codemeta.json

{
    "@context": "https://doi.org/10.5063/schema/codemeta-2.0",
    "@type": "SoftwareSourceCode",
    "name": "MARTINI: Mock spatially resolved spectral line observations of simulated galaxies",
    "description": "MARTINI (Mock Array Radio Telescope Interferometry of the Neutal ISM) creates synthetic resolved HI line observations (data cubes) of smoothed-particle hydrodynamics simulations of galaxies. The various aspects of the mock-observing process are divided logically into sub-modules handling the data cube, source, beam, noise, spectral model and SPH kernel. MARTINI is object-oriented: each sub-module provides a class (or classes) which can be configured as desired. For most sub-modules, base classes are provided to allow for straightforward customization. Instances of each sub-module class are given as parameters to the Martini class; a mock observation is then constructed by calling a handful of functions to execute the desired steps in the mock-observing process.",
    "identifier": "ascl:1911.005",
    "author": [
        {
            "@type": "Person",
            "givenName": "Kyle A.",
            "familyName": "Oman",
            "@id": "0000-0001-9857-7788",
        },
    ],
    "citation": "https://ui.adsabs.harvard.edu/abs/2019ascl.soft11005O",
    "relatedLink": [
        "https://pypi.org/project/astromartini",
    ],
    "codeRepository": [
        "https://github.com/kyleaoman/martini",
    ],
    "version": "2.1.9",
    "license": "https://spdx.org/licenses/GPL-3.0-only.html",
}