Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD

T. Hasebe; S. Kashima; P. A.R. Ade; Y. Akiba; D. Alonso; K. Arnold; J. Aumont; C. Baccigalupi; D. Barron; S. Basak; S. Beckman; J. Borrill; F. Boulanger; M. Bucher; E. Calabrese; Y. Chinone; H. M. Cho; A. Cukierman; D. W. Curtis; T. de Haan; M. Dobbs; A. Dominjon; T. Dotani; L. Duband; A. Ducout; J. Dunkley; J. M. Duval; T. Elleflot; H. K. Eriksen; J. Errard; J. Fischer; T. Fujino; T. Funaki; U. Fuskeland; K. Ganga; N. Goeckner-Wald; J. Grain; N. W. Halverson; T. Hamada; M. Hasegawa; K. Hattori; M. Hattori; L. Hayes; M. Hazumi; N. Hidehira; C. A. Hill; G. Hilton; J. Hubmayr; K. Ichiki; T. Iida; H. Imada; M. Inoue; Y. Inoue; K. D. Irwin; H. Ishino; O. Jeong; H. Kanai; D. Kaneko; N. Katayama; T. Kawasaki; S. A. Kernasovskiy; R. Keskitalo; A. Kibayashi; Y. Kida; K. Kimura; T. Kisner; K. Kohri; E. Komatsu; K. Komatsu; C. L. Kuo; N. A. Kurinsky; A. Kusaka; A. Lazarian; A. T. Lee; D. Li; E. Linder; B. Maffei; A. Mangilli; M. Maki; T. Matsumura; S. Matsuura; D. Meilhan; S. Mima; Y. Minami; K. Mitsuda; L. Montier; M. Nagai; T. Nagasaki; R. Nagata; M. Nakajima; S. Nakamura; T. Namikawa; M. Naruse; H. Nishino; T. Nitta; T. Noguchi; H. Ogawa; S. Oguri; N. Okada; A. Okamoto; T. Okamura; C. Otani; G. Patanchon; G. Pisano; G. Rebeiz; M. Remazeilles; P. L. Richards; S. Sakai; Y. Sakurai; Y. Sato; N. Sato; M. Sawada; Y. Segawa; Y. Sekimoto; U. Seljak; B. D. Sherwin; T. Shimizu; K. Shinozaki; R. Stompor; H. Sugai; H. Sugita; A. Suzuki; J. Suzuki; O. Tajima; S. Takada; R. Takaku; S. Takakura; S. Takatori; D. Tanabe; E. Taylor; K. L. Thompson; B. Thorne; T. Tomaru; T. Tomida; N. Tomita; M. Tristram; C. Tucker; P. Turin; M. Tsujimoto; S. Uozumi; S. Utsunomiya; Y. Uzawa; F. Vansyngel; I. K. Wehus; B. Westbrook; M. Willer; N. Whitehorn; Y. Yamada; R. Yamamoto; N. Yamasaki; T. Yamashita; M. Yoshida

doi:10.1007/s10909-018-1915-2

Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD

T. Hasebe
, S. Kashima
, P. A.R. Ade
, Y. Akiba
, D. Alonso
, K. Arnold
, J. Aumont
, C. Baccigalupi
, D. Barron
, S. Basak
, S. Beckman
, J. Borrill
, F. Boulanger
, M. Bucher
, E. Calabrese
, Y. Chinone
, H. M. Cho
, A. Cukierman
, D. W. Curtis
, T. de Haan

