LiteBIRD: Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection

H. Ishino; Y. Akiba; K. Arnold; D. Barron; J. Borrill; R. Chendra; Y. Chinone; S. Cho; A. Cukierman; T. De Haan; M. Dobbs; A. Dominjon; T. Dotani; T. Elleflot; J. Errard; T. Fujino; H. Fuke; T. Funaki; N. Goeckner-Wald; N. Halverson; P. Harvey; T. Hasebe; M. Hasegawa; K. Hattori; M. Hattori; M. Hazumi; N. Hidehira; C. Hill; G. Hilton; W. Holzapfel; Y. Hori; J. Hubmayr; K. Ichiki; H. Imada; J. Inatani; M. Inoue; Y. Inoue; F. Irie; K. Irwin; H. Ishitsuka; O. Jeong; H. Kanai; K. Karatsu; S. Kashima; N. Katayama; I. Kawano; T. Kawasaki; B. Keating; S. Kernasovskiy; R. Keskitalo; A. Kibayashi; Y. Kida; N. Kimura; K. Kimura; T. Kisner; K. Kohri; E. Komatsu; K. Komatsu; C. L. Kuo; S. Kuromiya; A. Kusaka; A. Lee; D. Li; E. Linder; M. Maki; H. Matsuhara; T. Matsumura; S. Matsuoka; S. Matsuura; S. Mima; Y. Minami; K. Mitsuda; M. Nagai; T. Nagasaki; R. Nagata; M. Nakajima; S. Nakamura; T. Namikawa; M. Naruse; T. Nishibori; K. Nishijo; H. Nishino; A. Noda; T. Noguchi; H. Ogawa; W. Ogburn; S. Oguri; I. Ohta; N. Okada; A. Okamoto; T. Okamura; C. Otani; G. Pisano; G. Rebeiz; P. Richards; S. Sakai; Y. Sakurai; Y. Sato; N. Sato; Y. Segawa; S. Sekiguchi; Y. Sekimoto; M. Sekine; U. Seljak; B. Sherwin; T. Shimizu; K. Shinozaki; S. Shu; R. Stompor; H. Sugai; H. Sugita; J. Suzuki; T. Suzuki; A. Suzuki; O. Tajima; S. Takada; S. Takakura; K. Takano; S. Takatori; Y. Takei; D. Tanabe; T. Tomaru; N. Tomita; P. Turin; S. Uozumi; S. Utsunomiya; Y. Uzawa; T. Wada; H. Watanabe; B. Westbrook; N. Whitehorn; Y. Yamada; R. Yamamoto; N. Yamasaki; T. Yamashita; T. Yoshida; M. Yoshida; K. Yotsumoto

doi:10.1117/12.2231995

LiteBIRD: Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection

H. Ishino, Y. Akiba, K. Arnold, D. Barron, J. Borrill, R. Chendra, Y. Chinone, S. Cho, A. Cukierman, T. De Haan, M. Dobbs, A. Dominjon, T. Dotani, T. Elleflot, J. Errard, T. Fujino, H. Fuke, T. Funaki, N. Goeckner-Wald, N. HalversonP. Harvey, T. Hasebe, M. Hasegawa, K. Hattori, M. Hattori, M. Hazumi, N. Hidehira, C. Hill, G. Hilton, W. Holzapfel, Y. Hori, J. Hubmayr, K. Ichiki, H. Imada, J. Inatani, M. Inoue, Y. Inoue, F. Irie, K. Irwin, H. Ishitsuka, O. Jeong, H. Kanai, K. Karatsu, S. Kashima, N. Katayama, I. Kawano, T. Kawasaki, B. Keating, S. Kernasovskiy, R. Keskitalo, A. Kibayashi, Y. Kida, N. Kimura, K. Kimura, T. Kisner, K. Kohri, E. Komatsu, K. Komatsu, C. L. Kuo, S. Kuromiya, A. Kusaka, A. Lee, D. Li, E. Linder, M. Maki, H. Matsuhara, T. Matsumura, S. Matsuoka, S. Matsuura, S. Mima, Y. Minami, K. Mitsuda, M. Nagai, T. Nagasaki, R. Nagata, M. Nakajima, S. Nakamura, T. Namikawa, M. Naruse, T. Nishibori, K. Nishijo, H. Nishino, A. Noda, T. Noguchi, H. Ogawa, W. Ogburn, S. Oguri, I. Ohta, N. Okada, A. Okamoto, T. Okamura, C. Otani, G. Pisano, G. Rebeiz, P. Richards, S. Sakai, Y. Sakurai, Y. Sato, N. Sato, Y. Segawa, S. Sekiguchi, Y. Sekimoto, M. Sekine, U. Seljak, B. Sherwin, T. Shimizu, K. Shinozaki, S. Shu, R. Stompor, H. Sugai, H. Sugita, J. Suzuki, T. Suzuki, A. Suzuki, O. Tajima, S. Takada, S. Takakura, K. Takano, S. Takatori, Y. Takei, D. Tanabe, T. Tomaru, N. Tomita, P. Turin, S. Uozumi, S. Utsunomiya, Y. Uzawa, T. Wada, H. Watanabe, B. Westbrook, N. Whitehorn, Y. Yamada, R. Yamamoto, N. Yamasaki, T. Yamashita, T. Yoshida, M. Yoshida, K. Yotsumoto

