LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization

M. Hazumi; P. A.R. Ade; A. Adler; E. Allys; K. Arnold; D. Auguste; J. Aumont; R. Aurlien; J. Austermann; C. Baccigalupi; A. J. Banday; R. Banjeri; R. B. Barreiro; S. Basak; J. Beall; D. Beck; S. Beckman; J. Bermejo; P. De Bernardis; M. Bersanelli; J. Bonis; J. Borrill; F. Boulanger; S. Bounissou; M. Brilenkov; M. Brown; M. Bucher; E. Calabrese; P. Campeti; A. Carones; F. J. Casas; A. Challinor; V. Chan; K. Cheung; Y. Chinone; J. F. Cliche; L. Colombo; F. Columbro; J. Cubas; A. Cukierman; D. Curtis; G. D'alessandro; N. Dachlythra; M. De Petris; C. Dickinson; P. Diego-Palazuelos; M. Dobbs; T. Dotani; L. Duband; S. Duff; J. M. Duval; K. Ebisawa; T. Elleflot; H. K. Eriksen; J. Errard; T. Essinger-Hileman; F. Finelli; R. Flauger; C. Franceschet; U. Fuskeland; M. Galloway; K. Ganga; J. R. Gao; R. Genova-Santos; M. Gerbino; M. Gervasi; T. Ghigna; E. Gjerløw; M. L. Gradziel; J. Grain; F. Grupp; A. Gruppuso; J. E. Gudmundsson; T. De Haan; N. W. Halverson; P. Hargrave; T. Hasebe; M. Hasegawa; M. Hattori; S. Henrot-Versillé; D. Herman; D. Herranz; C. A. Hill; G. Hilton; Y. Hirota; E. Hivon; R. A. Hlozek; Y. Hoshino; E. De La Hoz; J. Hubmayr; K. Ichiki; T. Iida; H. Imada; K. Ishimura; H. Ishino; G. Jaehnig; T. Kaga; S. Kashima; N. Katayama; A. Kato; T. Kawasaki; R. Keskitalo; T. Kisner; Y. Kobayashi; N. Kogiso; A. Kogut; K. Kohri; E. Komatsu; K. Komatsu; K. Konishi; N. Krachmalnicoff; I. Kreykenbohm; C. L. Kuo; A. Kushino; L. Lamagna; J. V. Lanen; M. Lattanzi; A. T. Lee; C. Leloup; F. Levrier; E. Linder; T. Louis; G. Luzzi; T. Maciaszek; B. Maffei; D. Maino; M. Maki; S. Mandelli; E. Martinez-Gonzalez; S. Masi; T. Matsumura; A. Mennella; M. Migliaccio; Y. Minami; K. Mitsuda; J. Montgomery; L. Montier; G. Morgante; B. Mot; Y. Murata; J. A. Murphy; M. Nagai; Y. Nagano; T. Nagasaki; R. Nagata; S. Nakamura; T. Namikawa; P. Natoli; S. Nerval; T. Nishibori; H. Nishino; F. Noviello; C. O'sullivan; H. Ogawa; H. Ogawa; S. Oguri; H. Ohsaki; I. S. Ohta; N. Okada; N. Okada; L. Pagano; A. Paiella; D. Paoletti; G. Patanchon; J. Peloton; F. Piacentini; G. Pisano; G. Polenta; D. Poletti; T. Prouvé; G. Puglisi; D. Rambaud; C. Raum; S. Realini; M. Reinecke; M. Remazeilles; A. Ritacco; G. Roudil; J. A. Rubino-Martin; M. Russell; H. Sakurai; Y. Sakurai; M. Sandri; M. Sasaki; G. Savini; D. Scott; J. Seibert; Y. Sekimoto; B. Sherwin; K. Shinozaki; M. Shiraishi; P. Shirron; G. Signorelli; G. Smecher; S. Stever; R. Stompor; H. Sugai; S. Sugiyama; A. Suzuki; J. Suzuki; T. L. Svalheim; E. Switzer; R. Takaku; H. Takakura; S. Takakura; Y. Takase; Y. Takeda; A. Tartari; E. Taylor; Y. Terao; H. Thommesen; K. L. Thompson; B. Thorne; T. Toda; M. Tomasi; M. Tominaga; N. Trappe; M. Tristram; M. Tsuji; M. Tsujimoto; C. Tucker; J. Ullom; G. Vermeulen; P. Vielva; F. Villa; M. Vissers; N. Vittorio; I. Wehus; J. Weller; B. Westbrook; J. Wilms; B. Winter; E. J. Wollack; N. Y. Yamasaki; T. Yoshida; J. Yumoto; M. Zannoni; A. Zonca

