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Programmi
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. | 10.076 | 10.076 |
allantools | A python library for calculating Allan deviation and related time & frequency statistics | 2018.3 | 2018.3 master |
analytic_infall | load Analytic Infall Models | 1.5 | 1.5 |
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 |
apsynsim | load apsynsim | 1.4 | 1.4 |
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 |
boost | Boost provides free peer-reviewed portable C++ source libraries. | 1.72.0 | 1.64.0 1.72.0 default |
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 |
captain | 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 | pipe | pipe |
carma_miriad | MIRIAD (Multichannel Image Reconstruction, Image Analysis and Display) is a toolbox, in the form of an environment with a large set of moderate-sized programs which perform individual tasks, involving calibration, mapping, deconvolution and image analysis of interferometric data | 4.3.8 | 4.3.8 |
carta | load Carta viewer | 1.4-RedHat7 | 1.2.2 1.4-RedHat7 v1.4-ubuntu |
casacore | The casacore package contains the core libraries of the old AIPS++/CASA package. This split was made to get a better separation of core libraries and applications. | 2.4.1 | 1.7.0 2.3.0 2.3.0-src 2.4.1 casacore-1.7.0 default |
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 | 34.0.19988-002-64b 42.1.29047-001-1-64b 42.2.30986-pipe-1-64b 4.3.0 4.3.1 4.5.1 4.5.27 6.1.0-118 default feature-CAS-10684-13.el6 feature-CAS-9108-11.el7 pipeline-release-5.6.1-8.el7 pipeline-release-5.6.2-2.el7 release-4.3.1-pipe-el6 release-4.3.1-pipe-el6.old release-4.4.0-el6 release-4.5.0-el6 release-4.5.2-el6 release-4.5.3-el6 release-4.6.0-el6 release-4.7.0-1-el7 release-4.7.0-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 stable-4.6.28 |
centos | a CentOS container able to run all IRA software | 7.202702 | 7 7.202702 default |
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 |
dysco | A compressing storage manager for Casacore measurement sets | 1.2 | 1.0.1 1.2 default |
funtools | Funtools is a FITS library and utility package originally developed at the the High Energy Astrophysics Division of SAO. Although no longer actively supported at SAO, it is still widely used within the astronomical community, especially among X-ray astronomers. | 1.4.7 | 1.4.7 default |
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 | 5.0.0 | 5.0.0 5.0.0-src |
idl | IDL, short for Interactive Data Language, is a programming language used for data analysis. | 85 | 80 82 85 86 87 |
ipython | load ipython console | 5.7.0 | 5.0.0 5.7.0 |
jdk | The JDK includes a private JVM and a few other resources to finish the development of a Java application. | 1.8.0_05 | 1.8.0_05 |
jre | the Java Runtime Environment | 1.8.0_102 | 1.7.0_05 1.8.0_102 1.8.0_73 1.8.0_91 |
karma | Karma is a toolkit for interprocess communications, authentication, encryption, graphics display, user interface and manipulating the Karma network data structure. | 1.7.25 | 1.7.25 current |
kern | KERN is a bi-annually released set of radio astronomical software packages. It should contain most of the standard tools that a radio astronomer needs to work with radio telescope data | 201119 | 181127.12 190722.11 201119 |
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 | 20110310 20120607 20130221 20141023 20150702 20160721 20190625 |
mpi4py | mpi4py python module | 3.0.0 | 3.0.0 |
multinest | load multinest library | 3.10 | 3.10 |
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 2.4 2.5 2.6 2.6_old 2.7 2.7_old 2.8 2.8.1 default |
xephem | XEphem is a star-charting, sky-simulating, ephemeris-generating program. | 3.7.7 | 3.7.7 |