En astronomie, la réduction de données consiste en un traitement des
données depuis des expositions brutes pour produire des données
scientifiquement exploitables. Cela comprend le traitement CCD de base, les
calibrations astrométriques et photométriques, le retraitement,
l'estimation des erreurs et d'autres étapes.
Ce métapaquet installe des infrastructures de réduction de données
astronomiques universellement utilisables, mais aussi d'autres pour des
télescopes spécifiques.
Official Debian packages with high relevance
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astap
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2024.05.01-1
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solveur astrométrique, empilement d'images, photométrie et visionneur FITS
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astap:
solveur astrométrique, empilement d'images, photométrie et visionneur FITS
- Description
-
✏
ASTAP est un programme libre de solveur astrométrique (« plate solver ») et d'empilage pour les images du ciel profond. Il fonctionne avec des images astronomiques au format FITS, mais peut importer des images RAW DSLR ou des images XISF, PGM, PPM, TIF, PNG et JPG. Il possède un visionneur FITS puissant et le solveur astronomique natif peut être utilisé par les programmes d'imagerie CCDCiel, NINA, APT ou SGP pour synchroniser la monture en se basant sur une image prise.
Principales caractéristiques :
– solveur astrométrique natif, ligne de commande compatible avec
PlateSolve2 ;
– empilage d'images astronomiques comprenant la correction d'image
d'obscurité et de champ plat ;
– filtrage des images de ciel profond basé sur la valeur
d'HFD et de valeur moyenne ;
– alignement utilisant une routine interne de correspondance
d'étoile, un solveur astrométrique interne ;
– construction de mosaïques couvrant de grandes régions utilisant
les solutions astrométriques linéaires WCS ou polynomiales WCS+SIP ;
– égaliseur d'arrière plan ;
– visionneur FITS avec fonction « swipe », ciel profond et
annotations d'étoile, photométrie et inspecteur CCD ;
– visionneur de miniatures FITS ;
– enregistrement des résultats dans des fichiers FITS 16 bits ou
32 bits flottants ;
– exportation vers des fichiers JPEG, PNG, TIFF, PFM, PPM et PGM ;
– édition d'en-têtes FITS ;
– fonction de recadrage FITS ;
– calibration de photométrie automatique avec les bases de
données Gaia, Johnson -V ou Gaia Bm ;
– inspecteur CCD ;
– annotations Deepsky et Hyperleda ;
– annotations d'objets solaires avec les éphémérides MPC ;
– lecture et écriture de binaires FITS et lecture de tables ASCII ;
– quelques fonctions de calcul de pixel et traitement de
développement numérique ;
– affichage des images et des tables de fichiers FITS à extensions
multiples ;
– routine de clignotement.
- Maintainer
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- Versions
-
- Popularity
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- 7 regular users
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9 recent
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91 total installations
(of 247608 submissions)
- Debian
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astap-cli
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2022.12.09-1
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solveur astrométrique, version en ligne de commande
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astap-cli:
solveur astrométrique, version en ligne de commande
- Description
-
✏
Ce paquet fournit un solveur en ligne de commande compact compatible avec la version avec interface graphique d'astap.
Pas de fenêtre contextuelle.
Il n'accepte pas les fichiers bruts et ne fonctionne pas avec SharpCap dans la mesure où le champ de vue n'est pas mémorisé.
- Maintainer
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- Versions
-
- Popularity
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- 4 regular users
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7 recent
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66 total installations
(of 247608 submissions)
- Debian
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astromatic
|
1.1
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collection logicielle d'infrastructure astronomique
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astromatic:
collection logicielle d'infrastructure astronomique
- Description
-
✏
Le logiciel AstrOmatic est conçu pour être lancé en mode batch sur de
grandes quantités de données, la plupart du temps sur des plateformes
Unix, avec un minimum d'intervention humaine. Il est actuellement utilisé
dans diverses infrastructures d'étude d'images dont TERAPIX, le système de
gestion des données d'étude de l'énergie noire et Astro-WISE.
Ce métapaquet installe tous les logiciels d'AstrOmatic.net empaquetés pour
Debian.