doi:10.1117/12.2563050

LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization

M. Hazumi^*, P. A.R. Ade, A. Adler, E. Allys, K. Arnold, D. Auguste, J. Aumont, R. Aurlien, J. Austermann, C. Baccigalupi, A. J. Banday, R. Banjeri, R. B. Barreiro, S. Basak, J. Beall, D. Beck, S. Beckman, J. Bermejo, P. De Bernardis, M. BersanelliJ. Bonis, J. Borrill, F. Boulanger, S. Bounissou, M. Brilenkov, M. Brown, M. Bucher, E. Calabrese, P. Campeti, A. Carones, F. J. Casas, A. Challinor, V. Chan, K. Cheung, Y. Chinone, J. F. Cliche, L. Colombo, F. Columbro, J. Cubas, A. Cukierman, D. Curtis, G. D'alessandro, N. Dachlythra, M. De Petris, C. Dickinson, P. Diego-Palazuelos, M. Dobbs, T. Dotani, L. Duband, S. Duff, J. M. Duval, K. Ebisawa, T. Elleflot, H. K. Eriksen, J. Errard, T. Essinger-Hileman, F. Finelli, R. Flauger, C. Franceschet, U. Fuskeland, M. Galloway, K. Ganga, J. R. Gao, R. Genova-Santos, M. Gerbino, M. Gervasi, T. Ghigna, E. Gjerløw, M. L. Gradziel, J. Grain, F. Grupp, A. Gruppuso, J. E. Gudmundsson, T. De Haan, N. W. Halverson, P. Hargrave, T. Hasebe, M. Hasegawa, M. Hattori, S. Henrot-Versillé, D. Herman, D. Herranz, C. A. Hill, G. Hilton, Y. Hirota, E. Hivon, R. A. Hlozek, Y. Hoshino, E. De La Hoz, J. Hubmayr, K. Ichiki, T. Iida, H. Imada, K. Ishimura, H. Ishino, G. Jaehnig, T. Kaga, S. Kashima, N. Katayama, A. Kato, T. Kawasaki, R. Keskitalo, T. Kisner, Y. Kobayashi, N. Kogiso, A. Kogut, K. Kohri, E. Komatsu, K. Komatsu, K. Konishi, N. Krachmalnicoff, I. Kreykenbohm, C. L. Kuo, A. Kushino, L. Lamagna, J. V. Lanen, M. Lattanzi, A. T. Lee, C. Leloup, F. Levrier, E. Linder, T. Louis, G. Luzzi, T. Maciaszek, B. Maffei, D. Maino, M. Maki, S. Mandelli, E. Martinez-Gonzalez, S. Masi, T. Matsumura, A. Mennella, M. Migliaccio, Y. Minami, K. Mitsuda, J. Montgomery, L. Montier, G. Morgante, B. Mot, Y. Murata, J. A. Murphy, M. Nagai, Y. Nagano, T. Nagasaki, R. Nagata, S. Nakamura, T. Namikawa, P. Natoli, S. Nerval, T. Nishibori, H. Nishino, F. Noviello, C. O'sullivan, H. Ogawa, H. Ogawa, S. Oguri, H. Ohsaki, I. S. Ohta, N. Okada, N. Okada, L. Pagano, A. Paiella, D. Paoletti, G. Patanchon, J. Peloton, F. Piacentini, G. Pisano, G. Polenta, D. Poletti, T. Prouvé, G. Puglisi, D. Rambaud, C. Raum, S. Realini, M. Reinecke, M. Remazeilles, A. Ritacco, G. Roudil, J. A. Rubino-Martin, M. Russell, H. Sakurai, Y. Sakurai, M. Sandri, M. Sasaki, G. Savini, D. Scott, J. Seibert, Y. Sekimoto, B. Sherwin, K. Shinozaki, M. Shiraishi, P. Shirron, G. Signorelli, G. Smecher, S. Stever, R. Stompor, H. Sugai, S. Sugiyama, A. Suzuki, J. Suzuki, T. L. Svalheim, E. Switzer, R. Takaku, H. Takakura, S. Takakura, Y. Takase, Y. Takeda, A. Tartari, E. Taylor, Y. Terao, H. Thommesen, K. L. Thompson, B. Thorne, T. Toda, M. Tomasi, M. Tominaga, N. Trappe, M. Tristram, M. Tsuji, M. Tsujimoto, C. Tucker, J. Ullom, G. Vermeulen, P. Vielva, F. Villa, M. Vissers, N. Vittorio, I. Wehus, J. Weller, B. Westbrook, J. Wilms, B. Winter, E. J. Wollack, N. Y. Yamasaki, T. Yoshida, J. Yumoto, M. Zannoni, A. Zonca

