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What to do next?

More than a thousand procedures and functions available in $\cal OYST\!ER $ support three main tasks: reducing and calibrating one night's interferometric data, as well as scheduling and HDS file access (this collection is referred to as CHAMELEON), computing stellar models and fitting them to the data (AMOEBA), and creating and managing stellar data bases and catalogs (STARBASE). Please refer to that part of this guide which is appropriate for your task. Note that many of the scripts are interdependent and share resources.

Christian Hummel 2017-06-29