The term data reduction in astronomy means the data processing from the raw
exposures up to scientific usable data. This includes the basic CCD
processing, the astrometric and photometric calibrations, the reprocessing,
error estimation and other steps.
This metapackage will install astronomy data reduction pipelines that can be
used universally, but also those for specific telescopes.
Official Debian packages with high relevance
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astap
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2024.05.01-1
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astrometric (plate) solver, stacking of images, photometry and FITS viewer
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astap:
astrometric (plate) solver, stacking of images, photometry and FITS viewer
- Description
-
ASTAP is a free stacking and astrometric solver (plate solver) program for
deep sky images. In works with astronomical images in the FITS format, but
can import RAW DSLR images or XISF, PGM, PPM, TIF, PNG and JPG images. It
has a powerful FITS viewer and the native astrometric solver can be used
by CCDCiel, NINA, APT or SGP imaging programs to synchronise the mount
based on an image taken.
Main features:
- Native astrometric solver, command line compatible with PlateSolve2.
- Stacking astronomical images including dark frame and flat field correction.
- Filtering of deep sky images based on HFD value and average value.
- Alignment using an internal star match routine,
internal astrometric solver.
- Mosaic building covering large areas using the astrometric linear
solution WCS or WCS+SIP polynomial.
- Background equalizing.
- FITS viewer with swipe functionality, deep sky and star annotation,
photometry and CCD inspector.
- FITS thumbnail viewer.
- Results can be saved to 16 bit or float (-32) FITS files.
- Export to JPEG, PNG, TIFF, PFM, PPM, PGM files.
- FITS header edit.
- FITS crop function.
- Automatic photometry calibration against Gaia database,
Johnson -V or Gaia Bm
- CCD inspector
- Deepsky and Hyperleda annotation
- Solar object annotation using MPC ephemerides
- Read/writes FITS binary and reads ASCII tables.
- Some pixel math functions and digital development process
- Can display images and tables from a multi-extension FITS.
- Blink routine.
- Maintainer
-
- 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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- Upstream
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astap-cli
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2022.12.09-1
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astrometric (plate) solver, command line version
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astap-cli:
astrometric (plate) solver, command line version
- Description
-
This package contains a barebone command-line solver compatible with
the GUI version of astap.
No pop-up notifier.
It will not accept raw files and will not work with SharpCap since
FOV is not stored.
- Maintainer
-
- Versions
-
- Popularity
-
- 4 regular users
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7 recent
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66 total installations
(of 247608 submissions)
- Debian
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- Upstream
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astromatic
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1.1
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천문 파이프라인 소프트웨어 모음
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astromatic:
천문 파이프라인 소프트웨어 모음
- Description
-
✏
AstrOmatic 소프트웨어는 사람의 개입을 최소로 하면서 대부분의 유닉스 플랫폼에서 대용량의 데이터에 대해 배치 모드로 실행되야 합니다. 현재 TERAPIX, Dark-Energy Survey Data Management 시스템 및 Astro-WISE 등을 포함해서 다양한 이미지 조사 파이프라인에서 사용되고 있습니다.
이 메타패키지는 데비안용으로 패키징된 AstrOmatic.net의 모든 소프트웨어를 설치할 것 입니다.
- Maintainer
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- Versions
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- Popularity
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85 total installations
(of 247608 submissions)
- Debian
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- Upstream
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astrometry.net
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0.97+dfsg-1
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Astrometry plate solver
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astrometry.net:
Astrometry plate solver
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-
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.
- Reference
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- Maintainer
-
- Versions
-
- Popularity
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- 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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- Improve entry
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esorex
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3.13.1-1+deb10u1
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Execution Tool for European Southern Observatory pipelines
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esorex:
Execution Tool for European Southern Observatory pipelines
- Description
-
EsoRex is the European Southern Observatory (ESO) Recipe Execution Tool. It
can list, configure and execute CPL-based recipes from the command line.
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.
- Maintainer
-
- 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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- Upstream
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- Improve entry
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fitsh
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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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- Upstream
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- Improve entry
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gnuastro
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0.8-1
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GNU Astronomy Utilities programs
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gnuastro:
GNU Astronomy Utilities programs
- Description
-
GNU Astronomy Utilities (Gnuastro) is a collection of libraries and programs
for astronomical data analysis and manipulation. The programs can be run on
the command-line for efficient and easy usage and the libraries can be used
within C and C++ programs.
This package contains Gnuastro's programs.
- Reference
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- Maintainer
-
- 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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- Improve entry
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missfits
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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
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- Maintainer
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- Versions
-
- Popularity
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- 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
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- 11 regular users
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14 recent
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118 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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munipack
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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
-
- 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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- Improve entry
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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
-
- 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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- Improve entry
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psfex
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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
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- 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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- Improve entry
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python3-astroscrappy
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1.0.8-1
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Optimized Cosmic Ray Annihilation in Python
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python3-astroscrappy:
Optimized Cosmic Ray Annihilation in Python
- Description
-
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.
