Ho-Il KIM 2011.11. 08.. Contents K-GMT Project GMT : Off-Axis Primary #1 GMT1 Surface Maps Primary Mirror Covers 1 st Generation Instruments Instrument.

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Presentation transcript:

Ho-Il KIM

Contents K-GMT Project GMT : Off-Axis Primary #1 GMT1 Surface Maps Primary Mirror Covers 1 st Generation Instruments Instrument Mounting GMT : Preparation to PDR Community-wide Science Promotion Preparation for GMT era in KASI K-GMT 2011 : Data Center FSM prototype development GMTNIRS 1. K-GMT in KMTNet in 2011

Development at SOML / Univ. Arizona Fabrication finish in Nov Most pacing item of GMT development GMT PM#2 casting : Jan GMT PM#3 casting : Feb. 2013

JuneAugust 71 nm 38 nm September

Mirror covers clear the beam – even for the center segment! The only ELT having mirror covers Mirror covers clear the beam – even for the center segment! The only ELT having mirror covers

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9 NameFunctionRemark GMACSWide field multi-object optical spectrographNon AO NIRMOSNIR multi-object spectrographNon AO GMTIFSIntegral-Field spectrographNon AO GMTNIRSHigh-Resolution NIR/MIR spectrographAO GCLEFHigh dispersion, high stability optical spectrographAO TIGERMIR Infrared imagerAO

NIRMOS GMACS GMTIFS GMTNIRS TIGER G-CLEF

PDR plan : the end of 2012 Science case update will be completed soon or later 1 st gen. instruments will be selected in this year Conceptual design contract for major parts Enclosure / facilities Site preparation Bearings / linear drives Data Archives and data center

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13 KASI endeavors to hire more and more young researchers

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18 M-band spectrograph shield L-band spectrograph shield JHK-band spectrograph Modules Slit/OIWFS housing LGS pickoff mirror

Detection of micro-Gravitational Lensing events Monitoring the Galactic Bulge Discovery of extra-solar planets

TelescopeCameraFOVSiteTarget PanSTARRS 4x1.8m1400M pixel CCD7.0 deg 2 Haleakala, USAAll sky survey MOA 1.8m80M pixel CCD2.4 deg 2 Mt. John, New ZealandGalactic Bulge KMTNet 3x1.6m340M pixel CCD4.0 deg 2 CTIO – SAAO – SSOGalactic Bulge SkyMapper 1.35m268M pixel CCD5.7 deg 2 SSO, AustraliaAll sky survey OGLE-IV 1.3m268M pixel CCD1.4 deg 2 LCO, ChileGalactic Bulge LCOGT 2x2.0m, 10x1.0m, 14x0.6m 16M pixel CCD 0.03 deg deg 2 Haleakala–Canary–CTIO– SAAO–SSO Follow-Up Obs. Exoplanet, GRB

SAAO SSO CTIO KASI

CTIO

SSO

SAAO

Development of the System 2009Concept Design of the Wide-Field Telescope and Mosaic Camera Jul.2010Contract of the KMTNet Telescope Mar.2011Final Design Completion of the Telescope Jun.2011Contract of the KMTNet Camera & Telescope Manufacturing Start Aug.2011Finish Polishing the First Primary Mirror Dec.2011Final Design Completion of the Camera Mid-2013First Light of the First System at CTIO in Chile By Mid-2014First Light of the Second and Third Systems

5 th EACOA