M. Dobbs, A. Dominjon, T. Dotani, L. Duband, A. Ducout, J. Dunkley, J. M. Duval, T. Elleflot, H. K. Eriksen, J. Errard, J. Fischer, T. Fujino, T. Funaki, U. Fuskeland, K. Ganga, N. Goeckner-Wald, J. Grain, N. W. Halverson, T. Hamada, M. Hasegawa, K. Hattori, M. Hattori, L. Hayes, M. Hazumi, N. Hidehira, C. A. Hill, G. Hilton, J. Hubmayr, K. Ichiki, T. Iida, H. Imada, M. Inoue, Y. Inoue, K. D. Irwin, H. Ishino, O. Jeong, H. Kanai, D. Kaneko, N. Katayama, T. Kawasaki, S. A. Kernasovskiy, R. Keskitalo, A. Kibayashi, Y. Kida, K. Kimura, T. Kisner, K. Kohri, E. Komatsu, K. Komatsu, C. L. Kuo, N. A. Kurinsky, A. Kusaka, A. Lazarian, A. T. Lee, D. Li, E. Linder, B. Maffei, A. Mangilli, M. Maki, T. Matsumura, S. Matsuura, D. Meilhan, S. Mima, Y. Minami, K. Mitsuda, L. Montier, M. Nagai, T. Nagasaki, R. Nagata, M. Nakajima, S. Nakamura, T. Namikawa, M. Naruse, H. Nishino, T. Nitta, T. Noguchi, H. Ogawa, S. Oguri, N. Okada, A. Okamoto, T. Okamura, C. Otani, G. Patanchon, G. Pisano, G. Rebeiz, M. Remazeilles, P. L. Richards, S. Sakai, Y. Sakurai, Y. Sato, N. Sato, M. Sawada, Y. Segawa, Y. Sekimoto, U. Seljak, B. D. Sherwin, T. Shimizu, K. Shinozaki, R. Stompor, H. Sugai, H. Sugita, A. Suzuki, J. Suzuki, O. Tajima, S. Takada, R. Takaku, S. Takakura, S. Takatori, D. Tanabe, E. Taylor, K. L. Thompson, B. Thorne, T. Tomaru, T. Tomida, N. Tomita, M. Tristram, C. Tucker, P. Turin, M. Tsujimoto, S. Uozumi, S. Utsunomiya, Y. Uzawa, F. Vansyngel, I. K. Wehus, B. Westbrook, M. Willer, N. Whitehorn, Y. Yamada, R. Yamamoto, N. Yamasaki, T. Yamashita, M. Yoshida

Research output: Contribution to journal › Article › peer-review

6 Scopus citations

Abstract

The high-frequency telescope for LiteBIRD is designed with refractive and reflective optics. In order to improve sensitivity, this paper suggests the new optical configurations of the HFT which have approximately 7 times larger focal planes than that of the original design. The sensitivities of both the designs are compared, and the requirement of anti-reflection (AR) coating on the lens for the refractive option is derived. We also present the simulation result of a sub-wavelength AR structure on both surfaces of silicon, which shows a band-averaged reflection of 1.1–3.2% at 101–448 GHz.

Original language	English (US)
Pages (from-to)	841-850
Number of pages	10
Journal	Journal of Low Temperature Physics
Volume	193
Issue number	5-6
DOIs	https://doi.org/10.1007/s10909-018-1915-2
State	Published - Dec 1 2018

All Science Journal Classification (ASJC) codes

Atomic and Molecular Physics, and Optics
General Materials Science
Condensed Matter Physics

Keywords

Cosmic microwave background radiation
Inflation
Satellite
Telescope

Access to Document

10.1007/s10909-018-1915-2

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Hasebe, T., Kashima, S., Ade, P. A. R., Akiba, Y., Alonso, D., Arnold, K., Aumont, J., Baccigalupi, C., Barron, D., Basak, S., Beckman, S., Borrill, J., Boulanger, F., Bucher, M., Calabrese, E., Chinone, Y., Cho, H. M., Cukierman, A., Curtis, D. W., ... Yoshida, M. (2018). Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD. Journal of Low Temperature Physics, 193(5-6), 841-850. https://doi.org/10.1007/s10909-018-1915-2

@article{b40a19d9c6cf480e9da8ebad12ed3629,

title = "Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD",

abstract = "The high-frequency telescope for LiteBIRD is designed with refractive and reflective optics. In order to improve sensitivity, this paper suggests the new optical configurations of the HFT which have approximately 7 times larger focal planes than that of the original design. The sensitivities of both the designs are compared, and the requirement of anti-reflection (AR) coating on the lens for the refractive option is derived. We also present the simulation result of a sub-wavelength AR structure on both surfaces of silicon, which shows a band-averaged reflection of 1.1–3.2\% at 101–448 GHz.",

keywords = "Cosmic microwave background radiation, Inflation, Satellite, Telescope",