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

36 Scopus citations

Abstract

LiteBIRD is a next generation satellite aiming for the detection of the Cosmic Microwave Background (CMB) B-mode polarization imprinted by the primordial gravitational waves generated in the era of the inflationary universe. The science goal of LiteBIRD is to measure the tensor-to-scaler ratio r with a precision of δr < 10^-3♦, oering us a crucial test of the major large-single-field slow-roll inflation models. LiteBIRD is planned to conduct an all sky survey at the sun-earth second Lagrange point (L2) with an angular resolution of about 0.5 degrees to cover the multipole moment range of 2 ≤ ℓ ≤ 200. We use focal plane detector arrays consisting of 2276 superconducting detectors to measure the frequency range from 40 to 400 GHz with the sensitivity of 3.2 μK·arcmin. including the ongoing studies.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2016
Subtitle of host publication	Optical, Infrared, and Millimeter Wave
Editors	Howard A. MacEwen, Makenzie Lystrup, Giovanni G. Fazio
Publisher	SPIE
ISBN (Electronic)	9781510601871
DOIs	https://doi.org/10.1117/12.2231995
State	Published - 2016
Event	Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave - Edinburgh, United Kingdom Duration: 26 Jun 2016 → 1 Jul 2016

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9904
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave
Country/Territory	United Kingdom
City	Edinburgh
Period	26/06/16 → 1/07/16

Keywords

B-mode polarization
Cosmic microwave background
LiteBIRD

Access to Document

10.1117/12.2231995

Cite this

Ishino, H., Akiba, Y., Arnold, K., Barron, D., Borrill, J., Chendra, R., Chinone, Y., Cho, S., Cukierman, A., De Haan, T., Dobbs, M., Dominjon, A., Dotani, T., Elleflot, T., Errard, J., Fujino, T., Fuke, H., Funaki, T., Goeckner-Wald, N., ... Yotsumoto, K. (2016). LiteBIRD: Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection. In H. A. MacEwen, M. Lystrup, & G. G. Fazio (Eds.), Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave Article 99040X (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9904). SPIE. https://doi.org/10.1117/12.2231995

Ishino, H. ; Akiba, Y. ; Arnold, K. et al. / LiteBIRD : Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection. Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave. editor / Howard A. MacEwen ; Makenzie Lystrup ; Giovanni G. Fazio. SPIE, 2016. (Proceedings of SPIE - The International Society for Optical Engineering).

@inproceedings{b06aba8fd79641b0bfd96d74989b5e47,

title = "LiteBIRD: Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection",

abstract = "LiteBIRD is a next generation satellite aiming for the detection of the Cosmic Microwave Background (CMB) B-mode polarization imprinted by the primordial gravitational waves generated in the era of the inflationary universe. The science goal of LiteBIRD is to measure the tensor-to-scaler ratio r with a precision of δr < 10-3♦, oering us a crucial test of the major large-single-field slow-roll inflation models. LiteBIRD is planned to conduct an all sky survey at the sun-earth second Lagrange point (L2) with an angular resolution of about 0.5 degrees to cover the multipole moment range of 2 ≤ ℓ ≤ 200. We use focal plane detector arrays consisting of 2276 superconducting detectors to measure the frequency range from 40 to 400 GHz with the sensitivity of 3.2 μK·arcmin. including the ongoing studies.",

keywords = "B-mode polarization, Cosmic microwave background, LiteBIRD",

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

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year = "2016",

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series = "Proceedings of SPIE - The International Society for Optical Engineering",

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editor = "MacEwen, {Howard A.} and Makenzie Lystrup and Fazio, {Giovanni G.}",