- Maintainer
-
- Versions
-
- Popularity
-
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85 total installations
(of 247608 submissions)
- Debian
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- Upstream
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astrometry.net
|
0.97+dfsg-1
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solveur de plaque photographique astrométrique
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astrometry.net:
solveur de plaque photographique astrométrique
-
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✏
Le moteur astrometry prend n'importe quelle image et renvoie le système de
coordonnées mondiales (WCS) d’astrométrie, une description basée sur les
standards de la transformation entre les coordonnées de l'image et les
coordonnées célestes.
- Reference
-
- Maintainer
-
- Versions
-
- Popularity
-
- 124 regular users
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115 recent
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1060 total installations
(of 247608 submissions)
- Enhancements
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- Debian
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- Upstream
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- Improve entry
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eso-pipelines
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1.3
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??? missing short description for package eso-pipelines :-(
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eso-pipelines:
??? missing short description for package eso-pipelines :-(
- Maintainer
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- Versions
-
- Popularity
-
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83 total installations
(of 247608 submissions)
- Debian
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- Upstream
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esorex
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3.13.1-1+deb10u1
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outils d’exécution pour des automatismes de l’Observatoire européen austral
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esorex:
outils d’exécution pour des automatismes de l’Observatoire européen austral
- Description
-
✏
EsoRex veut dire European Southern Observatory (ESO) Recipe Execution Tool,
outil d’exécution de procédés de l’ESO. Il peut lister, configurer et
exécuter des « recipes » (procédés) basés sur CPL à partir de la ligne de
commande.
CPL (Common Pipeline Library) se compose d’un ensemble de bibliothèques en
C ISO fournissant une boîte à outils logicielle complète, efficace et
fiable. Elle constitue une base pour la création de tâches automatisées de
réduction des données pour l’astronomie.
Une des fonctions fournies par CPL est la possibilité de créer des
algorithmes de réduction de données fonctionnant sous forme de greffons
(bibliothèques dynamiques). Ceux-ci sont appelés « recipes » (procédés) et
sont les éléments principaux de l’environnement CPL de développement de
réduction de données.
- Maintainer
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- Versions
-
- Tags
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✏
- field
- astronomy
- interface
- commandline
- role
- program
- science
- calculation
- use
- converting, organizing
- works-with
- image, image:raster
- Popularity
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- 4 regular users
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7 recent
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106 total installations
(of 247608 submissions)
- Debian
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fitsh
|
0.9.4-1
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Software package for astronomical image processing
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fitsh:
Software package for astronomical image processing
- Description
-
This software package provides independent binary programs (so called tasks)
which performs various steps of astronomical image reduction and data
processing. These tasks are designed for execution from a UNIX command line
shell or shell script. Each of these tasks performs a specific operation
(e.g. transforming an image to another reference frame, search and identifiy
stars or other point-like sources, do photometry, transform/display a
FITS image to a popular graphics format, ...) while the details of a
certain operation are specified via command switches and arguments.
Therefore this package does not need any higher level operating environment
than a standard UNIX shell, however, processing the related data might
require a little more knowledge of the used shell itself. If you find this
program useful in your research, please cite 2012MNRAS.421.1825P
as "2012, MNRAS, 421, 1825". See also the web page of the project, found at
http://fitsh.net/. That page gathers information about the program
(including documentation and examples), this is the primary download source
of the package itself, and additionally, serves a public forum for the
program users in various topics. Bug reports, comments and ideas are welcomed!
- Reference
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- Maintainer
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- Versions
-
- Popularity
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- 6 regular users
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6 recent
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90 total installations
(of 247608 submissions)
- Debian
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gnuastro
|
0.8-1
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programmes GNU Astronomy Utilities
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gnuastro:
programmes GNU Astronomy Utilities
- Description
-
✏
Gnuastro (GNU Astronomy Utilities) est un ensemble de bibliothèques et de
programmes pour l'analyse et la manipulation de données astronomiques. Les
programmes peuvent être exécutés en ligne de commande pour une utilisation
simple et efficace, et les bibliothèques peuvent être utilisées dans des
programmes C et C++.