author = "T. Hasebe and S. Kashima and Ade, \{P. A.R.\} and Y. Akiba and D. Alonso and K. Arnold and J. Aumont and C. Baccigalupi and D. Barron and S. Basak and S. Beckman and J. Borrill and F. Boulanger and M. Bucher and E. Calabrese and Y. Chinone and Cho, \{H. M.\} and A. Cukierman and Curtis, \{D. W.\} and \{de Haan\}, T. and M. Dobbs and A. Dominjon and T. Dotani and L. Duband and A. Ducout and J. Dunkley and Duval, \{J. M.\} and T. Elleflot and Eriksen, \{H. K.\} and J. Errard and J. Fischer and T. Fujino and T. Funaki and U. Fuskeland and K. Ganga and N. Goeckner-Wald and J. Grain and Halverson, \{N. W.\} and T. Hamada and M. Hasegawa and K. Hattori and M. Hattori and L. Hayes and M. Hazumi and N. Hidehira and Hill, \{C. A.\} and G. Hilton and J. Hubmayr and K. Ichiki and T. Iida and H. Imada and M. Inoue and Y. Inoue and Irwin, \{K. D.\} and H. Ishino and O. Jeong and H. Kanai and D. Kaneko and N. Katayama and T. Kawasaki and Kernasovskiy, \{S. A.\} and R. Keskitalo and A. Kibayashi and Y. Kida and K. Kimura and T. Kisner and K. Kohri and E. Komatsu and K. Komatsu and Kuo, \{C. L.\} and Kurinsky, \{N. A.\} and A. Kusaka and A. Lazarian and Lee, \{A. T.\} and D. Li and E. Linder and B. Maffei and A. Mangilli and M. Maki and T. Matsumura and S. Matsuura and D. Meilhan and S. Mima and Y. Minami and K. Mitsuda and L. Montier and M. Nagai and T. Nagasaki and R. Nagata and M. Nakajima and S. Nakamura and T. Namikawa and M. Naruse and H. Nishino and T. Nitta and T. Noguchi and H. Ogawa and S. Oguri and N. Okada and A. Okamoto and T. Okamura and C. Otani and G. Patanchon and G. Pisano and G. Rebeiz and M. Remazeilles and Richards, \{P. L.\} and S. Sakai and Y. Sakurai and Y. Sato and N. Sato and M. Sawada and Y. Segawa and Y. Sekimoto and U. Seljak and Sherwin, \{B. D.\} and T. Shimizu and K. Shinozaki and R. Stompor and H. Sugai and H. Sugita and A. Suzuki and J. Suzuki and O. Tajima and S. Takada and R. Takaku and S. Takakura and S. Takatori and D. Tanabe and E. Taylor and Thompson, \{K. L.\} and B. Thorne and T. Tomaru and T. Tomida and N. Tomita and M. Tristram and C. Tucker and P. Turin and M. Tsujimoto and S. Uozumi and S. Utsunomiya and Y. Uzawa and F. Vansyngel and Wehus, \{I. K.\} and B. Westbrook and M. Willer and N. Whitehorn and Y. Yamada and R. Yamamoto and N. Yamasaki and T. Yamashita and M. Yoshida",

note = "Publisher Copyright: {\textcopyright} 2018, Springer Science+Business Media, LLC, part of Springer Nature.",

year = "2018",

month = dec,

day = "1",

doi = "10.1007/s10909-018-1915-2",

language = "English (US)",

volume = "193",

pages = "841--850",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer New York",