- Reference
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- Maintainer
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- Versions
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- 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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- Improve entry
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python3-ccdproc
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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
-
- 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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- Upstream
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- Improve entry
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python3-cpl
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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
-
- Maintainer
-
- Versions
-
- Popularity
-
- 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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- Improve entry
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python3-montage-wrapper
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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
-
- 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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- Improve entry
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python3-photutils
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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
-
- 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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- Upstream
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scamp
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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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- Improve entry
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stiff
|
2.4.0-7
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convert scientific FITS images to the TIFF format
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stiff:
convert scientific FITS images to the TIFF format
- Description
-
STIFF is a program that converts scientific FITS images to the TIFF format
for illustration purposes. The main features of STIFF are:
- Accurate reproduction of the original surface brightnesses and colours
- Automatic or manual contrast and brightness adjustments
- Automatic sky background intensity and colour balance
- Adjustable colour saturation
- Colour-friendly gamma correction capabilities
- One or three input channels: gray-scale or true colour output
- Output with 8 or 16 bits per component
- Pixel rebinning and x/y flip options
- Support for arbitrarily large input and output images on standard
hardware (BigTIFF support)
- Support for tiled, multiresolution pyramids
- Support for lossless and lossy compression methods
- Multi-threaded code with load-balancing to take advantage of multiple
cores and processors.
- XML VOTable-compliant output of meta-data.
- 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
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102 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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theli
|
3.1.4-1
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Astronomical image data reduction pipeline
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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
-
6 recent
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49 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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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
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7 recent
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87 total installations
(of 247608 submissions)
- Debian
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- 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
|
▾
|
cpl-plugin-amber
|
4.3.4+dfsg-1
|
??? missing short description for package cpl-plugin-amber :-(
|
cpl-plugin-amber:
??? missing short description for package cpl-plugin-amber :-(
- Maintainer
-
- Versions
-
- Popularity
-
-
83 total installations
(of 247608 submissions)
- Debian
-
- Upstream
-
- Improve entry
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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
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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
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- Versions
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- Popularity
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26 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-giraf
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2.16.7+dfsg-4
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??? missing short description for package cpl-plugin-giraf :-(
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cpl-plugin-giraf:
??? missing short description for package cpl-plugin-giraf :-(
- Maintainer
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- Versions
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- Popularity
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83 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-hawki
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2.4.3+dfsg-1
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??? missing short description for package cpl-plugin-hawki :-(
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cpl-plugin-hawki:
??? missing short description for package cpl-plugin-hawki :-(
- 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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- Improve entry
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cpl-plugin-kmos
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1.3.5+dfsg-1
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ESO data reduction pipeline for the KMOS instrument
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cpl-plugin-kmos:
ESO data reduction pipeline for the KMOS instrument
- Description
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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
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- Versions
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- Popularity
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41 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-muse
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2.6+dfsg-1
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??? missing short description for package cpl-plugin-muse :-(
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cpl-plugin-muse:
??? missing short description for package cpl-plugin-muse :-(
- Reference
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- Maintainer
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- Versions
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- Popularity
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79 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-naco
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4.4.11+dfsg-1
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??? missing short description for package cpl-plugin-naco :-(
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cpl-plugin-naco:
??? missing short description for package cpl-plugin-naco :-(
- Maintainer
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- Versions
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- Popularity
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84 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-sinfo
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2.5.2+dfsg-2
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??? missing short description for package cpl-plugin-sinfo :-(
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cpl-plugin-sinfo:
??? missing short description for package cpl-plugin-sinfo :-(
- Reference
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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
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- Versions
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- Popularity
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3 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-uves
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5.9.1+dfsg-1
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??? missing short description for package cpl-plugin-uves :-(
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cpl-plugin-uves:
??? missing short description for package cpl-plugin-uves :-(
- Maintainer
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- Versions
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- Popularity
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79 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-vimos
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3.1.7+dfsg-1
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??? missing short description for package cpl-plugin-vimos :-(
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cpl-plugin-vimos:
??? missing short description for package cpl-plugin-vimos :-(
- Maintainer
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- Versions
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- Popularity
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82 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-visir
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4.3.0+dfsg1-1
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??? missing short description for package cpl-plugin-visir :-(
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cpl-plugin-visir:
??? missing short description for package cpl-plugin-visir :-(
- Maintainer
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- Versions
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- Popularity
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81 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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cpl-plugin-xshoo
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2.8.4+dfsg-3
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ESO data reduction pipeline for the XSHOOTER instrument
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cpl-plugin-xshoo:
ESO data reduction pipeline for the XSHOOTER instrument
- Description
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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
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- Versions
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- Popularity
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23 total installations
(of 247608 submissions)
- Debian
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- Upstream
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- Improve entry
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