Ce paquet fournit les programmes de Gnuastro.
- Reference
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- Maintainer
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- Versions
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- Popularity
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- 11 regular users
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6 recent
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94 total installations
(of 247608 submissions)
- Debian
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- Upstream
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missfits
|
2.8.0-5
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Basic maintenance and packaging tasks on FITS files
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missfits:
Basic maintenance and packaging tasks on FITS files
- Description
-
MissFITS is a program that performs basic maintenance and packaging tasks on
FITS files using an optimised FITS library. MissFITS can:
- add/edit/remove FITS header keywords
- split/join Multi-Extension-FITS (MEF) files
- unpile/pile FITS data-cubes
- create/check/update FITS checksums, using R. Seaman’s protocol.
- Reference
-
- Maintainer
-
- Versions
-
- Popularity
-
- 2 regular users
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7 recent
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90 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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montage
|
6.0+dfsg-6
↺
New upstream version
6.1
available
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Toolkit for assembling FITS images into mosaics
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montage:
Toolkit for assembling FITS images into mosaics
- Description
-
Montage is a toolkit for assembling astronomical images into custom mosaics.
It uses algorithms that preserve the calibration and positional (astrometric)
fidelity of the input images to deliver mosaics that meet user-specified
parameters of projection, coordinates, and spatial scale. It supports all
projections and coordinate systems in use in astronomy.
It contains independent modules for analyzing the geometry of images on the
sky, and for creating and managing mosaics; these modules are powerful tools
in their own right and have applicability outside mosaic production, in areas
such as data validation.
- Reference
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- Maintainer
-
- Versions
-
- Popularity
-
- 11 regular users
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14 recent
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118 total installations
(of 247608 submissions)
- Debian
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munipack
|
0.6.1-1
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Astronomical photometry software package
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munipack:
Astronomical photometry software package
- Description
-
Munipack is a general astronomical photometry software package.
Currently implements functions for standard photometry processing
(photometry reductions - dark, flat), aperture photometry, astrometry
and photometry calibration, accessing Virtual observatory, etc.
This is a dependency package providing recommended complete installation.
- Reference
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- Maintainer
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- Versions
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- Popularity
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86 total installations
(of 247608 submissions)
- Debian
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- Upstream
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planetary-system-stacker
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0.8.32~git20230901.01f3625-2
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create a sharp image of a planetary system object (moon, sun, planets)
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planetary-system-stacker:
create a sharp image of a planetary system object (moon, sun, planets)
- Description
-
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.
- Maintainer
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- Versions
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0.8.32~git20221019.66d7558-2
(bookworm)
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0.8.32~git20230901.01f3625-2
(trixie)
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0.8.32~git20230901.01f3625-2
(sid)
- Popularity
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- 8 regular users
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7 recent
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63 total installations
(of 247608 submissions)
- Debian
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- Upstream
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psfex
|
3.24.2-2
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Point Spread Function model extractor
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psfex:
Point Spread Function model extractor
- Description
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Extract models of the Point Spread Function (PSF) from FITS images processed
with SExtractor, and measures the quality of images. The generated PSF models
can be used for model-fitting photometry or morphological analyses.
- Reference
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- Maintainer
-
- Versions
-
- Popularity
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- 2 regular users
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8 recent
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89 total installations
(of 247608 submissions)
- Debian
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- Upstream
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python3-astroscrappy
|
1.0.8-1
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annihilation optimisée de rayons cosmiques avec Python
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python3-astroscrappy:
annihilation optimisée de rayons cosmiques avec Python
- Description
-
✏
Astro-SCRAPPY est conçu pour la détection des rayons cosmiques dans des
images (tableaux numpy), basée sur l’algorithme L.A.Cosmic de Pieter van
Dokkum. La parallélisation est réalisée en utilisant OpenMP.
- Reference
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- Maintainer
-
- Versions
-
- Popularity
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- 14 regular users
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15 recent
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173 total installations
(of 247608 submissions)
- Debian
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- Upstream
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python3-ccdproc
|
1.3.0-5
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Basic data reductions of astronomy CCD images
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python3-ccdproc:
Basic data reductions of astronomy CCD images
- Description
-
The ccdproc package provides many of the necessary tools for processing
of ccd images built on a framework to provide error propagation and bad
pixel tracking throughout the reduction process.
