Published in

Scientific detectors for astronomy 2005, p. 345-352

DOI: 10.1007/1-4020-4330-9_38

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The OmegaCAM 16Kx16K CCD detector system for the ESO VLT Survey Telescope (VST)

This paper is available in a repository.
This paper is available in a repository.

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Data provided by SHERPA/RoMEO

Abstract

A broad account of the main characteristics of the OmegaCAM 16Kx16K detector system is given. Requirements and additional constraints, design strategy, implementation, and first laboratory results are described for the detector head, cooling system, temperature and shutter control. Synchronization of multiple controllers, and careful safety provisions are explained The system has already passed most acceptance tests and will soon he ready for shipment. Commissioning in Chile is foreseen in 2006.