LiteBIRD: Mission Overview and Focal Plane Layout

T. Matsumura; Y. Akiba; K. Arnold; J. Borrill; R. Chendra; Y. Chinone; A. Cukierman; T. de Haan; M. Dobbs; A. Dominjon; T. Elleflot; J. Errard; T. Fujino; H. Fuke; N. Goeckner-wald; N. Halverson; P. Harvey; M. Hasegawa; K. Hattori; M. Hattori; M. Hazumi; C. Hill; G. Hilton; W. Holzapfel; Y. Hori; J. Hubmayr; K. Ichiki; J. Inatani; M. Inoue; Y. Inoue; F. Irie; K. Irwin; H. Ishino; H. Ishitsuka; O. Jeong; K. Karatsu; S. Kashima; N. Katayama; I. Kawano; B. Keating; A. Kibayashi; Y. Kibe; Y. Kida; K. Kimura; N. Kimura; K. Kohri; E. Komatsu; C. L. Kuo; S. Kuromiya; A. Kusaka; A. Lee; E. Linder; H. Matsuhara; S. Matsuoka; S. Matsuura; S. Mima; K. Mitsuda; K. Mizukami; H. Morii; T. Morishima; M. Nagai; T. Nagasaki; R. Nagata; M. Nakajima; S. Nakamura; T. Namikawa; M. Naruse; K. Natsume; T. Nishibori; K. Nishijo; H. Nishino; T. Nitta; A. Noda; T. Noguchi; H. Ogawa; S. Oguri; I. S. Ohta; C. Otani; N. Okada; A. Okamoto; A. Okamoto; T. Okamura; G. Rebeiz; P. Richards; S. Sakai; N. Sato; Y. Sato; Y. Segawa; S. Sekiguchi; Y. Sekimoto; M. Sekine; U. Seljak; B. Sherwin; K. Shinozaki; S. Shu; R. Stompor; H. Sugai; H. Sugita; T. Suzuki; A. Suzuki; O. Tajima; S. Takada; S. Takakura; K. Takano; Y. Takei; T. Tomaru; N. Tomita; P. Turin; S. Utsunomiya; Y. Uzawa; T. Wada; H. Watanabe; B. Westbrook; N. Whitehorn; Y. Yamada; N. Yamasaki; T. Yamashita; M. Yoshida; T. Yoshida; Y. Yotsumoto

doi:10.1007/s10909-016-1542-8

LiteBIRD: Mission Overview and Focal Plane Layout

T. Matsumura, Y. Akiba, K. Arnold, J. Borrill, R. Chendra, Y. Chinone, A. Cukierman, T. de Haan, M. Dobbs, A. Dominjon, T. Elleflot, J. Errard, T. Fujino, H. Fuke, N. Goeckner-wald, N. Halverson, P. Harvey, M. Hasegawa, K. Hattori, M. HattoriM. Hazumi, C. Hill, G. Hilton, W. Holzapfel, Y. Hori, J. Hubmayr, K. Ichiki, J. Inatani, M. Inoue, Y. Inoue, F. Irie, K. Irwin, H. Ishino, H. Ishitsuka, O. Jeong, K. Karatsu, S. Kashima, N. Katayama, I. Kawano, B. Keating, A. Kibayashi, Y. Kibe, Y. Kida, K. Kimura, N. Kimura, K. Kohri, E. Komatsu, C. L. Kuo, S. Kuromiya, A. Kusaka, A. Lee, E. Linder, H. Matsuhara, S. Matsuoka, S. Matsuura, S. Mima, K. Mitsuda, K. Mizukami, H. Morii, T. Morishima, M. Nagai, T. Nagasaki, R. Nagata, M. Nakajima, S. Nakamura, T. Namikawa, M. Naruse, K. Natsume, T. Nishibori, K. Nishijo, H. Nishino, T. Nitta, A. Noda, T. Noguchi, H. Ogawa, S. Oguri, I. S. Ohta, C. Otani, N. Okada, A. Okamoto, A. Okamoto, T. Okamura, G. Rebeiz, P. Richards, S. Sakai, N. Sato, Y. Sato, Y. Segawa, S. Sekiguchi, Y. Sekimoto, M. Sekine, U. Seljak, B. Sherwin, K. Shinozaki, S. Shu, R. Stompor, H. Sugai, H. Sugita, T. Suzuki, A. Suzuki, O. Tajima, S. Takada, S. Takakura, K. Takano, Y. Takei, T. Tomaru, N. Tomita, P. Turin, S. Utsunomiya, Y. Uzawa, T. Wada, H. Watanabe, B. Westbrook, N. Whitehorn, Y. Yamada, N. Yamasaki, T. Yamashita, M. Yoshida, T. Yoshida, Y. Yotsumoto

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

71 引文斯高帕斯（Scopus）

摘要

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 σ_r< 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.

