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VLTI technical advances: present and future
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2004
Year
EngineeringExperimental TechnologySpace OpticVlti Technical AdvancesInstrumentation EngineeringActive OpticsAstronomical Image AnalysisInfrared OpticElectronic PackagingInstrumentationObservational CosmologyElectrical EngineeringPhotometryRadio TelescopeMicroelectronicsNorthern ChileAstrophysicsAdaptive OpticVlsi ArchitectureFirst FringesAdaptive OpticsVlsi
The Very Large Telescope Interferometer (VLTI) on Cerro Paranal (2635 m) in Northern Chile reached a major milestone in September 2003 when the mid infrared instrument MIDI was offered for scientific observations to the community. This was only nine months after MIDI had recorded first fringes. In the meantime, the near infrared instrument AMBER saw first fringes in March 2004, and it is planned to offer AMBER in September 2004. The large number of subsystems that have been installed in the last two years - amongst them adaptive optics for the 8-m Unit Telescopes (UT), the first 1.8-m Auxiliary Telescope (AT), the fringe tracker FINITO and three more Delay Lines for a total of six, only to name the major ones - will be described in this article. We will also discuss the next steps of the VLTI mainly concerned with the dual feed system PRIMA and we will give an outlook to possible future extensions.