- Maintainer
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- Versions
-
- Popularity
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- 15 regular users
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9 recent
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165 total installations
(of 247608 submissions)
- Debian
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python3-cpl
|
0.7.2-1
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Control pipeline recipes from the ESO (Python3)
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python3-cpl:
Control pipeline recipes from the ESO (Python3)
- Description
-
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.
- Reference
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- Maintainer
-
- Versions
-
- Popularity
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- 13 regular users
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14 recent
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154 total installations
(of 247608 submissions)
- Debian
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- Upstream
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python3-montage-wrapper
|
0.9.9-4
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Python-3 wrapper for the Montage mosaicking toolkit
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python3-montage-wrapper:
Python-3 wrapper for the Montage mosaicking toolkit
- Description
-
This package provides a Python-3 wrapper to the Montage Astronomical Image
Mosaic Engine, including both functions to access individual Montage
commands, and high-level functions to facilitate mosaicking and
re-projecting.
- Maintainer
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- Versions
-
- Popularity
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- 3 regular users
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6 recent
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60 total installations
(of 247608 submissions)
- Debian
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python3-photutils
|
0.6-1
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Astropy affiliated package for image photometry (Python 3)
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python3-photutils:
Astropy affiliated package for image photometry (Python 3)
- Description
-
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.
- Maintainer
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- Versions
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- Popularity
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- 14 regular users
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20 recent
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183 total installations
(of 247608 submissions)
- Debian
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scamp
|
2.0.4-3
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Compute astrometric and photometric solutions
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scamp:
Compute astrometric and photometric solutions
- Description
-
SCAMP reads SExtractor catalogs and computes astrometric and
photometric solutions for any arbitrary sequence of FITS images in a
completely automatic way.
- Reference
-
- Maintainer
-
- Versions
-
- Popularity
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- 4 regular users
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7 recent
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92 total installations
(of 247608 submissions)
- Debian
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- Upstream
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stiff
|
2.4.0-7
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conversion d’images scientifiques FITS dans le format TIFF
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stiff:
conversion d’images scientifiques FITS dans le format TIFF
- Description
-
✏
STIFF est un programme qui convertit les images scientifiques FITS dans le
format TIFF pour servir d’illustrations. Les principales caractéristiques
sont :
– reproduction précise de la luminosité et de la couleur des surfaces originelles ;
– ajustement automatique ou manuel du contraste et de la brillance ;
– balance automatique de l’intensité et de la couleur du ciel d’arrière-plan ;
– saturation des couleurs ajustable ;
– possibilité de correction gamma adaptée aux couleurs ;
– un ou trois canaux d’entrée, sortie en niveau de gris ou vrai couleur ;
– sortie en 8 ou 16 bits par composante ;
– recombinaison de pixels (rebinning) et options de déplacement x/y ;
– prise en charge de grandes images d’entrée et sortie sur du matériel standard
(prise en charge du format BigTIFF) ;
– prise en charge de pyramides tuilées et multirésolutions ;
– prise en charge des méthodes de compression sans ou avec pertes ;
– code multi-processus légers avec équilibrage de charge pour pleinement utiliser
plusieurs cœurs et plusieurs processeurs ;
– sortie XML, conforme au format VOT, des métadonnées.
