Irasoft: Difference between revisions

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|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  
|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  
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|allantools||A python library for calculating Allan deviation and related time & frequency statistics||2018.3||2018.3 master
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|analytic_infall||load Analytic Infall Models||1.5||1.5
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|[https://gitlab.com/aroffringa/aoflagger 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  
|[https://gitlab.com/aroffringa/aoflagger 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  
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|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  
|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  
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|apsynsim||load apsynsim||1.4||1.4
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|[https://editeodoro.github.io/Bbarolo/ 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  
|[https://editeodoro.github.io/Bbarolo/ 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  
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|[https://www.boost.org/ boost]||Boost provides free peer-reviewed portable C++ source libraries.||1.72.0||1.64.0 1.72.0 default
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|[http://www.askanastronomer.co.uk/brats/ 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  
|[http://www.askanastronomer.co.uk/brats/ 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  
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|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
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|[https://www.mmarray.org/ 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
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|[https://cartavis.github.io/ carta]||load Carta viewer||1.4-RedHat7||1.2.2 1.4-RedHat7 v1.4-ubuntu  
|[https://cartavis.github.io/ carta]||load Carta viewer||1.4-RedHat7||1.2.2 1.4-RedHat7 v1.4-ubuntu  
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|[https://casacore.github.io/casacore/ 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
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|[https://casa.nrao.edu/ 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  
|[https://casa.nrao.edu/ 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  
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|centos||a CentOS container able to run all IRA software||7.202702||7 7.202702 default
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|[https://github.com/discos/discos2class 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  
|[https://github.com/discos/discos2class 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  
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|[https://github.com/aroffringa/dysco dysco]||A compressing storage manager for Casacore measurement sets||1.2||1.0.1 1.2 default
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|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
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|fv||Fv is an easy to use graphical program for viewing and editing any FITS format image or table.||5.3||5.3
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|[https://gcc.gnu.org/ 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  
|[https://gcc.gnu.org/ 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  
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|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
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|idl||IDL, short for Interactive Data Language, is a programming language used for data analysis.||85||80 82 85 86 87  
|idl||IDL, short for Interactive Data Language, is a programming language used for data analysis.||85||80 82 85 86 87  
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|ipython||load ipython console||5.7.0||5.0.0 5.7.0
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|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
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|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
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|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
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|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
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|[https://www.ira.inaf.it/lofar/ 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  
|[https://www.ira.inaf.it/lofar/ 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  
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|mpi4py||mpi4py python module||3.0.0||3.0.0
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|multinest||load multinest library||3.10||3.10
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|[https://gitlab.com/aroffringa/wsclean 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  
|[https://gitlab.com/aroffringa/wsclean 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  
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|xephem||XEphem is a star-charting, sky-simulating, ephemeris-generating program.||3.7.7||3.7.7
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Revision as of 12:58, 10 December 2020

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
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 load Carta viewer 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 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
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
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
idl IDL, short for Interactive Data Language, is a programming language used for data analysis. 85 80 82 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 20110310 20120607 20130221 20141023 20150702 20160721 20190625
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


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
ciao CIAO is the software package developed by the Chandra X-Ray Center for analysing data from the Chandra X-ray Telescope. It can also be used with data from other Astronomical observatories, whether ground or space based. 4.9 4.9
contbin Contour binning - https://www-xray.ast.cam.ac.uk/papers/contbin/ 1.4 1.4
coyote The Coyote Library evolved from work David Fanning was doing teaching IDL courses and answering IDL questions on the IDL newsgroup. 20180306 2014-01 20180306 29apr2013
cpan load cpan modules current current
debian A Debian container taylored to run IRA software 10.201209 10 10.201105 10.201116 10.201130 10.201209 default
discos2class A command line tool used to convert DISCOS spectroscopy files acquired with XARCOS into CLASS native format current current master
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
obit load Astronomy Software for Algorithm Development 22JUN10h 1.1.387-6 1.1.387-6-64b 1.1.479-1-64b 1.1.502-1-64b 22JUN10h
OpenBLAS OpenBLAS is an open-source implementation of the BLAS (Basic Linear Algebra Subprograms) and LAPACK APIs 0.3.10 0.3.10 default
pandas load pandas 0.23.4 0.20.1 0.22.0 0.23.4
parseltongue load parseltongue 2.1 2.1
pgplot loads pgplot 5.2 5.2 default
pit load LBTO Phase I Tool 2017B.2.0.0_linux64 2017B.2.0.0_linux64
ppgplot load python pgplot bindings 1.4 1.4
presto load presto 2.1 2.1
pvextractor load pvextractor git git
pyfits The PyFITS module is a Python library providing access to FITS files. 3.4 3.4
pymc PyMC is a Python package for Bayesian statistical modeling and probabilistic machine learning which focuses on advanced Markov chain Monte Carlo and variational fitting algorithms. 2.3.6 2.3.6
pymultinest PyMultiNest is a module to use the MultiNest sampling engine. 2.6 2.6
pyparsing pyparsing python module 2.2.0 2.2.0
pyrmsynth defines the pyrmsynth environment master 1.3.0 master
pysched pySCHED is a program for planning and scheduling very long baseline interferometry (VLBI) observations conducted by different networks such as the European VLBI Network (EVN), the Very Long Baseline Array (VLBA), the High Sensitivity Array (HSA), the Global VLBI, the Australian Long Baseline Array (LBA), or the Korean VLBI Network (KVN). pySCHED produces the standard files that need to be distributed to the different telescopes and correlators for VLBI observations and operations. 1.14.0 1.14.0 1.14.1 default
pysic load the pysic python module 0.6 0.6 0.6.old
python3 load python3 3.7.2 3.7.2
python-casacore load python casacore bindings 2.2.1 2.2.1
pyvo load pyvo 0.9.2 0.9.2
pywcs pywcs python module 1.12 1.12
qa2 load qa2 svn svn
qt Qt is a free and open-source widget toolkit for creating graphical user interfaces as well as cross-platform applications that run on various software and hardware platforms 5.12.3 4.7.4 4.8.7 5.12.3 default
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
tirific Tilted Ring Fitting Code (TiRiFiC) is a computer program to construct simulated (high-resolution) astronomical spectroscopic 3d-observations (data cubes) of simple kinematical- and morphological models of rotating (galactic) disks. 2.3.4 2.3.4 2.3.4_old
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. 4.6-3 4.5-1 4.6-1 4.6-3
udr load udr 0.9.4 0.9.4 master
wip load WIP 2p3 2p3

