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Allegro Software Repository

Scientific exploration of ALMA observations does not stop when an image is produced: there exists a wide range of tools that can be used to further explore your ALMA data, plot and inspect parts of your ALMA data, and compare your ALMA data to models of astrophysical objects. Many of the tools that are developed by the scientific community are publicly available.

To help ALMA users navigate the many options and find tools that they may not even know exist, Allegro, with the help of the European ARC node network, has developed an interactive inventory to ALMA-related software. This inventory is not intended to be complete and will always keep growing. If you know of useful tools to be added, or find an inaccuracy, please contact us at alma@strw.leidenunv.nl.

For each piece of software we list the name of the piece of software along with a link to its website, a short description taken from the software's website, a description of experience with the software within the ARC nodes, a list of tags for the software and notes about the software. More information about the ARC Nodes experience field and the Tags field is provided below.

ARC Nodes experience

For each piece of software in the catalogue, a descriptor of the current status of how recently experience has been reported with the software by staff in the ARC Nodes is given in the “Status” column. The different statuses are as follows:

  • Recent experience (<1 year ago) at the ARC nodes
  • Experience 1-2 years ago at the ARC nodes
  • Experience >2 years ago at the ARC nodes
  • No or uncertain experience at the ARC nodes

Staff at the ARC nodes are less likely to have experience with software with a status further down this list.

List of software

This is a searchable and sortable table of software listed in the software repository. Click on the arrows next to column titles to sort by that column. You can also use the search box to filter the content, for example try searching Working recently to see only working software that is listed as working recently. Software is also tagged with a number of properties that you can search by, for example try searching #visualisation to see software that can be used for visualisation.

The full list of tags is: #analysis, #archive, #calibration, #CASA, #datacubes, #GILDAS, #GPU_computing, #modeling, #modelling, #moments, #observing, #polarisation, #polarization, #python, #simulation, #visibilities, #visualisation, #visualization, #VLBI

There are currently 42 pieces of software in the repository.

Filter:

