of the package.

Package: astropy-utils
Description-md5: 66f91a2a4f6c2297733b7ed899429da7
Description-en: Command line tools from astropy
 The astropy package contains core functionality and some common tools
 needed for performing astronomy and astrophysics research with Python.
 .
 This package contains the tools that come with astropy:
 .
  * fitscheck: Detect and fix FITS standards violations
  * fits2bitmap: Create a bitmap file from a FITS image.
  * fitsdiff: Compare two FITS image files and report the differences in
    header keywords and data.
  * fitsheader: Print the header(s) of one or more FITS file(s) to the
    standard output in a human-readable format.
  * samp_hub: SAMP Hub Server.
  * volint: Check a VOTable file for compliance to the VOTable specification
  * wcslint: Check the WCS keywords in a FITS file for compliance against
    the standards

Package: python-astropy-doc
Description-md5: 142e0ddf11adb0314ec7d19a6e6e32f1
Description-en: Core functionality for performing astrophysics with Python (doc)
 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.
 .
 This package contains the package documentation.

Package: python3-astropy
Description-md5: d68fca10e089e4294adf8b1b26f541e5
Description-en: Core functionality for performing astrophysics with Python
 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.

Package: python3-astropy-healpix
Description-md5: 7ed8a3c89fa603ecc76331ec59fe9dac
Description-en: HEALPix representation of spherical data - Python 3
 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 is a BSD-licensed HEALPix package developed by the Astropy project
 and based on C code written by Dustin Lang in astrometry.net.
 .
 This package provides modules for Python 3.

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Package: astrometry.net
Description-md5: 5088a1bfc88af04d691f7b897003b643
Description-en: Astrometry plate solver
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.

Package: libastrometry-dev
Description-md5: b5a843798778b7ab6bf804109900ecb0
Description-en: Astrometry plate solver (development files)
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the development files (header files).

Package: libastrometry0t64
Description-md5: dd36773275e2c7f43405ef4cc3dd45c3
Description-en: Astrometry plate solver (shared lib)
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the shared library.

Package: python3-astrometry
Description-md5: 17cf233c1fb49e79f9a00e2b5738ddfc
Description-en: Astrometry plate solver (Python package)
 The astrometry engine will take any image and return the astrometry
 world coordinate system (WCS), a standards-based description of the
 transformation between image coordinates and sky coordinates.
 .
 This package contains the Python Package.

Package: python3-astroml
Description-md5: 8e8a4ce58b113433cddaea867fcfe70f
Description-en: Python 3 Machine Learning library for astronomy
 AstroML is a Python 3 module for machine learning and data mining built on
 numpy, scipy, scikit-learn, and matplotlib. It contains a growing library of
 statistical and machine learning routines for analyzing astronomical data in
 Python, loaders for several open astronomical datasets, and a large suite of
 examples of analyzing and visualizing astronomical datasets.

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Package: python3-astrodendro
Description-md5: c63461a16e92fbee251415a57aa31535
Description-en: Astronomical Dendrograms in Python 3
 Python 3 module is to provide an easy way to compute dendrograms of observed or
 simulated Astronomical data in Python 3.

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Package: python3-astlib
Description-md5: a0aa5fb13bc1a8ee544f54380dbaa38e
Description-en: General Python3 tools for astronomy
 astLib is a set of Python3 modules that provides some tools for research
 astronomers. It can be used for astronomical plots, some statistics, common
 calculations, coordinate conversions, and manipulating FITS images with World
 Coordinate System (WCS) information through PyWCSTools - a simple wrapping of
 WCSTools by Jessica Mink. PyWCSTools is distributed (and developed) as part
 of astLib.

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Package: asterisk-espeak
Description-md5: 1c95aef9393ef961171fa3c024e3bdf7
Description-en: eSpeak module for Asterisk
 Module for the Asterisk open source PBX which allows you to use the
 eSpeak voice synthesis engine to render text to speech.

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Package: python3-asdf-astropy
Description-md5: 39a889e1f0b286c5082b0b71ca57a2a0
Description-en: ASDF serialization support for astropy
 This package includes plugins that provide ASDF serialization support
 for astropy objects. The plugins are automatically enabled when the
 package is installed. ASDF (Advanced Scientific Data Format) is a
 proposed next generation interchange format for scientific data,
 mainly used by the Space Telescope Science Institude (STScI).

Package: python3-asdf-coordinates-schemas
Description-md5: 12f750cb462a787c006ea0df7802de83
Description-en: ASDF schemas for validating coordinates tags
 ASDF (Advanced Scientific Data Format) is a proposed
 next generation interchange format for scientific data. ASDF aims to
 exist in the same middle ground that made FITS so successful, by
 being a hybrid text and binary format: containing human editable
 metadata for interchange, and raw binary data that is fast to load
 and use. Unlike FITS, the metadata is highly structured and is
 designed up-front for extensibility.
 .
 This package provides ASDF schemas for validating coordinates tags.
 Users should not need to install this directly; instead, install an
 implementation package such as asdf-astropy.

Package: python3-asdf-standard
Description-md5: 12f7a4b84316047707c8033de2ae8d2e
Description-en: Python package describing the Advanced Scientific Data Format
 ASDF (Advanced Scientific Data Format) is a proposed
 next generation interchange format for scientific data. ASDF aims to
 exist in the same middle ground that made FITS so successful, by
 being a hybrid text and binary format: containing human editable
 metadata for interchange, and raw binary data that is fast to load
 and use. Unlike FITS, the metadata is highly structured and is
 designed up-front for extensibility.
 .
 This package provides the ASDF standard schemas.

Package: python3-asdf-transform-schemas
Description-md5: 81864429d634ace4faa3bc3e9a65ab8e
Description-en: ASDF schemas for validating transform tags
 ASDF (Advanced Scientific Data Format) is a proposed
 next generation interchange format for scientific data. ASDF aims to
 exist in the same middle ground that made FITS so successful, by
 being a hybrid text and binary format: containing human editable
 metadata for interchange, and raw binary data that is fast to load
 and use. Unlike FITS, the metadata is highly structured and is
 designed up-front for extensibility.
 .
 This package provides ASDF schemas for validating transform tags.
 Users should not need to install this directly; instead, install an
 implementation package such as asdf-astropy.

Package: python3-asdf-wcs-schemas
Description-md5: 739b0194322bff199a031e5286e11c5f
Description-en: ASDF schemas for validating WCS tags
 ASDF (Advanced Scientific Data Format) is a proposed
 next generation interchange format for scientific data. ASDF aims to
 exist in the same middle ground that made FITS so successful, by
 being a hybrid text and binary format: containing human editable
 metadata for interchange, and raw binary data that is fast to load
 and use. Unlike FITS, the metadata is highly structured and is
 designed up-front for extensibility.
 .
 This package provides ASDF schemas for validating WCS tags.
 Users should not need to install this directly; instead, install an
 implementation package such as asdf-astropy.

.
14943a
Package: python3-arpys
Description-md5: 8f081a618b6ffe009b92acd991db7531
Description-en: ARPES (Angle Resolved PhotoEmission Spectroscopy) data analysis
 Collection of libraries, functions and tools related to ARPES data
 loading and analysis.

.
12338c
 This package contains the MySQL / MariaDB database driver.
.
12329,12330c
Description-md5: f86fad3724e8feabd4e561588a1c6ad6
Description-en: Apache Portable Runtime Utility Library - MySQL/MariaDB Driver
.
11630,11642d
8901,8913d
2950,2959d