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Ishino, H, Akiba, Y, Arnold, K, Barron, D, Borrill, J, Chendra, R, Chinone, Y, Cho, S, Cukierman, A, De Haan, T, Dobbs, M, Dominjon, A, Dotani, T, Elleflot, T, Errard, J, Fujino, T, Fuke, H, Funaki, T, Goeckner-Wald, N, Halverson, N, Harvey, P, Hasebe, T, Hasegawa, M, Hattori, K, Hattori, M, Hazumi, M, Hidehira, N, Hill, C, Hilton, G, Holzapfel, W, Hori, Y, Hubmayr, J, Ichiki, K, Imada, H, Inatani, J, Inoue, M, Inoue, Y, Irie, F, Irwin, K, Ishitsuka, H, Jeong, O, Kanai, H, Karatsu, K, Kashima, S, Katayama, N, Kawano, I, Kawasaki, T, Keating, B, Kernasovskiy, S, Keskitalo, R, Kibayashi, A, Kida, Y, Kimura, N, Kimura, K, Kisner, T, Kohri, K, Komatsu, E, Komatsu, K, Kuo, CL, Kuromiya, S, Kusaka, A, Lee, A, Li, D, Linder, E, Maki, M, Matsuhara, H, Matsumura, T, Matsuoka, S, Matsuura, S, Mima, S, Minami, Y, Mitsuda, K, Nagai, M, Nagasaki, T, Nagata, R, Nakajima, M, Nakamura, S, Namikawa, T, Naruse, M, Nishibori, T, Nishijo, K, Nishino, H, Noda, A, Noguchi, T, Ogawa, H, Ogburn, W, Oguri, S, Ohta, I, Okada, N, Okamoto, A, Okamura, T, Otani, C, Pisano, G, Rebeiz, G, Richards, P, Sakai, S, Sakurai, Y, Sato, Y, Sato, N, Segawa, Y, Sekiguchi, S, Sekimoto, Y, Sekine, M, Seljak, U, Sherwin, B, Shimizu, T, Shinozaki, K, Shu, S, Stompor, R, Sugai, H, Sugita, H, Suzuki, J, Suzuki, T, Suzuki, A, Tajima, O, Takada, S, Takakura, S, Takano, K, Takatori, S, Takei, Y, Tanabe, D, Tomaru, T, Tomita, N, Turin, P, Uozumi, S, Utsunomiya, S, Uzawa, Y, Wada, T, Watanabe, H, Westbrook, B, Whitehorn, N, Yamada, Y, Yamamoto, R, Yamasaki, N, Yamashita, T, Yoshida, T, Yoshida, M & Yotsumoto, K 2016, LiteBIRD: Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection. in HA MacEwen, M Lystrup & GG Fazio (eds), Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave., 99040X, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9904, SPIE, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, Edinburgh, United Kingdom, 26/06/16. https://doi.org/10.1117/12.2231995

LiteBIRD: Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection. / Ishino, H.; Akiba, Y.; Arnold, K. et al.
Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave. ed. / Howard A. MacEwen; Makenzie Lystrup; Giovanni G. Fazio. SPIE, 2016. 99040X (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9904).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - LiteBIRD

T2 - Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave

AU - Ishino, H.

AU - Akiba, Y.

AU - Arnold, K.

AU - Barron, D.

AU - Borrill, J.

AU - Chendra, R.

AU - Chinone, Y.

AU - Cho, S.

AU - Cukierman, A.

AU - De Haan, T.

AU - Dobbs, M.

AU - Dominjon, A.

AU - Dotani, T.

AU - Elleflot, T.

AU - Errard, J.

AU - Fujino, T.

AU - Fuke, H.

AU - Funaki, T.

AU - Goeckner-Wald, N.

AU - Halverson, N.

AU - Harvey, P.

AU - Hasebe, T.

AU - Hasegawa, M.

AU - Hattori, K.

AU - Hattori, M.

AU - Hazumi, M.

AU - Hidehira, N.

AU - Hill, C.

AU - Hilton, G.

AU - Holzapfel, W.

AU - Hori, Y.

AU - Hubmayr, J.

AU - Ichiki, K.

AU - Imada, H.

AU - Inatani, J.

AU - Inoue, M.

AU - Inoue, Y.

AU - Irie, F.

AU - Irwin, K.

AU - Ishitsuka, H.

AU - Jeong, O.

AU - Kanai, H.

AU - Karatsu, K.

AU - Kashima, S.

AU - Katayama, N.

AU - Kawano, I.

AU - Kawasaki, T.

AU - Keating, B.

AU - Kernasovskiy, S.

AU - Keskitalo, R.

AU - Kibayashi, A.

AU - Kida, Y.

AU - Kimura, N.

AU - Kimura, K.

AU - Kisner, T.

AU - Kohri, K.

AU - Komatsu, E.

AU - Komatsu, K.

AU - Kuo, C. L.

AU - Kuromiya, S.

AU - Kusaka, A.

AU - Lee, A.

AU - Li, D.

AU - Linder, E.

AU - Maki, M.

AU - Matsuhara, H.

