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Flexible Spectro Interferometric modelling of OIFITS data with PMOIRED

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arxiv 2207.11047 v1 pith:NMADVMVV submitted 2022-07-22 astro-ph.IM

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keywords dataoifitspmoiredbecauseflexiblemodelmodellingsimple
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Despite image reconstruction becoming more widespread when interpreting OIFITS Data, model fitting in u,v space often remains the best way to interpret data, either because of the sparsity of the data, or because a quantitative measurement needs to be done. PMOIRED, is a flexible Python library to visualize, manipulate and model OIFITS data using simple geometric models. The strength of PMOIRED resides in its capability to combine linearly various simple components to create complex scenes, while linking, constraining, and adding priors to fitted parameters. The code also enables grid search to find global minima, as well as data resampling to better evaluate uncertainties. In addition to analytical functions, arbitrary radial profiles, azimuthal variations or sparse wavelet modelling of spectra are implemented.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Toward 3D orbits of wide sdO/B binaries I. Six composite systems spatially resolved with VLTI/GRAVITY

    astro-ph.SR 2026-07 conditional novelty 6.0 of 10

    VLTI/GRAVITY spatially resolved six wide sdO/B+MS binaries, yielding 1-8% precise projected separations of 1-3 au — the first interferometric sample toward 3D orbits and model-independent masses.

  2. HD 143006: Interferometric Confirmation of Misaligned Protoplanetary Disc with CHARA/MIRCX and VLTI/PIONIER

    astro-ph.EP 2025-06 conditional novelty 6.0 of 10

    The inner disc of HD 143006 is directly measured to be misaligned by 39 ± 4 degrees from the outer disc, confirming that this misalignment casts the observed shadows.

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