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ESO 3.6 m Telescope
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== Instruments == Since 22, the ESO 3.6 m telescope has hosted HARPS, the [[High Accuracy Radial Velocity Planet Searcher]] and NIRPS, the Near Infra Red Planet Searcher. HARPS is a fibre-fed high resolution [[Echelle grating|echelle spectrograph]] dedicated to the discovery of extrasolar planets. Other instruments on the telescope, now decommissioned, include:<ref>{{cite web|url=http://www.eso.org/sci/facilities/lasilla/telescopes/3p6/index.html | title = The ESO 3.6m Telescope | access-date = 2011-05-26}}</ref> * '''CES''': is a spectrograph that provides a resolving power of up to 235,000 in the 346β1028 nm region. * '''EFOSC2''': the ''ESO Faint Object Spectrograph and Camera (v.2)'', is a very versatile instrument for low resolution spectroscopy and imaging. * '''TIMMI-2''': the ''Thermal Infrared MultiMode Instrument'' dedicated to the 3β25 [[ΞΌm]] spectrum. * '''ADONIS''': is the acronym for ''Adaptive Optics Near Infrared System'', and was a second-generation [[adaptive optics]] system for the astronomical community.<ref name=Zirker2005/> More than 40 peer-reviewed scientific articles were published based on this instrument data.<ref name=SIMBAD_ADONIS/> ADONIS is the final version of diverse Adaptive Optics (AO) prototypes named Come-on and Come-on +. It was offered in its final version in October 1996 as an official [[ESO]] instrument,<ref name=RoussetBeuzit1999/> then decommissioned in 2001. ADONIS was the first AO system offered to a large community of astronomers.
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