Irasoft: Difference between revisions

From Istituto di Radioastronomia
Jump to navigation Jump to search
No edit summary
Line 55: Line 55:
|-
|-
|[https://heasarc.gsfc.nasa.gov/fitsio/ 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  
|[https://heasarc.gsfc.nasa.gov/fitsio/ 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
|-
|[https://github.com/idl-coyote/coyote 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
|-
|[https://github.com/discos/discos2class discos2class]||A command line tool used to convert DISCOS spectroscopy files acquired with XARCOS into CLASS native format||current||current master
|-
|-
|[https://numpy.org/ 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  
|[https://numpy.org/ 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
|-
|-
|[https://pyfits.readthedocs.io/en/latest/ pyfits]||The PyFITS module is a Python library providing access to FITS files.||3.4||3.4  
|[https://pyfits.readthedocs.io/en/latest/ 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
|-
|[https://johannesbuchner.github.io/PyMultiNest/ 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
|-
|[https://github.com/jive-vlbi/sched/archive/python.zip 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
|-
|[https://www.qt.io/ 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
|-
|-
|[https://www.tensorflow.org/ 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  
|[https://www.tensorflow.org/ 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
|-
|-
|}
|}

Revision as of 12:59, 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
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 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
Retrieved from "https://wiki.ira.inaf.it/index.php?title=Irasoft&oldid=614"