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1 2004/12/25 HOP JTPF JASMINE ILOM JAXA) SPICA JELT Yerkes 1m (1897) Palomar 5m (1948) Subaru 8m (1999)
2 6.5m Large Binocular Telescope(LBT) 8.4m Mt.Graham 18 3m-6m 6.5m 3m
3 Hubble Space Telescope 2.4m (0.115 ) 2.5 Spitzer Space Telescope 85cm 3.6~160 m GALEX 50cm m Astro-F soon 67cm m
4 Frontier z~6.6 Kodaira et al Subaru Suprime-Cam( FOCAS( z~7 ( ) Egami et al nm 935nm HST/NICMOS( SpitzerST
5 Frontier M31 HR From HST press release ( )
6 Frontier VLTI/MIDI 8.2m 103m 20mas proto-planetary disk from van Boekel et al cf. Okamoto et al. 2004
7 TMT CELT,GSMT ?? Giant Magellan 8.4m 7( ~21m) OWL 100m JWST 6.5m 2011?? JELT 30m SPICA 3m JWST
8 30m Ground-Based Telescopes: TMT HST TMT (Figures by Richard Ellis)
9 30m =1.5 H Hα in typical spiral galaxy: 10 5 sec exposure z=0 z=1.5 8m z=1.5 20m z=1.5 30m
10 Giant Magellan Telescope 8.4m 7( ~21m) LBT 8.4m
11 THE OWL 100-M TELESCOPE
12 James Webb Space Telescope 6.5m m ~0.1arcsec 2011 Near Infrared Camera (NIRCam) , m 2 5 Near Infrared Spectrograph (NIRSpec) m 3.4 R~100grism, R~1000 MOS, R~3000 IFU Mid Infrared Instrument (MIRI) 5-27 m 1.5
13 30m TMT vs 6.5m JWST Adaptive Optics R=10,000 R= 1000 R=5 TMT S/N 30m wins JWST wins t=4 1000s, S/N=10, no AO! By Richard Ellis CELT: adapted from Gillett & Mountain (1998)
14 JELT ( ) SPICA HOP JTPF astrometry JASMINE (with ILOM
15 Adaptive Optics SNAP (Supernova Acceleration Probe) 2m 2014 HOP VWFI
16 SNAP Supernova Acceleration Probe 2.0m m, 0.34 L Ia 2014?
17 Hubble Origins Probe Very Wide Field Imager HOP VWFI
18 Hubble Origins Probe deorbit = Hubble Origins Probe HOP Wide Field Camera 3 IR: nm UVIS: nm 3grisms, 100 filters IR: 2. 1 x 2. 3 (0.13 / pix) UVIS: 2. 7 x 2. 7 (0.04 / pix) IR: H=26 UVIS: 29.1 (10h, S/N=5, point source) Cosmic Origins Spectrograph NUV FUV FUV: nm NUV: nm F(130nm)=10-14 erg/s/cm 2 / S/N=30, 9200sec, R=
19 Very Wide Field Imager HOP VWFI Key Science nm ( 0.05 pix (PSF ~0.1 80%EE) ~150 HST ACS ALMA m~29 (20h SN=5) z=6-9 VWFI m (=1000 nm) VWFI orbits ( Obts. ~29 HUDF 50 4 ~28 HDF-N 7 4 ~27 COSMO S 1 1
20 Goals of VWFI Surveys (I) Cosmology DEEP SURVEY Ia 0.5 < z < 2 Ia m lim ~26-27 VWFI + WFC3 + AO
21 Goals of VWFI Surveys (II) Galaxy Formation z =6-9 DEEP SURVEY z= deg 2 - i-drop (z~6) ~ z-drop (z~7) > limited coverage bywfc3 -z R -drop (z~8-9) WFC3 ALMA / JWST
22 Goals of VWFI Surveys (III) Galaxy Evolution z~1.5 DEEP SURVEY HUDF (z~26 GOODS 5 orbits HUDF 144 orbits z AB =26.3 z phot =1.52 No evolution M*+1 z AB =25.7 z phot =1.45 z AB =26.1 z phot =1.60 Photo-z is possible with ground-base UBVRI (m < 27-29) + JHK (m < 25)
23 Goals of VWFI Surveys (IV) Weak Lensing Mass Mapping WIDE SURVEY - m~27 weal lensing - -A few x M sun => Hamana et al. 2003
24 2004 NASA Origins: Future Mission Concept Study ~ HOP WG HOP HOP (STScI, JHU) NASA roadmap HOP
25 JTPF
26 ftp://optik3.mtk.nao.ac.jp/pub/hide/jtpf/
27 5000Å 9000Å
28 9
29 JASMINE( ) JASMINE JASMINE JASMINE Galactic Structure Surveyor Japan Astrometry Satellite Mission for INfrared Exploration
