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• (70) • • • • •
Page 1 and 2: UC Berkeley 2010410
Page 3: • ~0.5% • ~0.1-1.5% • 4.5%
Page 6 and 7: IRCS (AO188) Infrared imager and sp
Page 10 and 11: • Ia Ia
Page 12 and 13: Ia • Ia • •
Page 14 and 15: Ia • Ia • • • •
Page 16: E = 1 2 mȧ2 − G Nm a 4π 3 a3 ρ
Page 23 and 24: • (70) •
Page 25: • (70) • • •
Page 29: • (70) • • • • •
Page 32: • • •
Page 35: • • •
Page 38 and 39: • (w
Page 40 and 41: • • “quintessence” • m
Page 42 and 43: Cosmic Coincidence Problem • ρΛ
Page 44: • • • w=-p/ρ=w(a) • D
Page 47 and 48: ds 2 = dt 2 − a(t) 2 dr 2 1 −
Page 49 and 50: 4 • SN (Type-Ia supernovae) • C
Page 51 and 52: Weak Lensing
Page 53 and 54: y (x,y) x r r0 d 1 lens d 2 star
Page 55 and 56: Text
Page 57 and 58: 2000 ~10%
Page 59 and 60: 2000 ~10%
Page 61 and 62: Intrinsic shape of a background gal
Page 63 and 64: cosmic shear • 2lensing power γ(
Page 65 and 66: photometric redshift
Page 67 and 68: BAO
Page 69 and 70: BAO
Page 71 and 72: BAO • (148±3 Mpc) 5
Page 73 and 74: BAO • (148±3 Mpc) • 5
Page 75 and 76: BAO • (148±3 Mpc) • •
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BAO • (148±3 Mpc) • •
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sound horizon http://astro.berkeley
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A. Reid et al. SDSS DR7 Figure 2. A
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• • • • • systematics
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SuMIRe • • 93 • () • 3
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Lens Barrel to complete Feb. 2011.
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HSC ≈300M galaxies
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PFS • 2000−3000 • HSC • f
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• •
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• • • • 8
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• • • • 8 • SuMIRe
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137 100 70 85 3 1.8 COSMOS Surve
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@IPMU 34 22 Big Bang! 60 : 2000
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@IPMU 60 34 22 Big Bang! : 2000
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@IPMU 60 34 22 Big Bang! : 2000
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ACT 2008 2009 2010 @IPMU Δw~10
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ACT 2008 2009 2010 @IPMU Δw~10
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Δw~3% ACT 2008 2009 2010 @IP
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• 30 • 95
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• 30 • 95 •
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• 30 • 95 • • • 27
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• optical frequency combredshift
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