原文	???core.languages.en_GB???
頁（從 - 到）	824-831
頁數	8
期刊	Journal of Low Temperature Physics
卷	184
發行號	3-4
DOIs	https://doi.org/10.1007/s10909-016-1542-8
出版狀態	已出版 - 1 8月 2016

存取文件

10.1007/s10909-016-1542-8

引用此

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., ... Yotsumoto, Y. (2016). LiteBIRD: Mission Overview and Focal Plane Layout. Journal of Low Temperature Physics, 184(3-4), 824-831. https://doi.org/10.1007/s10909-016-1542-8

@article{e9e0bfad14e04ce3bf28990d678ce534,

title = "LiteBIRD: Mission Overview and Focal Plane Layout",

abstract = "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.",

keywords = "CMB, Inflation, MKID, Polarization, Primordial B-mode, Satellite, TES bolometer",

author = "T. Matsumura and Y. Akiba and K. Arnold and J. Borrill and R. Chendra and Y. Chinone and A. Cukierman and {de Haan}, T. and M. Dobbs and A. Dominjon and T. Elleflot and J. Errard and T. Fujino and H. Fuke and N. Goeckner-wald and N. Halverson and P. Harvey and M. Hasegawa and K. Hattori and M. Hattori and M. Hazumi and C. Hill and G. Hilton and W. Holzapfel and Y. Hori and J. Hubmayr and K. Ichiki and J. Inatani and M. Inoue and Y. Inoue and F. Irie and K. Irwin and H. Ishino and H. Ishitsuka and O. Jeong and K. Karatsu and S. Kashima and N. Katayama and I. Kawano and B. Keating and A. Kibayashi and Y. Kibe and Y. Kida and K. Kimura and N. Kimura and K. Kohri and E. Komatsu and Kuo, {C. L.} and S. Kuromiya and A. Kusaka and A. Lee and E. Linder and H. Matsuhara and S. Matsuoka and S. Matsuura and S. Mima and K. Mitsuda and K. Mizukami and H. Morii and T. Morishima and M. Nagai and T. Nagasaki and R. Nagata and M. Nakajima and S. Nakamura and T. Namikawa and M. Naruse and K. Natsume and T. Nishibori and K. Nishijo and H. Nishino and T. Nitta and A. Noda and T. Noguchi and H. Ogawa and S. Oguri and Ohta, {I. S.} and C. Otani and N. Okada and A. Okamoto and A. Okamoto and T. Okamura and G. Rebeiz and P. Richards and S. Sakai and N. Sato and Y. Sato and Y. Segawa and S. Sekiguchi and Y. Sekimoto and M. Sekine and U. Seljak and B. Sherwin and K. Shinozaki and S. Shu and R. Stompor and H. Sugai and H. Sugita and T. Suzuki and A. Suzuki and O. Tajima and S. Takada and S. Takakura and K. Takano and Y. Takei and T. Tomaru and N. Tomita and P. Turin and S. Utsunomiya and Y. Uzawa and T. Wada and H. Watanabe and B. Westbrook and N. Whitehorn and Y. Yamada and N. Yamasaki and T. Yamashita and M. Yoshida and T. Yoshida and Y. Yotsumoto",

note = "Publisher Copyright: {\textcopyright} 2016, Springer Science+Business Media New York.",

year = "2016",

month = aug,

day = "1",

doi = "10.1007/s10909-016-1542-8",

language = "???core.languages.en_GB???",

volume = "184",

pages = "824--831",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

number = "3-4",

}

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 2016, 'LiteBIRD: Mission Overview and Focal Plane Layout', Journal of Low Temperature Physics, 卷 184, 編號 3-4, 頁 824-831. https://doi.org/10.1007/s10909-016-1542-8

TY - JOUR

T1 - LiteBIRD

T2 - Mission Overview and Focal Plane Layout

AU - Matsumura, T.