Software Description ARC Node experience Status Tags Notes
3D-Barolo 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. No or uncertain experience #analysis #datacubes #modeling #modelling #python A paper on the tool can be found at https://ui.adsabs.harvard.edu/abs/2015MNRAS.451.3021D/abstract
ADMIT The ALMA Data Mining Toolkit (ADMIT) is a value-added Python software package which integrates with the ALMA archive and CASA to provide scientists with quick access to traditional science data products such as moment maps, as well as with new innovative tools for exploring data cubes and their many derived products. No or uncertain experience #archive #CASA #python
ALMA FITS Keywords filler The ALMA Keywords Filler (AKF) CASA task is build to generate and eventually ingest in the headers the new FITS keywords that we suggest could be useful for a generic ALMA archive miner. No or uncertain experience #archive #CASA #python The AKF command functions as a normal CASA function, typing inp(AKF) will show input options. A CASA memo on the tool can be accessed at https://www.alma.inaf.it/images/AKF_v1.2.pdf
ALMA Observing Tool 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). It is also used for preparing and submitting Director's Discretionary Time (DDT) proposals and Supplemental Call (ACA stand-alone) proposals. Recent experience #observing
ALminer alminer is a Python-based code to effectively query, analyse, and visualize the ALMA science archive. It also allows users to directly download ALMA data products and/or raw data for further image processing. Recent experience #archive #python #visualisation #visualization There is an online tutorial notebook that showcases alminer's various functions with examples. There is an I-TRAIN training avaliable for ALminer, with recording of the session avaliable as a YouTube video. Full details can be found on I-TRAIN website under the heading I-TRAIN #8: Exploring the ALMA Science Archive with ALminer
APSYNSIM Aperture Synthesis Simulator for Radio Astronomy. Based on python/matplotlib, it is fully interactive and the plots are updated almost in real time. Antennas can be dragged with the mouse. Number of antennas, observing frequency, observatory-source coordinates, visibility weighting, etc. can be changed on the fly. No or uncertain experience #python #simulation An arXiv paper on the tool can be found at https://ui.adsabs.harvard.edu/abs/2017arXiv170600936M/abstract
ARTIST ARTIST (Adaptable Radiative Transfer Innovations for Submillimeter Telescopes) is a set of two CASA tools that allow you to select one of nine pre-coded astrophysical models describing young stellar objects, planet forming disks, or circumstellar shells; adapt the parameters of these models; calculate the excitation of a user-selected molecule using the LIME (LIne Modeling Engine) accelerated monte-carlo code; and calculate the (sub) millimeter line emission of this object at a specified distance and orientation. Experience >2 years ago #CASA #modeling #modelling #python
ASTRO Dedicated to ephemeris and observation preparation. Recent experience #GILDAS #observing
Astroquery Astroquery is a set of tools for querying astronomical web forms and databases. Recent experience #archive #python
Better Moments bettermoments creates moment maps of spectral line data and their associated uncertainties. The command-line interface makes it as seamless as possible to make all the traditional moment maps, in addition other, oftentimes more useful, maps. In addition to the many traditional statistical moments, bettermoments contains many alternative ways collapse the cube. No or uncertain experience #datacubes #moments #python
CARTA Cube Analysis and Rendering Tool for Astronomy, is a next generation image visualization and analysis tool designed for ALMA, VLA, and SKA pathfinders. Recent experience #datacubes #python #visualisation #visualization There is an I-TRAIN training avaliable for LineStacker, with recording of the session avaliable as a YouTube video. Full details can be found on the I-TRAIN website under the heading I-TRAIN #12: CARTA tutorial
CASA CASA, the Common Astronomy Software Applications, is the primary data processing software for the Atacama Large Millimeter/submillimeter Array (ALMA) and Karl G. Jansky Very Large Array (VLA), and is often used also for other radio telescopes. Recent experience #calibration #CASA #datacubes #moments #python #visibilities
CASAIRING Simple task to compute radial profiles of images (and image cubes). It generates plots and ascii files with the profile values. Recent experience #CASA #python The casairing command functions as a normal CASA function, typing inp(casairing) will show input options and help casairing will some some example of how to use the function.
CASSIS A free interactive spectrum analyser. Recent experience #modeling #modelling #simulation Allegro has developed a simple cookbook that describes how to use CASSIS with a special emphasis on ALMA observations. It can be accessed from this link.
CHECKRES CASA interactive task for a quick check of image residuals, but in Fourier space. It overplots the UV tracks of the baselines corresponding to selected antennas, so it should be easy to locate the antennas (and/or baselines) responsible of dynamic-range limitations. Recent experience #CASA #python The checkres command functions as a normal CASA function, typing inp(checkres) will show input options.
closures CASA task to plot closure phases (or amplitudes) vs. time or frequency. Recent experience #CASA #python The closures command functions as a normal CASA function, typing inp(closures) will show input options.
FAKEOBS FAKEOBS is a CASA task to generate model visibilities from already-existing measurement sets. Recent experience #CASA #python #simulation The fakeobs command functions as a normal CASA function, typing inp(fakeobs) will show input options.
galario galario is a library that exploits the computing power of modern graphic cards (GPUs) to accelerate the comparison of model predictions to radio interferometer observations. No or uncertain experience #GPU_computing #modeling #modelling #python #visibilities
Glue Glue is an open-source Python library to explore relationships within and between related datasets No or uncertain experience #python #visualisation #visualization
GoFish No or uncertain experience #python A paper on the tool can be found at https://ui.adsabs.harvard.edu/abs/2019JOSS....4.1632T/abstract
