Irasoft

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.	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

Librerie

name	description	default version	available versions
ase	The Atomic Simulation Environment (ASE) is a set of tools and Python modules for setting up, manipulating, running, visualizing and analyzing atomistic simulations	3.12.0	3.11.0_old 3.12.0 3.13.0
astron	A collection of low-level routines, mainly related to astronomy, written in the commercial language IDL. needs coyote-setup.	2018-02-16	2011-05-16 2011-08-19 2014-01-14 2016-05-25 2018-02-16 current Nov2007 Sep2004
astropy	The Astropy Project is a community effort to develop a core package for astronomy using the Python programming language and improve usability, interoperability, and collaboration between astronomy Python packages	2.0.6	1.0.3-old 1.0.3-src 1.2.1 2.0.2 2.0.6 3.0.2
astroquery	Astroquery is a set of tools for querying astronomical web forms and databases.	0.3.9	0.3.2 0.3.2.old 0.3.7 0.3.9 0.3.dev2794
atlas	load atlas library	3.10.2	3.10.2 default
cfitsio	CFITSIO is a library of C and Fortran subroutines for reading and writing data files in FITS (Flexible Image Transport System) data format.	3.47	3360 3370 3420 3440 3450 3450.old 3.47 default
numpy	NumPy is a library for the Python programming language, adding support for large, multi-dimensional arrays and matrices, along with a large collection of high-level mathematical functions to operate on these arrays.	1.19.4	1.11.2 1.11.2.old 1.14.2 1.14.3 1.15.4 1.16.6 1.19.4 default
pyfits	The PyFITS module is a Python library providing access to FITS files.	3.4	3.4
tensorflow	TensorFlow is an end-to-end open source platform for machine learning. It has a comprehensive, flexible ecosystem of tools, libraries and community resources that lets researchers push the state-of-the-art in ML and developers easily build and deploy ML powered applications.	2.3.1-cp37	1.11.0 1.13.1 1.14.0 2.0.0b1 2.3.1-cp37

Sviluppo

name	description	default version	available versions
gcc	The GNU Compiler Collection includes front ends for C, C++, Objective-C, Fortran, Ada, Go, and D, as well as libraries for these languages (libstdc++,...)	8.2.0	8.2.0 infrastructure
go	Go is an open source programming language that makes it easy to build simple, reliable, and efficient software.	1.15.2	1.15.2
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
llvm	The LLVM Project is a collection of modular and reusable compiler and toolchain technologies	10.0.0	10.0.0 default
R	load the R language and environment. needs gcc-setup.	3.6.0	3.1.0 3.6.0

Ambienti

name	description	default version	available versions
centos	a CentOS container able to run all IRA software	7.202702	7 7.202702 default
cuda	A Debian container with cuda toolchain and runtime	10.210112	10.210112
debian	A Debian container taylored to run IRA software	10.210114	10 10.201105 10.201116 10.201130 10.201209 10.210114 default
jre	the Java Runtime Environment	1.8.0_102	1.8.0_102
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	201119
lofar	A singularity image containing the IRA LOFAR software environment	191118.16	191003.13 191107.16 191111.19pub 191118.16 191121.15pub 191205.13pub 200323.12 d10.201020.09-ddf-private d10.201223-pybdsf default public