AU - Matsumura, T.

AU - Matsuoka, S.

AU - Matsuura, S.

AU - Mima, S.

AU - Minami, Y.

AU - Mitsuda, K.

AU - Nagai, M.

AU - Nagasaki, T.

AU - Nagata, R.

AU - Nakajima, M.

AU - Nakamura, S.

AU - Namikawa, T.

AU - Naruse, M.

AU - Nishibori, T.

AU - Nishijo, K.

AU - Nishino, H.

AU - Noda, A.

AU - Noguchi, T.

AU - Ogawa, H.

AU - Ogburn, W.

AU - Oguri, S.

AU - Ohta, I.

AU - Okada, N.

AU - Okamoto, A.

AU - Okamura, T.

AU - Otani, C.

AU - Pisano, G.

AU - Rebeiz, G.

AU - Richards, P.

AU - Sakai, S.

AU - Sakurai, Y.

AU - Sato, Y.

AU - Sato, N.

AU - Segawa, Y.

AU - Sekiguchi, S.

AU - Sekimoto, Y.

AU - Sekine, M.

AU - Seljak, U.

AU - Sherwin, B.

AU - Shimizu, T.

AU - Shinozaki, K.

AU - Shu, S.

AU - Stompor, R.

AU - Sugai, H.

AU - Sugita, H.

AU - Suzuki, J.

AU - Suzuki, T.

AU - Suzuki, A.

AU - Tajima, O.

AU - Takada, S.

AU - Takakura, S.

AU - Takano, K.

AU - Takatori, S.

AU - Takei, Y.

AU - Tanabe, D.

AU - Tomaru, T.

AU - Tomita, N.

AU - Turin, P.

AU - Uozumi, S.

AU - Utsunomiya, S.

AU - Uzawa, Y.

AU - Wada, T.

AU - Watanabe, H.

AU - Westbrook, B.

AU - Whitehorn, N.

AU - Yamada, Y.

AU - Yamamoto, R.

AU - Yamasaki, N.

AU - Yamashita, T.

AU - Yoshida, T.

AU - Yoshida, M.

AU - Yotsumoto, K.

PY - 2016

Y1 - 2016

N2 - LiteBIRD is a next generation satellite aiming for the detection of the Cosmic Microwave Background (CMB) B-mode polarization imprinted by the primordial gravitational waves generated in the era of the inflationary universe. The science goal of LiteBIRD is to measure the tensor-to-scaler ratio r with a precision of δr < 10-3♦, oering us a crucial test of the major large-single-field slow-roll inflation models. LiteBIRD is planned to conduct an all sky survey at the sun-earth second Lagrange point (L2) with an angular resolution of about 0.5 degrees to cover the multipole moment range of 2 ≤ ℓ ≤ 200. We use focal plane detector arrays consisting of 2276 superconducting detectors to measure the frequency range from 40 to 400 GHz with the sensitivity of 3.2 μK·arcmin. including the ongoing studies.

AB - LiteBIRD is a next generation satellite aiming for the detection of the Cosmic Microwave Background (CMB) B-mode polarization imprinted by the primordial gravitational waves generated in the era of the inflationary universe. The science goal of LiteBIRD is to measure the tensor-to-scaler ratio r with a precision of δr < 10-3♦, oering us a crucial test of the major large-single-field slow-roll inflation models. LiteBIRD is planned to conduct an all sky survey at the sun-earth second Lagrange point (L2) with an angular resolution of about 0.5 degrees to cover the multipole moment range of 2 ≤ ℓ ≤ 200. We use focal plane detector arrays consisting of 2276 superconducting detectors to measure the frequency range from 40 to 400 GHz with the sensitivity of 3.2 μK·arcmin. including the ongoing studies.

KW - B-mode polarization

KW - Cosmic microwave background

KW - LiteBIRD

UR - http://www.scopus.com/inward/record.url?scp=84991396066&partnerID=8YFLogxK

U2 - 10.1117/12.2231995

DO - 10.1117/12.2231995

M3 - 會議論文篇章

AN - SCOPUS:84991396066

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2016

A2 - MacEwen, Howard A.

A2 - Lystrup, Makenzie

A2 - Fazio, Giovanni G.

PB - SPIE

Y2 - 26 June 2016 through 1 July 2016

ER -

Ishino H, Akiba Y, Arnold K, Barron D, Borrill J, Chendra R et al. LiteBIRD: Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection. In MacEwen HA, Lystrup M, Fazio GG, editors, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave. SPIE. 2016. 99040X. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2231995

LiteBIRD: Lite satellite for the study of B-mode polarization and inflation from cosmic microwave background radiation detection

Abstract

Publication series

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Keywords

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