- Reference
-
- Maintainer
-
- Versions
-
- Popularity
-
- 3 regular users
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7 recent
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98 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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swarp
|
2.19.1-1
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Resample and co-add together FITS images
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swarp:
Resample and co-add together FITS images
- Description
-
Resample and co-add together FITS images using any arbitrary astrometric
projection defined in the WCS standard. The main features of SWarp
are:
- FITS format (including multi-extensions) in input and output,
- Full handling of weight-maps in input and output,
- Ability to work with very large images (up to 500 Mpixels on
32-bit machines and 10^6 Tpixels with 64-bits), thanks to customized
virtual-memory-mapping and buffering,
- Works with arrays in up to 9 dimensions (including or not two spherical
coordinates),
- Selectable high-order interpolation method (up to 8-tap filters) in any
dimension,
- Compatible with WCS and TNX (IRAF) astrometric descriptions,
- Support for equatorial, galactic and equatorial coordinate systems,
- Astrometric and photometric parameters are read from FITS headers or
external ASCIIfiles,
- Built-in background subtraction,
- Built-in noise-level measurement for automatic weighting,
- Automatic centering and sizing functions of the output field,
- Multi-threaded code with load-balancing to take advantageof multiple
processors.
- XML VOTable-compliant output of meta-data.
- Reference
-
-
E. Bertin, Y. Mellier, M. Radovich, G. Missonnier, P. Didelon and B. Morin:
The TERAPIX Pipeline.
281:228
(2002)
- Maintainer
-
- Versions
-
- Popularity
-
- 5 regular users
-
7 recent
-
102 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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theli
|
3.1.4-1
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Astronomical image data reduction pipeline
|
theli:
Astronomical image data reduction pipeline
-
-
THELI is a powerful tool to reduce optical, near- and mid-infrared
astronomical imaging data, supporting more than 100 different single-
and multi-chip instruments at professional observatories world-wide. The
graphical user interface and internal data model allow the user to
concentrate on the highly automated data processing, without being
side-tracked by the specific complexities and characteristics of optical
and infrared instruments. THELI is fully scalable on multi-processor
machines with shared memory, allowing fast processing also of large data
sets. The integrated data viewer allows access to any products on drive
as well as in memory. User-defined instruments can be added, making
THELI interesting for amateur astronomers as well.
- Reference
-
- Maintainer
-
- Versions
-
- Popularity
-
- 2 regular users
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6 recent
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49 total installations
(of 247608 submissions)
- Debian
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weightwatcher
|
1.12-1
|
Combine maps and polygon data for astronomical image processing
|
weightwatcher:
Combine maps and polygon data for astronomical image processing
- Description
-
WeightWatcher is a program that combines weight-maps, flag-maps and polygon
data in order to produce control maps which can directly be used in
astronomical image-processing packages like Drizzle, Swarp or SExtractor.
Weight-thresholding and/or specific flag selections are applied by
WeightWatcher through a configuration file: this alleviates other programs
from such interpretation work. WeightWatcher will mostly be useful as part of
an imaging survey pipeline. Its main features are:
- Processing speed: limited by the I/O performances of the machine
(typically 50 Mpixel/s on a workstation),
- Ability to work with very large images (up to, say, 10^8 × 10^9 pixels on
a 64 bit system),
- FITS format (including Multi-Extension) is used for input and
output. Output flag-map format selection is automatic (8, 16 or 32bits),
- Up to 30 weight-maps, 30 flag-maps, and thousands of polygons can be
handled simultaneously.
- Automatic rasterizing of DS9 .reg files,
- Statistics of flagged and weighted areas,
- Metadata output in XML-VOTable format.
- Reference
-
- Maintainer
-
- Versions
-
- Popularity
-
- 4 regular users
-
7 recent
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87 total installations
(of 247608 submissions)
- Debian
-
- Upstream
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- Improve entry
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|
▾
|
yorick-mira
|
1.1.0+git20170124.3bd1c3~dfsg1-2
↺
New upstream version
2.2.0
available
|
optical interferometry image reconstruction within Yorick
|
yorick-mira:
optical interferometry image reconstruction within Yorick
-
-
MiRA is an algorithm for image reconstruction from data provided by
optical interferometers. It is written in the Yorick language and
operated through the Yorick interpreter.
