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VISTA (telescope)
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VISTA (telescope) : ウィキペディア英語版
VISTA (telescope)

The VISTA (Visible and Infrared Survey Telescope for Astronomy) is a wide-field reflecting telescope with a 4.1 metre mirror, located at the Paranal Observatory in Chile. It is operated by the European Southern Observatory and started science operations in December 2009. VISTA is a survey telescope working at infrared wavelengths, and is by far the largest telescope in the world dedicated to surveying the sky at near-infrared wavelengths.〔(【引用サイトリンク】title=The ESO Survey Telescopes )〕 The telescope has only one instrument: VIRCAM, the Vista InfraRed CAMera. This is a 3-tonne camera containing 16 special detectors sensitive to infrared light, with a combined total of 67 million pixels.
A second-generation instrument (4MOST, a 2400-object fibre-fed multi-object spectrograph) is under development for installation around 2020.
Observing at wavelengths longer than those visible to the human eye allows VISTA to study objects that may be almost impossible to see in visible light because they are cool, obscured by dust clouds or because their light has been stretched towards redder wavelengths by the expansion of space during the light’s long journey from the early Universe.〔
VISTA was conceived and developed by a consortium of universities in the United Kingdom led by Queen Mary, University of London and became an in-kind contribution to ESO as part of the UK's accession agreement, with the subscription paid by the UK Science and Technology Facilities Council (STFC).〔
== The project ==

VISTA is carrying out surveys of the southern sky at near infrared wavelengths. Such surveys should both return direct scientific results and help select objects for further studies with larger telescopes. There are two related projects: the Wide Field Camera (WFCAM) on the United Kingdom Infrared Telescope in Hawaii carries out infrared surveys of the northern sky, and the VLT Survey Telescope in Chile carries out surveys of the southern sky in visible light.

The project was initiated in 1999 by the VISTA Consortium〔The VISTA consortium consists of Queen Mary, University of London as consortium leader, Queen's University Belfast, University of Birmingham, University of Cambridge, Cardiff University, University of Central Lancashire, Durham University, University of Edinburgh, University of Hertfordshire, Keele University, University of Leicester, Liverpool John Moores University, University of Nottingham, University of Oxford, University of St Andrews, University of Southampton, University of Sussex, and University College London.〕 of 18 universities in the United Kingdom (UK), which obtained funding from a joint infrastructure fund of the UK government and further funding from the Particle Physics and Astronomy Research Council. The project is valued at €46M (£36M).
After considering several sites in Chile, the consortium chose the Paranal Observatory of the European Southern Observatory (ESO), namely a secondary peak 1,500 m from the Very Large Telescope (VLT). The consortium selected the UK Astronomy Technology Centre to take technical responsibility for design and construction of the telescope. Two years later – in 2002 – the UK joined ESO, and VISTA became an in-kind component of the joining fee. The consortium then completed the construction and commissioning of the telescope, and the Science and Technology Facilities Council – on behalf of the UK – handed over the telescope to ESO, for the benefit of astronomers in all its member countries.〔

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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