LiteBIRD: Mission Overview and Focal Plane Layout
- Matsumura, T;
- Akiba, Y;
- Arnold, K;
- Borrill, J;
- Chendra, R;
- Chinone, Y;
- Cukierman, A;
- de Haan, T;
- Dobbs, M;
- Dominjon, A;
- Elleflot, T;
- Errard, J;
- Fujino, T;
- Fuke, H;
- Goeckner-wald, N;
- Halverson, N;
- Harvey, P;
- Hasegawa, M;
- Hattori, K;
- Hattori, M;
- Hazumi, M;
- Hill, C;
- Hilton, G;
- Holzapfel, W;
- Hori, Y;
- Hubmayr, J;
- Ichiki, K;
- Inatani, J;
- Inoue, M;
- Inoue, Y;
- Irie, F;
- Irwin, K;
- Ishino, H;
- Ishitsuka, H;
- Jeong, O;
- Karatsu, K;
- Kashima, S;
- Katayama, N;
- Kawano, I;
- Keating, B;
- Kibayashi, A;
- Kibe, Y;
- Kida, Y;
- Kimura, K;
- Kimura, N;
- Kohri, K;
- Komatsu, E;
- Kuo, CL;
- Kuromiya, S;
- Kusaka, A;
- Lee, A;
- Linder, E;
- Matsuhara, H;
- Matsuoka, S;
- Matsuura, S;
- Mima, S;
- Mitsuda, K;
- Mizukami, K;
- Morii, H;
- Morishima, T;
- Nagai, M;
- Nagasaki, T;
- Nagata, R;
- Nakajima, M;
- Nakamura, S;
- Namikawa, T;
- Naruse, M;
- Natsume, K;
- Nishibori, T;
- Nishijo, K;
- Nishino, H;
- Nitta, T;
- Noda, A;
- Noguchi, T;
- Ogawa, H;
- Oguri, S;
- Ohta, IS;
- Otani, C;
- Okada, N;
- Okamoto, A;
- Okamoto, A;
- Okamura, T;
- Rebeiz, G;
- Richards, P;
- Sakai, S;
- Sato, N;
- Sato, Y;
- Segawa, Y;
- Sekiguchi, S;
- Sekimoto, Y;
- Sekine, M;
- Seljak, U;
- Sherwin, B;
- Shinozaki, K;
- Shu, S;
- Stompor, R;
- Sugai, H;
- Sugita, H;
- Suzuki, T;
- Suzuki, A;
- Tajima, O;
- Takada, S;
- Takakura, S;
- Takano, K;
- Takei, Y;
- Tomaru, T;
- Tomita, N;
- Turin, P;
- Utsunomiya, S;
- Uzawa, Y;
- Wada, T;
- Watanabe, H;
- Westbrook, B;
- Whitehorn, N;
- Yamada, Y;
- Yamasaki, N;
- Yamashita, T;
- Yoshida, M;
- Yoshida, T;
- Yotsumoto, Y
- et al.
Published Web Location
https://link.springer.com/article/10.1007/s10909-016-1542-8Abstract
LiteBIRD is a proposed CMB polarization satellite project to probe the inflationary B-mode signal. The satellite is designed to measure the tensor-to-scalar ratio with a 68 % confidence level uncertainty of σr< 10 - 3, including statistical, instrumental systematic, and foreground uncertainties. LiteBIRD will observe the full sky from the second Lagrange point for 3 years. We have a focal plane layout for observing frequency coverage that spans 40–402 GHz to characterize the galactic foregrounds. We have two detector candidates, transition-edge sensor bolometers and microwave kinetic inductance detectors. In both cases, a telecentric focal plane consists of approximately 2 × 10 3 superconducting detectors. We will present the mission overview of LiteBIRD, the project status, and the TES focal plane layout.
Many UC-authored scholarly publications are freely available on this site because of the UC's open access policies. Let us know how this access is important for you.