Modelling of Astrophysical Observables for the Very Large Telescope Interferometer

Details Modelling of Astrophysical Observables for the Very Large Telescope Interferometer Modelling of Astrophysical Observables for the Very Large Telescope Interferometer

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..589t&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

For a 2, 3 and even 4 telescopes interferometer, the sparse UV coverage will generally not allow to reconstruct the image of the object. The only way to interpret the physical observables (visibility, closure phase and differential phase) is via a model of the object. The Mariotti Center is studying the development of a MODEL software package which will allow the user to implement its own analytic model of the object spatial spectrum, and to compute automatically the maximum likelihood estimates of the model parameters. We describe this module.

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