Interferopy A Python library of common tasks used in the observational radio/mm interferometry data analysis. The package was developed to aid in the studies of the interstellar medium in high-redshift quasar host galaxies using emission lines, as well as to create publication quality plots. No or uncertain experience #python #visualisation #visualization
jupyter-casa A Jupyter kernel for CASA. No or uncertain experience #CASA #python
LIME LIME is a 3D molecular excitation and radiation transfer code for far-infrared and (sub-)millimeter wavelength. LIME will calculate spectra of rotational transitions of atoms and molecules, given a user-supplied physical model. Experience >2 years ago #modeling #modelling A paper on the tool can be found at https://ui.adsabs.harvard.edu/abs/2010A%26A...523A..25B/abstract
LineStacker LineStacker is a new open access tool for stacking of spectral lines. LineStacker is an ensemble of both CASA tasks and native python tasks, and can stack both 3Dcubes or already extracted spectra. Additionaly a set of tools are included to help further analyse stacked spectra and stacked sample. No or uncertain experience #analysis #python There is an I-TRAIN training avaliable for LineStacker, with a recording of the session avaliable as a YouTube video. Full details can be found on the I-TRAIN website under the heading I-TRAIN #9: Stacking spectra in the image domain with LineStacker.
MAPPING Dedicated to imaging and deconvolution of aperture synthesis data; MAPPING also includes an ALMA simulator. Recent experience #GILDAS #visibilities #visualisation #visualization
Molecular EMissiOn IdentifieR (MEMOIR) MEMOIR detects the lines present in a spectrum and identifies them by comparing their frequencies against those of known-lines. No or uncertain experience #analysis #python
Photutils Photutils is an affiliated package of Astropy that primarily provides tools for detecting and performing photometry of astronomical sources. No or uncertain experience #analysis #python
PolConvert Advanced polarization calibration of linear feeds in VLBI observations. No or uncertain experience #calibration #polarisation #polarization #python #VLBI
POLSIMULATE CASA task for a basic simulator of ALMA/J-VLA full-polarization observations. Recent experience #CASA #polarisation #polarization #python #simulation The polsimulate command functions as a normal CASA function, typing inp(polsimulate) will show input options.
Position-Velocity Slice Extractor The concept of the pvextractor package is simple - given a path defined in sky coordinates, and a spectral cube, extract a slice of the cube along that path, and along the spectral axis, producing a position-velocity or position-frequency slice. No or uncertain experience #datacubes #python #visualisation #visualization
pyuvdata pyuvdata defines a pythonic interface to interferometric data sets. Currently pyuvdata supports reading and writing of miriad, uvfits, CASA measurement sets and uvh5 files and reading of FHD (Fast Holographic Deconvolution) visibility save files, SMA Mir files and MWA correlator FITS files. No or uncertain experience #python #visibilities
RADEX Radex is a computer program to calculate the strengths of atomic and molecular lines from interstellar clouds which are assumed to be homogeneous. No or uncertain experience #modeling #modelling #simulation A paper on the tool can be found at https://ui.adsabs.harvard.edu/abs/2007A%26A...468..627V/abstract
Radio Beam A simple toolkit for reading and manipulating beams from astrophysical radio spectral data cubes. No or uncertain experience #python
RADMC3D RADMC-3D is a code package for diagnostic radiative transfer calculations in astronomy and astrophysics. It calculates, for a given geometrical distribution of gas and/or dust, what its images and/or spectra look like when viewed from a certain angle, allowing modelers to compare their models with observed data. No or uncertain experience #python #simulation
SD2vis CASA task to generate synthetic visibilities based on a Total-Power (Single Dish) image. Recent experience #CASA #python #simulation #visibilities The SD2vis command functions as a normal CASA function, typing inp(SD2vis) will show input options.
Spectral Cube The spectral-cube package provides an easy way to read, manipulate, analyze, and write data cubes with two positional dimensions and one spectral dimension, optionally with Stokes parameters. Recent experience #datacubes #moments #python
STACKER STACKER is a library for stacking sources in interferometric data, i.e., averaging emission from different sources. The library allows stacking to be done directly on visibility data as well as in the image domain. No or uncertain experience #analysis #python #visibilities
STATCONT STATCONT is a python-based tool designed to determine the continuum emission level in line-rich spectral data. The tool inspects the intensity distribution of a given spectrum and automatically determines the continuum level by using different statistical approaches. No or uncertain experience #python There is an I-TRAIN training avaliable for LineStacker, with a recording of the session avaliable as a YouTube video. Full details can be found on the I-TRAIN website under the heading I-TRAIN #11: Statistical continuum determination with STATCONT
uvmultifit A CASA-based flexible visibility-fitting engine developed at the Nordic node of the ALMA Regional Center. Recent experience #CASA #python #visibilities There is an I-TRAIN training avaliable for uvmultifit, with recording of the session avaliable as a YouTube video. Full details can be found on I-TRAIN website under the heading I-TRAIN #3: UVMultiFit
UVPLOT A simple Python package to make nice plots of deprojected interferometric visibilities, often called uvplots. No or uncertain experience #python #visibilities Some functionality is only available if imported within CASA
WVR Scaling Module Software package to optimise the application of the WVR solutions for ALMA Observations. No or uncertain experience #calibration #CASA #python Requires astropy version 1.3.3 and CASA < 5.0 (CASA 4.7.2 is the latest working version). A paper on the tool can be found at https://ui.adsabs.harvard.edu/abs/2017A%26A...605A.121M/abstract
XCLASS A toolbox for the Common Astronomy Software Applications package (CASA) containing a couple of new functions for modelling interferometric and single dish data. No or uncertain experience #CASA #modeling #modelling #python #visibilities

allegrosoftwarerepo/index.1669130842.txt.gz · Last modified: by michiel

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