MiRA won the 2008' Interferometric Imaging Beauty Contest organized
by International Astronomical Union (IAU) to compare the image
synthesis algorithms designed for optical interferometry. In a
nutshell, MiRA proceeds by direct minimization of a penalized
likelihood. This penalty is the sum of two terms: a likelihood term
(typically a χ2) which enforces agreement of the model with the data,
plus a regularization term to account for priors. The priors are
required to lever the many degeneracies due to the sparseness of the
spatial frequency sampling. MiRA implements many different
regularizations (quadratic or edge-preserving smoothness, total
variation, maximum entropy, etc.) and let the user defines his own
priors. The likelihood penalty is modular and designed to account for
available data of any kind (complex visibilities, powerspectra and/or
closure phase). One of the strength of MiRA is that it is purely
based on an inverse problem approach and can therefore cope with
incomplete data set; for instance, MiRA can build an image without
any Fourier phase information. Input data must be in OI-FITS format.
- Maintainer
-
- Versions
-
-
0.9.10+dfsg-1
(jessie)
-
1.1.0+git20170124.3bd1c3~dfsg1-2
(sid)
-
1.1.0+git20170124.3bd1c3~dfsg1-2
(trixie)
-
1.1.0+git20170124.3bd1c3~dfsg1-2
(buster)
-
1.1.0+git20170124.3bd1c3~dfsg1-2
(stretch)
-
1.1.0+git20170124.3bd1c3~dfsg1-2
(bullseye)
-
2.2.0
(upstream)
- Popularity
-
-
68 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
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Official Debian packages with lower relevance
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cpl-plugin-amber
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4.3.4+dfsg-1
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tuyauterie de réduction de données pour l’instrument AMBER de l’ESO
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cpl-plugin-amber:
tuyauterie de réduction de données pour l’instrument AMBER de l’ESO
- Maintainer
-
- Versions
-
- Popularity
-
-
83 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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▾
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cpl-plugin-fors
|
5.3.11+dfsg-1
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ESO data reduction pipeline for the FORS1/2 instruments
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cpl-plugin-fors:
ESO data reduction pipeline for the FORS1/2 instruments
- Description
-
FORS pipeline recipes for the reduction of data obtained with the FORS1 and
FORS2 instruments in the LSS, MOS, MXU, PMOS, and direct imaging instrument
modes.
FORS is the visual and near UV FOcal Reducer and low dispersion Spectrograph
for the Very Large Telescope (VLT) of the European Southern Observatory
(ESO). Two versions of FORS have been built, upgraded and moved to the
Cassegrain foci of different telescopes in the past years. In April 2009,
FORS1 was dismounted to make room for X-shooter, so only FORS2 is in
operation. FORS is designed as an all-dioptric instrument for the wavelength
range from 330 nm to 1100 nm and provides an image scale of 0".25/pixel (or
0".125/pixel with the high resolution collimator) in the standard readout
mode (2x2 binning). FORS2 is installed on UT1 (Antu) and is by default
equipped with a detector system that is optimised for the red with a very low
level of fringes thanks to a mosaic of two 2k x 4k MIT CCDs (with 15 μm
pixels). However, the blue-optimised detector system that was previously
available on FORS1 has been commissioned on FORS2 and can be requested for
Visitor Mode observation. The geometries of both detector systems are
similar, with the optical axis falling ~30" above the gap and offsets of a
few arc-seconds between the two chips. FORS2 has many modes, including
multi-object spectroscopy with exchangeable masks, long-slit spectroscopy,
imaging and spectro-polarimetry and high-time resolution imaging and
spectroscopy.
- Maintainer
-
- Versions
-
- Popularity
-
-
26 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
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|
▾
|
cpl-plugin-giraf
|
2.16.7+dfsg-4
|
??? missing short description for package cpl-plugin-giraf :-(
|
cpl-plugin-giraf:
??? missing short description for package cpl-plugin-giraf :-(
- Maintainer
-
- Versions
-
- Popularity
-
-
83 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
-
|
▾
|
cpl-plugin-hawki
|
2.4.3+dfsg-1
|
??? missing short description for package cpl-plugin-hawki :-(
|
cpl-plugin-hawki:
??? missing short description for package cpl-plugin-hawki :-(
- Maintainer
-
- Versions
-
- Popularity
-
-
86 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
-
|
▾
|
cpl-plugin-kmos
|
1.3.5+dfsg-1
|
ESO data reduction pipeline for the KMOS instrument
|
cpl-plugin-kmos:
ESO data reduction pipeline for the KMOS instrument
- Description
-
This is the data reduction pipeline for the KMOS instrument of the
Very Large Telescope (VLT) from the European Southern Observatory (ESO).