^*Corresponding author for this work

Faculty of Physical Sciences

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

Abstract

LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. JAXA selected LiteBIRD in May 2019 as a strategic large-class (L-class) mission, with its expected launch in the late 2020s using JAXA's H3 rocket. LiteBIRD plans to map the cosmic microwave background (CMB) polarization over the full sky with unprecedented precision. Its main scientific objective is to carry out a definitive search for the signal from cosmic inflation, either making a discovery or ruling out well-motivated inflationary models. The measurements of LiteBIRD will also provide us with an insight into the quantum nature of gravity and other new physics beyond the standard models of particle physics and cosmology. To this end, LiteBIRD will perform full-sky surveys for three years at the Sun-Earth Lagrangian point L2 for 15 frequency bands between 34 and 448 GHz with three telescopes, to achieve a total sensitivity of 2.16 μK-arcmin with a typical angular resolution of 0.5° at 100 GHz. We provide an overview of the LiteBIRD project, including scientific objectives, mission requirements, top-level system requirements, operation concept, and expected scientific outcomes.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2020
Subtitle of host publication	Optical, Infrared, and Millimeter Wave
Editors	Makenzie Lystrup, Marshall D. Perrin
Publisher	SPIE
ISBN (Electronic)	9781510636736
DOIs	https://doi.org/10.1117/12.2563050
Publication status	Published - 2020
Event	Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave - Virtual, Online, United States Duration: 14 Dec 2020 → 22 Dec 2020

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	11443
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave
Country/Territory	United States
City	Virtual, Online
Period	14/12/20 → 22/12/20

Bibliographical note

Funding Information:
This work is supported in Japan by ISAS/JAXA for Pre-Phase A2 studies, by the acceleration program of JAXA research and development directorate, by the World Premier International Research Center Initiative (WPI) of MEXT, by the JSPS Core-to-Core Program of A. Advanced Research Networks, and by JSPS KAKENHI Grant Numbers JP15H05891, JP17H01115, and JP17H01125. The Italian LiteBIRD phase A contribution is supported by the Italian Space Agency (ASI Grants No. 2020-9-HH.0 and 2016-24-H.1-2018), the National Institute for Nuclear Physics (INFN) and the National Institute for Astrophysics (INAF). The French LiteBIRD phase A contribution is supported by the Centre National d’Etudes Spatiale (CNES), by the Centre National de la Recherche Scientifique (CNRS), and by the Commissariat à l’Energie Atomique (CEA). The Canadian contribution is supported by the Canadian Space Agency. The US contribution is supported by NASA grant no. 80NSSC18K0132. Norwegian participation in LiteBIRD is supported by the Research Council of Norway (Grant No. 263011). The Spanish LiteBIRD phase A contribution is supported by the Spanish Agencia Estatal de Investigación (AEI), project refs. PID2019-110610RB-C21 and AYA2017-84185-P. Funds that support the Swedish contributions come from the Swedish National Space Agency (SNSA/Rymdstyrelsen) and the Swedish Research Council (Reg. no. 2019-03959). The German participation in LiteBIRD is supported in part by the Excellence Cluster ORIGINS, which is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy (Grant No. EXC-2094 - 390783311). This research used resources of the Central Computing System owned and operated by the Computing Research Center at KEK, as well as resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy.

