野辺山の将来- 新望遠鏡-rk.pptx
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1 10 NRO/NAOJ Jul. 28, 2011
2 30? 45m, NMA - ASTE - VLBI VSOP- I (VERA) (VSOP- II Impact ) VLBI NMA LMA/LMSA ALMA
3 30? ALMA - /NAOJ - - (SMA, IRAM, CARMA, ATCA ) - - -
4 NRO 10 1/ ( ; ) - NRO ( 45m - ALMA ( RK m - NRO 45m ( ) - ;BEARS 35 - ALMA (2SB RX/ ) ( ; RK) WG(45m ; ) m - 4, => ISAS/JAXA
5 NRO 10 2/ RK ALMA NRO WG 45m Legacy (+ ASTE Key Science) - AzTEC ASTE (UMASS/INAOE ); => (S) (Chair; Ron Ekers) m ( ) - ( ) ; 45m z- machine & ASTE TES - / 2009 ~ 3 (2 ) - 45m - ASTE
6 ( ) 45m Legacy AzTEC/ASTE NMA 45m ASTE NMA/ Rainbow SMA
7 NRO 10 ( ) step-by-step transi'on - - Legacy/Key Science - 45m ALMA -? - RK will disappear? ALMA - EA - ( )
8 NRO Master Plan ( ) Feedback to ALMA 45m 45m Ant. 45m Remote 2010~ ALMA/NRO 2013~ ALMA/NRO 2017?~ ALMA/ 45m Z- Machine ASTE S 45m 70GHz ASTE THz ASTE THz THz??
9 NRO/NAOJ Jul. 28, 2011
10 Roles of NRO in ALMA Era Enhancing Science with 45m/ASTE toward ALMA Era New Developments to create new seeds for the future Planning a Large mm/sub- mm Single dish for opening new discovery space in ALMA/SKA- era NRO 45m Telescope D ~ m Freq. = 70 GHz 1 THz? Completion ~ 2018?? Natural Transiion ASTE 10 m In Chie Wide Field Imaging Serendipity Census in the Universe Incubate Original Ideas
11 ALMA/SPICA Synergy TElescope (AS1-3TE) (仮称) A New Large mm/sub- mm Single dish Telescope - complementary to ALMA, SPICA, SKA,.. - opening new discovery space in ALMA/SPICA/SKA- era Wide Field Imaging & Ulimate wide- band Spectroscopy NRO 45m Tel Natural Evoluion ASTE 10 m Telescope In Chie D ~ 30 m or 50 m? Freq. = 70 GHz 1 THz (or 400 GHz??) Completion ~ ?? Wide Field CO Tomography Serendipity Census in the Universe Incubate Original Ideas
12 New mm/sub- mm Telescope Natural transiion from 45m/ASTE 45m - limitaion of observing wavelength: 3mm(or 2mm) due to atmosphere/antenna performance years old; need mm/sub- mm new telescopes! ASTE - Limitaion of FOV (7.5 arcmin.); future 10 k- pix camera unavailable, & need larger FOV - Confusion Limited SMG survey; need smaller beam - Small RX Cabin; can accommodate only one RX need bigger cabin
13 AzTEC/ASTE Deep Wide- field SMG Surveys AKARI Deep Field South (ADF-S) Subaru/XMM- Newton Deep Field (SXDF) SSA22 Coverage (arcmin 2 ) Depth (1σ, mjy) No sources (>3.5σ) reference Hatsukade+10 MNRAS in press Ikarashi+10 arxiv i Tamura+ 09, 10 Nature, 459, 61 ApJ, in press ADF-S SXDF SSA 22
14 New mm/sub- mm Telescope New Discovery Space complement to ALMA - Break through in depth & area coverage + ASTE SMG sample fainter SMGs 1 deg 2 survey deg 2 survey Muli- Colors Spectroscopic Imaging - Break through in spectroscopy 45m: 2 GHz x 16sets 1~ 10 THz coverage 4 beam SIS array HEMT array +?
15 Survey sensiivity; SD vs ALMA (12m x50) Assuming same observing ime & area (SD equipped with camera Our Target (Tentative) easte with k-pix Camera SD; 5 times deeper SD; 2 times deeper AzTEC/ASTE Same depth for SD & ALMA Deeper Confusion Noise
16 Key Science (1/2) Galaxy Formaion and Cosmology - SZ cosmology 3mm (min. confusion) mapping of low- mass (3e14 M sun ) cluster at z=1 with beam < 20 arcsec (to resolve Virial core) Komatsu- san s request - Galaxy Redshis Survey with CO/CII lines BAO for z = 0 to 3 or 4 (CO), z > 4 (CII) Large- scale structure formaion internal kinemaics of clusters - Deep mm/sub- mm Survey with very low confus. IR background, faint end of number count
17 CO Tomography: reaches to z= ~ 7? Tamura 2011
18 Key Science (2/2) Physic and Chemistry of Interstellar Medium - Chemistry from starless cores to planetary disk and atmosphere; two archetypes, WCCC (Warm Carbon Chain Chemistry) and hot- core (Organic Molecules) Chemistry - Large Organic Molecules and Origin of Life Large Molecules and Carbon- chain molecules has rotaional transiions at cm to long sub- mm - Origin of Interstellar Turbulence and IMF - Physics and Chemistry in external galaxies (Mm/sub- mm VLBI?)
19 ALMA/SPICA Synergy TElescope (AS 2 TE) ( ) Two Opions?? - ~50 m telescope up to ~400 GHz (~ THz for good condi.) big advantage at mm/longer sub- mm limited use at 450 um & shorter with under- illuminaion conflicing with LMT(?), but share southern/northern skies - ~30 m telescope covering up to ~THz (5000m site in Chile?) completely conflicing with CCAT (a liule bit) advantageous at mm/longer sub- mm disadvantageous at shorter sub- mm Timeline?? Construcion complete unil ???
20 AS 2 TE ( ) , - ISAS - - NAOJ, NAOJ - NRO/ALMA m/ASTE, ACA ;?
21 SPICA/ISAS/JAXA Synergies Litebird/KEK Inflation to Dark Age Satellite Technology Mm to FIR Camera CMB Secondary ALMA & ASTE-II (JP Univ./NAOJ) Origin of Life Imaging Spectroscopy
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