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Interferometry basics in practice: Exercises
Authors:Florentin Millour  Damien Sgransan  Jean-Philippe Berger  Gilles Duvert  Fabien Malbet
Institution:aMax-Planck-Institut für Radio-astronomie, Auf dem Hügel 69, 53121 Bonn, Germany;bObservatoire Astronomique de l’Université de Genève, 51, chemin des Maillettes, CH-1290 Sauverny, Switzerland;cLaboratoire d’Astrophysique, Observatoire de Grenoble, 414, Rue de la Piscine, Domaine Universitaire, 38400 Saint-Martin d’Hères, France
Abstract:The following exercises aim to learn the link between the object intensity distribution and the corresponding visibility curves of a long-baseline optical interferometer. They are also intended to show the additional constraints on observability that an interferometer has.This practical session is meant to be carried out with the ASPRO software, from the Jean-Marie Mariotti Center, but can also be done using other observation preparation software, such as viscalc from ESO.There are two main parts with series of exercises and the exercises corrections. The first one aims at understanding the visibility and its properties by practicing with simple examples, and the second one is about UV coverage.
Keywords:Optical long-baseline interferometry  Visibility  Phase  UV coverage  VLTI  ASPRO
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