Publisher Copyright:
© COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.

Other keywords

B-mode polarization
Cosmic in ation
Cosmic microwave background
LiteBIRD
Primordial gravi- tational waves
Quantum gravity
Space telescope

Access to Document

10.1117/12.2563050

Cite this

Hazumi, M., Ade, P. A. R., Adler, A., Allys, E., Arnold, K., Auguste, D., Aumont, J., Aurlien, R., Austermann, J., Baccigalupi, C., Banday, A. J., Banjeri, R., Barreiro, R. B., Basak, S., Beall, J., Beck, D., Beckman, S., Bermejo, J., De Bernardis, P., ... Zonca, A. (2020). LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization. In M. Lystrup, & M. D. Perrin (Eds.), Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave [114432F] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11443). SPIE. https://doi.org/10.1117/12.2563050

Hazumi, M. ; Ade, P. A.R. ; Adler, A. et al. / LiteBIRD satellite : JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization. Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave. editor / Makenzie Lystrup ; Marshall D. Perrin. SPIE, 2020. (Proceedings of SPIE - The International Society for Optical Engineering).

@inproceedings{539bad45d494416388b049fc287238bf,

title = "LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization",

abstract = "LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. JAXA selected LiteBIRD in May 2019 as a strategic large-class (L-class) mission, with its expected launch in the late 2020s using JAXA's H3 rocket. LiteBIRD plans to map the cosmic microwave background (CMB) polarization over the full sky with unprecedented precision. Its main scientific objective is to carry out a definitive search for the signal from cosmic inflation, either making a discovery or ruling out well-motivated inflationary models. The measurements of LiteBIRD will also provide us with an insight into the quantum nature of gravity and other new physics beyond the standard models of particle physics and cosmology. To this end, LiteBIRD will perform full-sky surveys for three years at the Sun-Earth Lagrangian point L2 for 15 frequency bands between 34 and 448 GHz with three telescopes, to achieve a total sensitivity of 2.16 μK-arcmin with a typical angular resolution of 0.5° at 100 GHz. We provide an overview of the LiteBIRD project, including scientific objectives, mission requirements, top-level system requirements, operation concept, and expected scientific outcomes.",

keywords = "B-mode polarization, Cosmic in ation, Cosmic microwave background, LiteBIRD, Primordial gravi- tational waves, Quantum gravity, Space telescope",