30 z-band:0.9 m ) (z<14mag)
31 1 (1mas) [ ] 10 (10 mas)
32 Hipparcos ESA SIM NASA as@ V=20 GAIA ESA as@ V=15 OBSS USNO as@ V=14 JASMINE z=17 10 as@ z=14 cf. VERA as Remark:
33 VERA * * 1
34 1.5m 0.24
35 H-IIA (dual launch) L2
36 JASMINE :,
37 20cm ILOM In situ Lunar Orientation Measurements) ILOM
38 ILOM
39
40
41
42
43 )
44
45 ILOM NICT ILOM IAU Hilton 1980
46 JELT ( ) SPICA HOP JTPF astrometry JASMINE (with ILOM
47
48 JASMINE: stars of the bulge in the survey area (with / <0.1) GAIA: 400 stars in the same area as that in JASMINE (with / <0.1) (excluding Baade s window)
49
50 Resolving the stars in Virgo (60 million light years away) HST OWL AAT 3.9-m Hi precision HRD down to 1 M
51
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Microsoft PowerPoint - subaru_um.pptx
WFIRST and Subaru in Middle 2020 s Euclid 0.4 1.8μm WISH 1 5μm Wide field Space Missions in 2020 s WFIRST 0.6 2μm (option 2.4μm) Wide-field Imaging Surveyor for High-redshift 超広視野初期宇宙探査衛星計画 ISAS Call for
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THE STAR FORMATION NEWSLETTER No.291-14 March 2017 2017/04/28 16-20 16. X-Shooter spectroscopy of young stellar objects in Lupus. Atmospheric parameters, membership and activity diagnostics 17. The evolution
Contents 1. Ia cosmology 2. Ia / rate 3.
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Independent discoveries of a tidally disrupting dwarf galaxy around NGC 253! A Tidally Disrupting Dwarf Galaxy in the Halo of NGC 253 Toloba, E. et al. 2016, ApJL, 816, L5 (hereafter T16, accepted 2015.12.07)
太陽系外惑星探査
http://hubblesite.org/newscenter/archive/2001/38/ Terra MODIS http://modarch.gsfc.nasa.gov/ http://www.nasa.gov/home/index.html / 2 Are we alone? Origins Where are they? (Fermi 1950) 3 4 0.5 arcsec 10pc
Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5.
Type Ia Supernova Survey w/ WISH Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5. Contents 1. Ia? 2. Ia 3. WISH Ia cosmology 4. WISH Ia + rate 5. Type Ia Supernova + +?? (single degenerate)?
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SuMIRe/PFS 村山斉 (IPMU & Berkeley) Subaru Users Meeting @ 国立天文台 2011.1.19 PFS HSC 5 PFS (FIRST) HSC PFS weak lensing BAO dark energy PFS cf. white paper UM UM PFS exciting SAC HSC UM Eric Prieto (Marseille)
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次世代赤外線天文衛星 SPICA の概要 2011 年 1 月 6 日中川貴雄 (JAXA) SPICA team 企画セッション :SPICA の挑戦 概要 次世代赤外線天文衛星 SPICA の概要 ( 中川 JAXA ) SPICA 観測装置 ( 片坐 JAXA ) 科学目的 SPICA の目指すもの ( 松原 JAXA ) SPICA で探る太陽系科学 ( 渡部 天文台 ) SPICA による系外惑星研究
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, (NAOJ) (Kyoto U.) Telescope aperture 1.5mφ Telescope length Fit within the H-IIA nose fairing Spatial resolution 0.1" in UV 0.16" in Vis/NIR (Diffraction limit of 1.5mφ at 1µm ) FOV ~200" x 200" to cover
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Summary of WISH Filter Set and Sensitivity: Filters suitable for various scientific case Filters cover wavelength range of 1-5µm without any gaps Narr
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