Sviluppo

name description default version available versions
gcc load the GNU C Compiler 8.2.0 4.6-20110603 4.6-20130405 4.7-20110423 4.8-20131121 4.8-20140501 4.8-infrastructure 4.9-20131110 8.2.0 infrastructure
go load the GO programming language 1.15.2 1.15.2
gsl The GNU Scientific Library (GSL) is a numerical library for C and C++ programmers. 2.5 2.5 2.5-src default
hdf5 Hierarchical Data Format (HDF) is a set of file formats (HDF4, HDF5) designed to store and organize large amounts of data. 1.8.20 1.8.20 1.8.20-src current default
healpix HEALPix is an acronym for Hierarchical Equal Area isoLatitude Pixelation of a sphere. As suggested in the name, this pixelation produces a subdivision of a spherical surface in which each pixel covers the same surface area as every other pixel. 3.31 2.20a 3.00 3.31
heasoft A Unified Release of the FTOOLS and XANADU Software Packages. 6.24 6.16 6.24 6.25 6.26.1
hipe defines the casapy environment 12.1.0 12.1.0
llvm The LLVM Project is a collection of modular and reusable compiler and toolchain technologies 10.0.0 10.0.0 default
lofar A singularity image containing the LOFAR software environment 191118.16 190103 190103.16 190129.15 190307.12 190311.18 190312.11 190313.15 190319.13 190325.12 190429.18 190508.18 190516.17pub 190527.16pub 190611.15pub 190618.15pub 191003.13 191107.16 191111.19pub 191118.16 191121.15pub 191205.13pub 200323.12 2.4 d10.201020.09-ddf-private default public school test ubuntu-190611.11
matlab load matlab R2016b R2016b
matplotlib Matplotlib is a comprehensive library for creating static, animated, and interactive visualizations in Python. screenshots. 2.2.2 1.5.3 2.2.2 2.2.2.old 2.2.2.old2
R load the R language and environment. needs gcc-setup. 3.6.0 3.1.0 3.6.0
scanamorphos load the scanamorphos routines. 23july14 23july14
sciencetools Fermi Science Tools 20140520 20140520
scipy scipy python module 1.5.4 0.15.1 0.17.0 0.18.1 1.1.0 1.5.3 1.5.4 default
sextractor load sextractor 2.19.5 2.19.5 2.19.5-src
singularity A containerization program that can be used to package entire scientific workflows, software and libraries. 3.6.3 2.2 2.2.1 2.3.1 2.4.1 2.4.2 2.5.1 3.4.0 3.5.2 3.6.3 default
sma2casa loads sma2casa master master
spam SPAM is a Python-based extension to AIPS, aimed at reducing high-resolution, low-frequency radio interferometric observations in a very efficient, systematic and reproducible way. 20200617 200219.16 20200617
starlink The Starlink Project was a long running UK Project supporting astronomical data processing. It was shut down in 2005 but the software continued to be developed at the Joint Astronomy Centre until March 2015, and is now maintained by the East Asian Observatory. The code is open source. 2014A 2014A git hikianalia
swarp load swarp 2.38.0 2.38.0 2.38.0-src
tempo load tempo 20190212 20190212
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