author = "M. Hazumi and Ade, {P. A.R.} and A. Adler and E. Allys and K. Arnold and D. Auguste and J. Aumont and R. Aurlien and J. Austermann and C. Baccigalupi and Banday, {A. J.} and R. Banjeri and Barreiro, {R. B.} and S. Basak and J. Beall and D. Beck and S. Beckman and J. Bermejo and {De Bernardis}, P. and M. Bersanelli and J. Bonis and J. Borrill and F. Boulanger and S. Bounissou and M. Brilenkov and M. Brown and M. Bucher and E. Calabrese and P. Campeti and A. Carones and Casas, {F. J.} and A. Challinor and V. Chan and K. Cheung and Y. Chinone and Cliche, {J. F.} and L. Colombo and F. Columbro and J. Cubas and A. Cukierman and D. Curtis and G. D'alessandro and N. Dachlythra and {De Petris}, M. and C. Dickinson and P. Diego-Palazuelos and M. Dobbs and T. Dotani and L. Duband and S. Duff and Duval, {J. M.} and K. Ebisawa and T. Elleflot and Eriksen, {H. K.} and J. Errard and T. Essinger-Hileman and F. Finelli and R. Flauger and C. Franceschet and U. Fuskeland and M. Galloway and K. Ganga and Gao, {J. R.} and R. Genova-Santos and M. Gerbino and M. Gervasi and T. Ghigna and E. Gjerl{\o}w and Gradziel, {M. L.} and J. Grain and F. Grupp and A. Gruppuso and Gudmundsson, {J. E.} and {De Haan}, T. and Halverson, {N. W.} and P. Hargrave and T. Hasebe and M. Hasegawa and M. Hattori and S. Henrot-Versill{\'e} and D. Herman and D. Herranz and Hill, {C. A.} and G. Hilton and Y. Hirota and E. Hivon and Hlozek, {R. A.} and Y. Hoshino and {De La Hoz}, E. and J. Hubmayr and K. Ichiki and T. Iida and H. Imada and K. Ishimura and H. Ishino and G. Jaehnig and T. Kaga and S. Kashima and N. Katayama and A. Kato and T. Kawasaki and R. Keskitalo and T. Kisner and Y. Kobayashi and N. Kogiso and A. Kogut and K. Kohri and E. Komatsu and K. Komatsu and K. Konishi and N. Krachmalnicoff and I. Kreykenbohm and Kuo, {C. L.} and A. Kushino and L. Lamagna and Lanen, {J. V.} and M. Lattanzi and Lee, {A. T.} and C. Leloup and F. Levrier and E. Linder and T. Louis and G. Luzzi and T. Maciaszek and B. Maffei and D. Maino and M. Maki and S. Mandelli and E. Martinez-Gonzalez and S. Masi and T. Matsumura and A. Mennella and M. Migliaccio and Y. Minami and K. Mitsuda and J. Montgomery and L. Montier and G. Morgante and B. Mot and Y. Murata and Murphy, {J. A.} and M. Nagai and Y. Nagano and T. Nagasaki and R. Nagata and S. Nakamura and T. Namikawa and P. Natoli and S. Nerval and T. Nishibori and H. Nishino and F. Noviello and C. O'sullivan and H. Ogawa and H. Ogawa and S. Oguri and H. Ohsaki and Ohta, {I. S.} and N. Okada and N. Okada and L. Pagano and A. Paiella and D. Paoletti and G. Patanchon and J. Peloton and F. Piacentini and G. Pisano and G. Polenta and D. Poletti and T. Prouv{\'e} and G. Puglisi and D. Rambaud and C. Raum and S. Realini and M. Reinecke and M. Remazeilles and A. Ritacco and G. Roudil and Rubino-Martin, {J. A.} and M. Russell and H. Sakurai and Y. Sakurai and M. Sandri and M. Sasaki and G. Savini and D. Scott and J. Seibert and Y. Sekimoto and B. Sherwin and K. Shinozaki and M. Shiraishi and P. Shirron and G. Signorelli and G. Smecher and S. Stever and R. Stompor and H. Sugai and S. Sugiyama and A. Suzuki and J. Suzuki and Svalheim, {T. L.} and E. Switzer and R. Takaku and H. Takakura and S. Takakura and Y. Takase and Y. Takeda and A. Tartari and E. Taylor and Y. Terao and H. Thommesen and Thompson, {K. L.} and B. Thorne and T. Toda and M. Tomasi and M. Tominaga and N. Trappe and M. Tristram and M. Tsuji and M. Tsujimoto and C. Tucker and J. Ullom and G. Vermeulen and P. Vielva and F. Villa and M. Vissers and N. Vittorio and I. Wehus and J. Weller and B. Westbrook and J. Wilms and B. Winter and Wollack, {E. J.} and Yamasaki, {N. Y.} and T. Yoshida and J. Yumoto and M. Zannoni and A. Zonca",

