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• • redshift • a/a0 = 1/(1+z) • • standard candle: SNe • standard ruler: BAO
ds 2 = dt 2 − a(t) 2 dr 2 1 − kr 2 + r2 d 2 Ω • comoving (proper) distance ds 2 =0−→ d = • luminosity distance • angular diameter distance dr √ 1 − kr 2 = d L = d(1 + z) d A = d/(1 + z) dt a(t) = dz H(z)
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 and 26: • (70) • • •
Page 27 and 28: • (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 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) • •
Page 77 and 78: BAO • (148±3 Mpc) • •
Page 79 and 80: sound horizon http://astro.berkeley
Page 87 and 88: A. Reid et al. SDSS DR7 Figure 2. A
Page 89: • • • • • systematics
Page 92 and 93: SuMIRe • • 93 • () • 3
Page 94 and 95: Lens Barrel to complete Feb. 2011.
Page 96 and 97:
HSC ≈300M galaxies
Page 98:
PFS • 2000−3000 • HSC • f
Page 101 and 102:
• •
Page 103 and 104:
• • • • 8
Page 105 and 106:
• • • • 8 • SuMIRe
Page 107 and 108:
137 100 70 85 3 1.8 COSMOS Surve
Page 109 and 110:
@IPMU 34 22 Big Bang! 60 : 2000
Page 111 and 112:
@IPMU 60 34 22 Big Bang! : 2000
Page 113 and 114:
@IPMU 60 34 22 Big Bang! : 2000
Page 115 and 116:
ACT 2008 2009 2010 @IPMU Δw~10
Page 117 and 118:
ACT 2008 2009 2010 @IPMU Δw~10
Page 119:
Δw~3% ACT 2008 2009 2010 @IP
Page 122 and 123:
• 30 • 95
Page 124 and 125:
• 30 • 95 •
Page 126 and 127:
• 30 • 95 • • • 27
Page 128:
• optical frequency combredshift
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