| name
|
description
|
default version
|
available versions
|
| aips |
The Astronomical Image Processing System is a software package for calibration, data analysis, image display, plotting, and a variety of ancillary tasks on Astronomical Data. It comes from the National Radio Astronomy Observatory. |
31DEC18 |
31DEC13 31DEC14 31DEC15 31DEC16 31DEC18 31DEC18.old
|
| aladin |
Aladin is an interactive sky atlas allowing the user to visualize digitized astronomical images or full surveys, superimpose entries from astronomical catalogues or databases, and interactively access related data and information from the Simbad database, the VizieR service and other archives for all known astronomical objects in the field. |
11.024 |
10.076 11.024
|
| aoflagger |
The AOFlagger is a flagger framework that implements several methods to deal with radio-frequency interference or RFI |
2.13.0 |
2.13.0 2.15.0 default
|
| aot |
The ALMA Observing Tool (OT) is a Java desktop application used for the preparation and submission of ALMA Phase 1 proposals and, for those which are accepted, Phase 2 materials (Scheduling Blocks). |
Cycle4 |
Cycle3PhaseII Cycle4 Cycle4_old Cycle4PhaseII
|
| bbarolo |
3D-Barolo (3D-Based Analysis of Rotating Object via Line Observations) or BBarolo is a tool for fitting 3D tilted-ring models to emission-line data-cubes |
1.3 |
1.3
|
| brats |
BRATS is a software package which provides a variety of tools for the spectral analysis of both new broad-bandwidth radio data, along with legacy support for narrowband telescopes |
2.6.3 |
2.6.3
|
| carta |
Cube Analysis and Rendering Tool for Astronomy, is a next generation image visualization and analysis tool designed for ALMA, VLA, and SKA pathfinders. |
1.4-RedHat7 |
1.2.2 1.4-RedHat7 v1.4-ubuntu
|
| casapy |
CASA, the Common Astronomy Software Applications package, is the primary data processing software for the Atacama Large Millimeter/submillimeter Array (ALMA) and NSF's Karl G. Jansky Very Large Array (VLA), and is frequently used also for other radio telescopes. |
release-5.1.1-5.el7 |
6.1.0-118 6.1.2-7-pipeline-2020.1.0.36 default feature-CAS-9108-11.el7 pipeline-release-5.6.1-8.el7 pipeline-release-5.6.2-2.el7 release-4.7.2-el7 release-5.0.0-218.el7 release-5.1.1-5.el7 release-5.1.2-4.el7 release-5.3.0-143.el7 release-5.4.0-68.el7 release-5.4.0-70.el7 release-5.4.1-31.el7 release-5.5.0-149.el7
|
| difmap |
Difmap is a program developed for synthesis imaging of visibility data from interferometer arrays of radio telescopes world-wide. Its prime advantages over traditional packages, are its emphasis on interactive processing, speed, and the use of Difference mapping techniques. |
2.5e |
2.5e
|
| ds9 |
SAOImageDS9. An image display and visualization tool for astronomical data. |
8.2 |
7.7.5 7.7.6b8 8.0.1 8.2 8.2.deb
|
| fv |
Fv is an easy to use graphical program for viewing and editing any FITS format image or table. |
5.3 |
5.3
|
| gildas |
GILDAS is a collection of state-of-the-art software oriented toward (sub-)millimeter radioastronomical applications (either single-dish or interferometer). |
exe-jun19c |
default exe-jun19c exe-mar18c exe-nov16b exe-oct16a src-jun19c
|
| gnuplot |
gnuplot is a command-line program that can generate two- and three-dimensional plots of functions, data, and data fits |
5.4.1 |
5.0.0 5.4.1
|
| idl |
IDL, short for Interactive Data Language, is a programming language used for data analysis. |
85 |
85 86 87
|
| miriad |
Miriad is a radio interferometry data reduction package of particular interest to users of the Australia Telescope Compact Array (ATCA). It can be used for the reduction of continuum and spectral line observations from beginning to end, starting with the loading of the data (either FITS, the ATNF RPFITS or old BIMA formats) through to image synthesis, analysis and display with publication quality graphics. |
20190625 |
20141023 20150702 20160721 20190625
|
| sofia |
SoFiA 2 is a reimplementation of the original SoFiA pipeline in the C programming language. It is intended for use in HI data analysis pipelines |
2.2.0 |
2.2.0
|
| topcat |
TOPCAT is an interactive graphical viewer and editor for tabular data. Its aim is to provide most of the facilities that astronomers need for analysis and manipulation of source catalogues and other tables, though it can be used for non-astronomical data as well. |
4.8.0 |
4.5-1 4.6-1 4.6-3 4.8.0
|
| wsclean |
WSClean (w-stacking clean) is a fast generic widefield imager. It uses the w-stacking algorithm and can make use of the w-snapshot algorithm. |
2.10.1 |
2.10.1 2.8 2.8.1 default
|