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B mode from Space -- Part 1: The Science goals, status of spaceborne projects, foregrounds (Dec 10 -12), Part 2: Mission design, technologies and challenges for the spaceborne observations (Dec 14 -16) --

10–16 Dec 2015
Asia/Tokyo timezone

Session

Cosmology

10 Dec 2015, 13:00

Presentation materials

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  1. 0. Welcome Hitoshi Murayama (Kavli IPMU)
    Dr Hitoshi Murayama (Kavli IPMU/UCB)
    10/12/2015, 13:00
  2. 1. Why B mode? Eiichiro Komatsu(MPA)
    Dr Eiichiro Komatsu (MPA)
    10/12/2015, 13:05
  3. 2. Why do we need dr < 0.001 (Lyth bounds etc.) Kazunori Kohri (KEK)
    Dr Kazunori Kohri (KEK)
    10/12/2015, 13:35
  4. 25. Lensing B mode at low ell
    Dr Toshiya Namikawa
    10/12/2015, 14:00
  5. 78. The information hidden in the anisotropies of the CMB spectral distortions Khatri TIFR
    Dr Rishi Khatri (TIFR)
    10/12/2015, 14:25
  6. 4. Large scale EE and tau - Jo Dunkley (Oxford)
    Dr Jo Dunkley (Oxford)
    10/12/2015, 15:20
  7. 5. New Physics from an All-Sky Polarization Experiment Cora Dvorkin (Harvard)
    Dr Cora Dvorkin (Harvard)
    10/12/2015, 15:45
  8. 6. Tensor mode bispectrum - Maresuke Shiraishi (Kavli IPMU)
    Dr Maresuke Shiraisi (Kavli IPMU)
    10/12/2015, 16:10
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