AU - Akiba, Y.

AU - Arnold, K.

AU - Borrill, J.

AU - Chendra, R.

AU - Chinone, Y.

AU - Cukierman, A.

AU - de Haan, T.

AU - Dobbs, M.

AU - Dominjon, A.

AU - Elleflot, T.

AU - Errard, J.

AU - Fujino, T.

AU - Fuke, H.

AU - Goeckner-wald, N.

AU - Halverson, N.

AU - Harvey, P.

AU - Hasegawa, M.

AU - Hattori, K.

AU - Hattori, M.

AU - Hazumi, M.

AU - Hill, C.

AU - Hilton, G.

AU - Holzapfel, W.

AU - Hori, Y.

AU - Hubmayr, J.

AU - Ichiki, K.

AU - Inatani, J.

AU - Inoue, M.

AU - Inoue, Y.

AU - Irie, F.

AU - Irwin, K.

AU - Ishino, H.

AU - Ishitsuka, H.

AU - Jeong, O.

AU - Karatsu, K.

AU - Kashima, S.

AU - Katayama, N.

AU - Kawano, I.

AU - Keating, B.

AU - Kibayashi, A.

AU - Kibe, Y.

AU - Kida, Y.

AU - Kimura, K.

AU - Kimura, N.

AU - Kohri, K.

AU - Komatsu, E.

AU - Kuo, C. L.

AU - Kuromiya, S.

AU - Kusaka, A.

AU - Lee, A.

AU - Linder, E.

AU - Matsuhara, H.

AU - Matsuoka, S.

AU - Matsuura, S.

AU - Mima, S.

AU - Mitsuda, K.

AU - Mizukami, K.

AU - Morii, H.

AU - Morishima, T.

AU - Nagai, M.

AU - Nagasaki, T.

AU - Nagata, R.

AU - Nakajima, M.

AU - Nakamura, S.

AU - Namikawa, T.

AU - Naruse, M.

AU - Natsume, K.

AU - Nishibori, T.

AU - Nishijo, K.

AU - Nishino, H.

AU - Nitta, T.

AU - Noda, A.

AU - Noguchi, T.

AU - Ogawa, H.

AU - Oguri, S.

AU - Ohta, I. S.

AU - Otani, C.

AU - Okada, N.

AU - Okamoto, A.

AU - Okamura, T.

AU - Rebeiz, G.

AU - Richards, P.

AU - Sakai, S.

AU - Sato, N.

AU - Sato, Y.

AU - Segawa, Y.

AU - Sekiguchi, S.

AU - Sekimoto, Y.

AU - Sekine, M.

AU - Seljak, U.

AU - Sherwin, B.

AU - Shinozaki, K.

AU - Shu, S.

AU - Stompor, R.

AU - Sugai, H.

AU - Sugita, H.

AU - Suzuki, T.

AU - Suzuki, A.

AU - Tajima, O.

AU - Takada, S.

AU - Takakura, S.

AU - Takano, K.

AU - Takei, Y.

AU - Tomaru, T.

AU - Tomita, N.

AU - Turin, P.

AU - Utsunomiya, S.

AU - Uzawa, Y.

AU - Wada, T.

AU - Watanabe, H.

AU - Westbrook, B.

AU - Whitehorn, N.

AU - Yamada, Y.

AU - Yamasaki, N.

AU - Yamashita, T.

AU - Yoshida, M.

AU - Yoshida, T.

AU - Yotsumoto, Y.

PY - 2016/8/1

Y1 - 2016/8/1

N2 - 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.

AB - 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.

KW - CMB

KW - Inflation

KW - MKID

KW - Polarization

KW - Primordial B-mode

KW - Satellite

KW - TES bolometer

UR - http://www.scopus.com/inward/record.url?scp=84962712089&partnerID=8YFLogxK

U2 - 10.1007/s10909-016-1542-8

DO - 10.1007/s10909-016-1542-8

M3 - 期刊論文

AN - SCOPUS:84962712089

SN - 0022-2291

VL - 184

SP - 824

EP - 831

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 3-4

ER -

LiteBIRD: Mission Overview and Focal Plane Layout

摘要

存取文件

指紋

引用此