Prime Focus Spectrograph (PFS) for the Subaru Telescope: Overview, recent progress, and future perspectives

preprint2016arXivOpen access
Naoyuki TamuraNaruhisa TakatoAtsushi ShimonoYuki MoritaniKiyoto YabeYuki IshizukaAkitoshi UedaYukiko KamataHrand AghazarianStephane ArnoutsGabriel BarbanRobert H. BarkhouserRenato C. BorgesDavid F. BraunMichael A. CarrPierre-Yves ChabaudYin-Chang ChangHsin-Yo ChenMasashi ChibaRichard C. Y. ChouYou-Hua ChuJudith G. CohenRodrigo P. de AlmeidaAntonio C. de OliveiraLigia S. de OliveiraRichard G. DekanyKjetil DohlenJesulino B. dos SantosLeandro H. dos SantosRichard S. EllisMaximilian FabriciusDidier FerrandDecio FerreiraMirek GolebiowskiJenny E. GreeneJohannes GrossJames E. GunnRandolph HammondAlbert HardingMurdock HartTimothy M. HeckmanChristopher M. HirataPaul HoStephen C. HopeLarry HovlandShu-Fu HsuYen-Shan HuPing-Jie HuangMarc JaquetYipeng JingJennifer KarrMasahiko KimuraMatthew E. KingEiichiro KomatsuVincent Le BrunOlivier Le FevreArnaud Le FurDavid Le MignantHung-Hsu LingCraig P. LoomisRobert H. LuptonFabrice MadecPeter MaoLucas S. MarraraClaudia Mendes de OliveiraYosuke MinowaChaz N. MorantzHitoshi MurayamaGraham J. MurrayYouichi OhyamaJoseph OrndorffSandrine PascalJefferson M. PereiraDaniel J. ReileyMartin ReineckeAndreas RitterMitsuko RobertsMark A. SchwochertMichael D. SeiffertStephen A. SmeeLaerte Sodre Jr.David N. SpergelAaron J. SteinkrausMichael A. StraussChristian SuraceYasushi SutoNao SuzukiJohn SwinbankPhilip J. TaitMasahiro TakadaTomonori TamuraYoko TanakaLaurence TresseOrlando Verducci Jr.Didier VibertClement VidalShiang-Yu WangChih-Yi WenChi-Hung YanNaoki Yasuda

Abstract

PFS (Prime Focus Spectrograph), a next generation facility instrument on the 8.2-meter Subaru Telescope, is a very wide-field, massively multiplexed, optical and near-infrared spectrograph. Exploiting the Subaru prime focus, 2394 reconfigurable fibers will be distributed over the 1.3 deg field of view. The spectrograph has been designed with 3 arms of blue, red, and near-infrared cameras to simultaneously observe spectra from 380nm to 1260nm in one exposure at a resolution of ~1.6-2.7A. An international collaboration is developing this instrument under the initiative of Kavli IPMU. The project is now going into the construction phase aiming at undertaking system integration in 2017-2018 and subsequently carrying out engineering operations in 2018-2019. This article gives an overview of the instrument, current project status and future paths forward.

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