note = "Funding Information: This work is supported in Japan by ISAS/JAXA for Pre-Phase A2 studies, by the acceleration program of JAXA research and development directorate, by the World Premier International Research Center Initiative (WPI) of MEXT, by the JSPS Core-to-Core Program of A. Advanced Research Networks, and by JSPS KAKENHI Grant Numbers JP15H05891, JP17H01115, and JP17H01125. The Italian LiteBIRD phase A contribution is supported by the Italian Space Agency (ASI Grants No. 2020-9-HH.0 and 2016-24-H.1-2018), the National Institute for Nuclear Physics (INFN) and the National Institute for Astrophysics (INAF). The French LiteBIRD phase A contribution is supported by the Centre National d{\textquoteright}Etudes Spatiale (CNES), by the Centre National de la Recherche Scientifique (CNRS), and by the Commissariat {\`a} l{\textquoteright}Energie Atomique (CEA). The Canadian contribution is supported by the Canadian Space Agency. The US contribution is supported by NASA grant no. 80NSSC18K0132. Norwegian participation in LiteBIRD is supported by the Research Council of Norway (Grant No. 263011). The Spanish LiteBIRD phase A contribution is supported by the Spanish Agencia Estatal de Investigaci{\'o}n (AEI), project refs. PID2019-110610RB-C21 and AYA2017-84185-P. Funds that support the Swedish contributions come from the Swedish National Space Agency (SNSA/Rymdstyrelsen) and the Swedish Research Council (Reg. no. 2019-03959). The German participation in LiteBIRD is supported in part by the Excellence Cluster ORIGINS, which is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany{\textquoteright}s Excellence Strategy (Grant No. EXC-2094 - 390783311). This research used resources of the Central Computing System owned and operated by the Computing Research Center at KEK, as well as resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy. Publisher Copyright: {\textcopyright} COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.; Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave ; Conference date: 14-12-2020 Through 22-12-2020",

