Interferometry basics in practice: Exercises |
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Authors: | Florentin Millour Damien Sgransan Jean-Philippe Berger Gilles Duvert Fabien Malbet |
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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 |
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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. |
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Keywords: | Optical long-baseline interferometry Visibility Phase UV coverage VLTI ASPRO |
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