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dc.contributor.authorKimura, Masahiko
dc.contributor.authorMaihara, Toshinori
dc.contributor.authorIwamuro, Fumihide
dc.contributor.authorAkiyama, Masayuki
dc.contributor.authorTamura, Naoyuki
dc.contributor.authorDalton, Gavin B.
dc.contributor.authorTakato, Naruhisa
dc.contributor.authorTait, Philip
dc.contributor.authorOhta, Kouji
dc.contributor.authorEto, Shigeru
dc.contributor.authorMochida, Daisaku
dc.contributor.authorElms, Brian
dc.contributor.authorKawate, Kaori
dc.contributor.authorKurakami, Tomio
dc.contributor.authorMoritani, Yuuki
dc.contributor.authorNoumaru, Junichi
dc.contributor.authorOhshima, Norio
dc.contributor.authorSumiyoshi, Masanao
dc.contributor.authorYabe, Kiyoto
dc.contributor.authorBrzeski, Jurek
dc.contributor.authorFarrell, Tony
dc.contributor.authorFrost, Gabriella
dc.contributor.authorGillingham, Peter R.
dc.contributor.authorHaynes, Roger
dc.contributor.authorMoore, Anna M.
dc.contributor.authorMuller, Rolf
dc.contributor.authorSmedley, Scott
dc.contributor.authorSmith, Greg
dc.contributor.authorBonfield, David G.
dc.contributor.authorBrooks, Charles B.
dc.contributor.authorHolmes, Alan R.
dc.contributor.authorLake, Emma Curtis
dc.contributor.authorLee, Hanshin
dc.contributor.authorLewis, Ian J.
dc.contributor.authorFroud, Tim R.
dc.contributor.authorTosh, Ian A.
dc.contributor.authorWoodhouse, Guy F.
dc.contributor.authorBlackburn, Colin
dc.contributor.authorContent, Robert
dc.contributor.authorDipper, Nigel
dc.contributor.authorMurray, Graham
dc.contributor.authorSharples, Ray
dc.contributor.authorRobertson, David J.
dc.date.accessioned2011-12-14T17:01:07Z
dc.date.available2011-12-14T17:01:07Z
dc.date.issued2010
dc.identifier.citationKimura , M , Maihara , T , Iwamuro , F , Akiyama , M , Tamura , N , Dalton , G B , Takato , N , Tait , P , Ohta , K , Eto , S , Mochida , D , Elms , B , Kawate , K , Kurakami , T , Moritani , Y , Noumaru , J , Ohshima , N , Sumiyoshi , M , Yabe , K , Brzeski , J , Farrell , T , Frost , G , Gillingham , P R , Haynes , R , Moore , A M , Muller , R , Smedley , S , Smith , G , Bonfield , D G , Brooks , C B , Holmes , A R , Lake , E C , Lee , H , Lewis , I J , Froud , T R , Tosh , I A , Woodhouse , G F , Blackburn , C , Content , R , Dipper , N , Murray , G , Sharples , R & Robertson , D J 2010 , ' Fibre Multi-Object Spectrograph (FMOS) for the Subaru Telescope ' , Publications of the Astronomical Society of Japan , vol. 62 , no. 5 , pp. 1135-1147 . < http://pasj.asj.or.jp/#past >
dc.identifier.issn0004-6264
dc.identifier.otherPURE: 496514
dc.identifier.otherPURE UUID: 94c33466-37a7-40d0-9c28-f20740b63a5e
dc.identifier.otherWOS: 000283885700006
dc.identifier.otherScopus: 78149242333
dc.identifier.urihttp://hdl.handle.net/2299/7286
dc.description.abstractFibre Multi-Object Spectrograph (FMOS) is the first near-infrared instrument with a wide field of view capable of acquiring spectra simultaneously from up to 400 objects. It has been developed as a common-use instrument for the F/2 prime-focus of the Subaru Telescope. The field coverage of 30' diameter is achieved using a new 3-element corrector optimized in the near-infrared (0.9-1.8 mu m) wavelength range. Due to limited space at the prime-focus, we have had to develop a novel fibre positioner, called "Echidna", together with two OH-airglow suppressed spectrographs. FMOS consists of three subsystems: the prime focus unit for IR, the fibre positioning system/connector units, and the two spectrographs. After full systems integration, FMOS was installed on the telescope in late 2007. Many aspects of the performance were checked through various test and engineering observations. In this paper, we present the optical and mechanical components of FMOS, and show the results of our on-sky engineering observations to date.en
dc.format.extent13
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of Japan
dc.subjectcosmology: observations
dc.subjectinstrumentation: spectrographs
dc.subjectsurveys
dc.subjecttelescopes: Subaru
dc.subjectOH-AIRGLOW SUPPRESSOR
dc.subjectECHIDNA
dc.subjectPOSITIONER
dc.subjectPROJECT
dc.titleFibre Multi-Object Spectrograph (FMOS) for the Subaru Telescopeen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.identifier.urlhttp://pasj.asj.or.jp/#past
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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