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Exercise #1 Modeling an astrophysical source in preparation for interferometric observations

Published online by Cambridge University Press:  31 January 2003

G. Perrin ,
F. Malbet ,
J.-P. Berger ,
E. Tatulli  and
E. Lecoarer
J.-P. Berger
Affiliation:
Harvard Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
E. Tatulli
Affiliation:
Laboratoire d'Astrophysique de l'Observatoire de Grenoble, BP. 53, Grenoble Cedex 9, France
E. Lecoarer
Affiliation:
Harvard Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA Laboratoire d'Astrophysique de l'Observatoire de Grenoble, BP. 53, Grenoble Cedex 9, France
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Abstract

The following exercices are aimed to get trained to the link between theobject intensity distribution and the corresponding visibilitycurves. They were intended to be the practical application of theseminar "Introduction to visibility modeling" (Berger samevolume). This practical session was initially meant to be done with theASPRO software (see Duvert same volume), uv tables and the fits filecan be donwloaded from the ASPRO website. However, any imageprocessing or mathematical software (Idl, Yorick, Mathlab, Mathematica...) associated with the object equations given in Berger can be usedfor most exercises.

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Type
Research Article
Information
European Astronomical Society Publications Series , Volume 6: Observing with the VLTI , 2003 , pp. 43
Copyright
© EAS, EDP Sciences, 2003

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