number = "5-6",

}

Hasebe, T, Kashima, S, Ade, PAR, Akiba, Y, Alonso, D, Arnold, K, Aumont, J, Baccigalupi, C, Barron, D, Basak, S, Beckman, S, Borrill, J, Boulanger, F, Bucher, M, Calabrese, E, Chinone, Y, Cho, HM, Cukierman, A, Curtis, DW, de Haan, T, Dobbs, M, Dominjon, A, Dotani, T, Duband, L, Ducout, A, Dunkley, J, Duval, JM, Elleflot, T, Eriksen, HK, Errard, J, Fischer, J, Fujino, T, Funaki, T, Fuskeland, U, Ganga, K, Goeckner-Wald, N, Grain, J, Halverson, NW, Hamada, T, Hasegawa, M, Hattori, K, Hattori, M, Hayes, L, Hazumi, M, Hidehira, N, Hill, CA, Hilton, G, Hubmayr, J, Ichiki, K, Iida, T, Imada, H, Inoue, M, Inoue, Y, Irwin, KD, Ishino, H, Jeong, O, Kanai, H, Kaneko, D, Katayama, N, Kawasaki, T, Kernasovskiy, SA, Keskitalo, R, Kibayashi, A, Kida, Y, Kimura, K, Kisner, T, Kohri, K, Komatsu, E, Komatsu, K, Kuo, CL, Kurinsky, NA, Kusaka, A, Lazarian, A, Lee, AT, Li, D, Linder, E, Maffei, B, Mangilli, A, Maki, M, Matsumura, T, Matsuura, S, Meilhan, D, Mima, S, Minami, Y, Mitsuda, K, Montier, L, Nagai, M, Nagasaki, T, Nagata, R, Nakajima, M, Nakamura, S, Namikawa, T, Naruse, M, Nishino, H, Nitta, T, Noguchi, T, Ogawa, H, Oguri, S, Okada, N, Okamoto, A, Okamura, T, Otani, C, Patanchon, G, Pisano, G, Rebeiz, G, Remazeilles, M, Richards, PL, Sakai, S, Sakurai, Y, Sato, Y, Sato, N, Sawada, M, Segawa, Y, Sekimoto, Y, Seljak, U, Sherwin, BD, Shimizu, T, Shinozaki, K, Stompor, R, Sugai, H, Sugita, H, Suzuki, A, Suzuki, J, Tajima, O, Takada, S, Takaku, R, Takakura, S, Takatori, S, Tanabe, D, Taylor, E, Thompson, KL, Thorne, B, Tomaru, T, Tomida, T, Tomita, N, Tristram, M, Tucker, C, Turin, P, Tsujimoto, M, Uozumi, S, Utsunomiya, S, Uzawa, Y, Vansyngel, F, Wehus, IK, Westbrook, B, Willer, M, Whitehorn, N, Yamada, Y, Yamamoto, R, Yamasaki, N, Yamashita, T & Yoshida, M 2018, 'Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD', Journal of Low Temperature Physics, vol. 193, no. 5-6, pp. 841-850. https://doi.org/10.1007/s10909-018-1915-2

TY - JOUR

T1 - Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD

AU - Hasebe, T.

AU - Kashima, S.

AU - Ade, P. A.R.

AU - Akiba, Y.

AU - Alonso, D.

AU - Arnold, K.

AU - Aumont, J.

AU - Baccigalupi, C.

AU - Barron, D.

AU - Basak, S.

AU - Beckman, S.

AU - Borrill, J.

AU - Boulanger, F.

AU - Bucher, M.

AU - Calabrese, E.

AU - Chinone, Y.

AU - Cho, H. M.

AU - Cukierman, A.

AU - Curtis, D. W.

AU - de Haan, T.

AU - Dobbs, M.

AU - Dominjon, A.

AU - Dotani, T.

AU - Duband, L.

AU - Ducout, A.

AU - Dunkley, J.

AU - Duval, J. M.

AU - Elleflot, T.

AU - Eriksen, H. K.

AU - Errard, J.

AU - Fischer, J.

AU - Fujino, T.

AU - Funaki, T.

AU - Fuskeland, U.

AU - Ganga, K.

AU - Goeckner-Wald, N.

AU - Grain, J.

AU - Halverson, N. W.

AU - Hamada, T.

AU - Hasegawa, M.

AU - Hattori, K.

AU - Hattori, M.

AU - Hayes, L.

AU - Hazumi, M.

AU - Hidehira, N.

AU - Hill, C. A.

AU - Hilton, G.

AU - Hubmayr, J.

AU - Ichiki, K.

AU - Iida, T.

AU - Imada, H.

AU - Inoue, M.

AU - Inoue, Y.

AU - Irwin, K. D.

AU - Ishino, H.

AU - Jeong, O.

AU - Kanai, H.

AU - Kaneko, D.

AU - Katayama, N.

AU - Kawasaki, T.

AU - Kernasovskiy, S. A.

AU - Keskitalo, R.

AU - Kibayashi, A.

AU - Kida, Y.