The K-band Multi Object Spectrograph (KMOS) is a second-generation instrument
designed for operation on the VLT. The key feature of KMOS is its ability to
perform Integral Field Spectroscopy in the near-infrared bands for 24 targets
simultaneously.
- Maintainer
-
- Versions
-
- Popularity
-
-
41 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
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|
▾
|
cpl-plugin-muse
|
2.6+dfsg-1
|
??? missing short description for package cpl-plugin-muse :-(
|
cpl-plugin-muse:
??? missing short description for package cpl-plugin-muse :-(
- Reference
-
- Maintainer
-
- Versions
-
- Popularity
-
-
79 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
-
|
▾
|
cpl-plugin-naco
|
4.4.11+dfsg-1
|
??? missing short description for package cpl-plugin-naco :-(
|
cpl-plugin-naco:
??? missing short description for package cpl-plugin-naco :-(
- Maintainer
-
- Versions
-
- Popularity
-
-
84 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
-
|
▾
|
cpl-plugin-sinfo
|
2.5.2+dfsg-2
|
??? missing short description for package cpl-plugin-sinfo :-(
|
cpl-plugin-sinfo:
??? missing short description for package cpl-plugin-sinfo :-(
- Reference
-
-
F. Eisenhauer, R. Abuter, K. Bickert, F. Biancat-Marchet, H. Bonnet, J. Brynnel, R.D. Conzelmann, B. Delabre, R. Donaldson, J. Farinato, E. Fedrigo, R. Genzel, N.N. Hubin, C. Iserlohe, M.E. Kasper, M. Kissler-Patig, G.J. Monnet, C. Roehrle, J. Schreiber, S. Stroebele, M. Tecza, N.A. Thatte and H. Weisz:
SINFONI - Integral field spectroscopy at 50 milli-arcsecond resolution with the ESO VLT.
Instrument Design and Performance for Optical/Infrared Ground-based Telescopes
4841:1548-1561
(2003)
(eprint)
- Maintainer
-
- Versions
-
- Popularity
-
-
3 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
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|
▾
|
cpl-plugin-uves
|
5.9.1+dfsg-1
|
??? missing short description for package cpl-plugin-uves :-(
|
cpl-plugin-uves:
??? missing short description for package cpl-plugin-uves :-(
- Maintainer
-
- Versions
-
- Popularity
-
-
79 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
-
|
▾
|
cpl-plugin-vimos
|
3.1.7+dfsg-1
|
??? missing short description for package cpl-plugin-vimos :-(
|
cpl-plugin-vimos:
??? missing short description for package cpl-plugin-vimos :-(
- Maintainer
-
- Versions
-
- Popularity
-
-
82 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
-
|
▾
|
cpl-plugin-visir
|
4.3.0+dfsg1-1
|
??? missing short description for package cpl-plugin-visir :-(
|
cpl-plugin-visir:
??? missing short description for package cpl-plugin-visir :-(
- Maintainer
-
- Versions
-
- Popularity
-
-
81 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
-
|
▾
|
cpl-plugin-xshoo
|
2.8.4+dfsg-3
|
ESO data reduction pipeline for the XSHOOTER instrument
|
cpl-plugin-xshoo:
ESO data reduction pipeline for the XSHOOTER instrument
- Description
-
This is the data reduction pipeline for the XSHOOTER instrument of the
Very Large Telescope (VLT) from the European Southern Observatory (ESO).
XSHOOTER is a multi wavelength (300-2500nm) medium resolution spectrograph
mounted at the UT2 Cassegrain focus. XSHOOTER consists of 3 arms, each with
optimized optics, dispersive elements and detectors:
- UVB, covering the wavelength range 300-559.5 nm,
- VIS, covering the wavelength range 559.5-1024 nm,
- NIR, covering the wavelength range 1024-2480 nm.
- Maintainer
-
- Versions
-
- Popularity
-
-
23 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
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|