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dc.contributor.authorMOONS
dc.contributor.authorRees, P.
dc.contributor.authorEvans, C.
dc.contributor.authorAtkinson, D.
dc.contributor.authorTojeiro, R.
dc.contributor.authorWild, V.
dc.date.accessioned2020-10-12T14:30:02Z
dc.date.available2020-10-12T14:30:02Z
dc.date.issued2020-06-01
dc.identifier270684311
dc.identifier6b7b5375-ce3a-4f6a-88bb-3005e9696cc2
dc.identifier.citationMOONS , Rees , P , Evans , C , Atkinson , D , Tojeiro , R & Wild , V 2020 , ' MOONS : the new Multi-Object Spectrograph for the VLT ' The Messenger , vol. 180 , pp. 10-17 . https://doi.org/10.18727/0722-6691/5195en
dc.identifier.issn0722-6691
dc.identifier.otherBibCode: 2020Msngr.180...10C
dc.identifier.urihttps://hdl.handle.net/10023/20772
dc.description.abstractMOONS is the new Multi-Object Optical and Near-infrared Spectrograph currently under construction for the Very Large Telescope (VLT) at ESO. This remarkable instrument combines, for the first time, the collecting power of an 8-m telescope, 1000 fibres with individual roboticp ositioners, and both low- and high-resolution simultaneous spectral coverage across the 0.64–1.8 μm wavelength range. This facility will provide the astronomical community with a powerful, world-leading instrument able to serve a wide range of Galactic, extragalactic and cosmological studies. Construction is now proceeding full steam ahead and this overview article presents some of the science goals and the technical description of the MOONS instrument. More detailed information on the MOONS surveys is provided in the other dedicated articles in this Messenger issue.
dc.format.extent3086025
dc.language.isoeng
dc.relation.ispartofThe Messengeren
dc.subject3rd-DASen
dc.titleMOONS : the new Multi-Object Spectrograph for the VLTen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.18727/0722-6691/5195
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2020Msngr.180...10Cen


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