AU - Kimura, K.

AU - Kisner, T.

AU - Kohri, K.

AU - Komatsu, E.

AU - Komatsu, K.

AU - Kuo, C. L.

AU - Kurinsky, N. A.

AU - Kusaka, A.

AU - Lazarian, A.

AU - Lee, A. T.

AU - Li, D.

AU - Linder, E.

AU - Maffei, B.

AU - Mangilli, A.

AU - Maki, M.

AU - Matsumura, T.

AU - Matsuura, S.

AU - Meilhan, D.

AU - Mima, S.

AU - Minami, Y.

AU - Mitsuda, K.

AU - Montier, L.

AU - Nagai, M.

AU - Nagasaki, T.

AU - Nagata, R.

AU - Nakajima, M.

AU - Nakamura, S.

AU - Namikawa, T.

AU - Naruse, M.

AU - Nishino, H.

AU - Nitta, T.

AU - Noguchi, T.

AU - Ogawa, H.

AU - Oguri, S.

AU - Okada, N.

AU - Okamoto, A.

AU - Okamura, T.

AU - Otani, C.

AU - Patanchon, G.

AU - Pisano, G.

AU - Rebeiz, G.

AU - Remazeilles, M.

AU - Richards, P. L.

AU - Sakai, S.

AU - Sakurai, Y.

AU - Sato, Y.

AU - Sato, N.

AU - Sawada, M.

AU - Segawa, Y.

AU - Sekimoto, Y.

AU - Seljak, U.

AU - Sherwin, B. D.

AU - Shimizu, T.

AU - Shinozaki, K.

AU - Stompor, R.

AU - Sugai, H.

AU - Sugita, H.

AU - Suzuki, A.

AU - Suzuki, J.

AU - Tajima, O.

AU - Takada, S.

AU - Takaku, R.

AU - Takakura, S.

AU - Takatori, S.

AU - Tanabe, D.

AU - Taylor, E.

AU - Thompson, K. L.

AU - Thorne, B.

AU - Tomaru, T.

AU - Tomida, T.

AU - Tomita, N.

AU - Tristram, M.

AU - Tucker, C.

AU - Turin, P.

AU - Tsujimoto, M.

AU - Uozumi, S.

AU - Utsunomiya, S.

AU - Uzawa, Y.

AU - Vansyngel, F.

AU - Wehus, I. K.

AU - Westbrook, B.

AU - Willer, M.

AU - Whitehorn, N.

AU - Yamada, Y.

AU - Yamamoto, R.

AU - Yamasaki, N.

AU - Yamashita, T.

AU - Yoshida, M.

PY - 2018/12/1

Y1 - 2018/12/1

N2 - The high-frequency telescope for LiteBIRD is designed with refractive and reflective optics. In order to improve sensitivity, this paper suggests the new optical configurations of the HFT which have approximately 7 times larger focal planes than that of the original design. The sensitivities of both the designs are compared, and the requirement of anti-reflection (AR) coating on the lens for the refractive option is derived. We also present the simulation result of a sub-wavelength AR structure on both surfaces of silicon, which shows a band-averaged reflection of 1.1–3.2% at 101–448 GHz.

AB - The high-frequency telescope for LiteBIRD is designed with refractive and reflective optics. In order to improve sensitivity, this paper suggests the new optical configurations of the HFT which have approximately 7 times larger focal planes than that of the original design. The sensitivities of both the designs are compared, and the requirement of anti-reflection (AR) coating on the lens for the refractive option is derived. We also present the simulation result of a sub-wavelength AR structure on both surfaces of silicon, which shows a band-averaged reflection of 1.1–3.2% at 101–448 GHz.

KW - Cosmic microwave background radiation

KW - Inflation

KW - Satellite

KW - Telescope

UR - https://www.scopus.com/pages/publications/85046822941

UR - https://www.scopus.com/pages/publications/85046822941#tab=citedBy

U2 - 10.1007/s10909-018-1915-2

DO - 10.1007/s10909-018-1915-2

M3 - Article

AN - SCOPUS:85046822941

SN - 0022-2291

VL - 193

SP - 841

EP - 850

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 5-6

ER -

Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD

Abstract

All Science Journal Classification (ASJC) codes

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