year = "2020",

doi = "10.1117/12.2563050",

language = "English",

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

publisher = "SPIE",

editor = "Makenzie Lystrup and Perrin, {Marshall D.}",

booktitle = "Space Telescopes and Instrumentation 2020",

address = "United States",

}

Hazumi, M, Ade, PAR, Adler, A, Allys, E, Arnold, K, Auguste, D, Aumont, J, Aurlien, R, Austermann, J, Baccigalupi, C, Banday, AJ, Banjeri, R, Barreiro, RB, Basak, S, Beall, J, Beck, D, Beckman, S, Bermejo, J, De Bernardis, P, Bersanelli, M, Bonis, J, Borrill, J, Boulanger, F, Bounissou, S, Brilenkov, M, Brown, M, Bucher, M, Calabrese, E, Campeti, P, Carones, A, Casas, FJ, Challinor, A, Chan, V, Cheung, K, Chinone, Y, Cliche, JF, Colombo, L, Columbro, F, Cubas, J, Cukierman, A, Curtis, D, D'alessandro, G, Dachlythra, N, De Petris, M, Dickinson, C, Diego-Palazuelos, P, Dobbs, M, Dotani, T, Duband, L, Duff, S, Duval, JM, Ebisawa, K, Elleflot, T, Eriksen, HK, Errard, J, Essinger-Hileman, T, Finelli, F, Flauger, R, Franceschet, C, Fuskeland, U, Galloway, M, Ganga, K, Gao, JR, Genova-Santos, R, Gerbino, M, Gervasi, M, Ghigna, T, Gjerløw, E, Gradziel, ML, Grain, J, Grupp, F, Gruppuso, A, Gudmundsson, JE, De Haan, T, Halverson, NW, Hargrave, P, Hasebe, T, Hasegawa, M, Hattori, M, Henrot-Versillé, S, Herman, D, Herranz, D, Hill, CA, Hilton, G, Hirota, Y, Hivon, E, Hlozek, RA, Hoshino, Y, De La Hoz, E, Hubmayr, J, Ichiki, K, Iida, T, Imada, H, Ishimura, K, Ishino, H, Jaehnig, G, Kaga, T, Kashima, S, Katayama, N, Kato, A, Kawasaki, T, Keskitalo, R, Kisner, T, Kobayashi, Y, Kogiso, N, Kogut, A, Kohri, K, Komatsu, E, Komatsu, K, Konishi, K, Krachmalnicoff, N, Kreykenbohm, I, Kuo, CL, Kushino, A, Lamagna, L, Lanen, JV, Lattanzi, M, Lee, AT, Leloup, C, Levrier, F, Linder, E, Louis, T, Luzzi, G, Maciaszek, T, Maffei, B, Maino, D, Maki, M, Mandelli, S, Martinez-Gonzalez, E, Masi, S, Matsumura, T, Mennella, A, Migliaccio, M, Minami, Y, Mitsuda, K, Montgomery, J, Montier, L, Morgante, G, Mot, B, Murata, Y, Murphy, JA, Nagai, M, Nagano, Y, Nagasaki, T, Nagata, R, Nakamura, S, Namikawa, T, Natoli, P, Nerval, S, Nishibori, T, Nishino, H, Noviello, F, O'sullivan, C, Ogawa, H, Ogawa, H, Oguri, S, Ohsaki, H, Ohta, IS, Okada, N, Okada, N, Pagano, L, Paiella, A, Paoletti, D, Patanchon, G, Peloton, J, Piacentini, F, Pisano, G, Polenta, G, Poletti, D, Prouvé, T, Puglisi, G, Rambaud, D, Raum, C, Realini, S, Reinecke, M, Remazeilles, M, Ritacco, A, Roudil, G, Rubino-Martin, JA, Russell, M, Sakurai, H, Sakurai, Y, Sandri, M, Sasaki, M, Savini, G, Scott, D, Seibert, J, Sekimoto, Y, Sherwin, B, Shinozaki, K, Shiraishi, M, Shirron, P, Signorelli, G, Smecher, G, Stever, S, Stompor, R, Sugai, H, Sugiyama, S, Suzuki, A, Suzuki, J, Svalheim, TL, Switzer, E, Takaku, R, Takakura, H, Takakura, S, Takase, Y, Takeda, Y, Tartari, A, Taylor, E, Terao, Y, Thommesen, H, Thompson, KL, Thorne, B, Toda, T, Tomasi, M, Tominaga, M, Trappe, N, Tristram, M, Tsuji, M, Tsujimoto, M, Tucker, C, Ullom, J, Vermeulen, G, Vielva, P, Villa, F, Vissers, M, Vittorio, N, Wehus, I, Weller, J, Westbrook, B, Wilms, J, Winter, B, Wollack, EJ, Yamasaki, NY, Yoshida, T, Yumoto, J, Zannoni, M & Zonca, A 2020, LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization. in M Lystrup & MD Perrin (eds), Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave., 114432F, Proceedings of SPIE - The International Society for Optical Engineering, vol. 11443, SPIE, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave, Virtual, Online, United States, 14/12/20. https://doi.org/10.1117/12.2563050

LiteBIRD satellite : JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization. / Hazumi, M.; Ade, P. A.R.; Adler, A. et al.

Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave. ed. / Makenzie Lystrup; Marshall D. Perrin. SPIE, 2020. 114432F (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 11443).

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

TY - GEN

T1 - LiteBIRD satellite

T2 - Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave

AU - Hazumi, M.

AU - Ade, P. A.R.

AU - Adler, A.

AU - Allys, E.

AU - Arnold, K.

AU - Auguste, D.

AU - Aumont, J.

AU - Aurlien, R.

AU - Austermann, J.

AU - Baccigalupi, C.

AU - Banday, A. J.

AU - Banjeri, R.

AU - Barreiro, R. B.

AU - Basak, S.

AU - Beall, J.

AU - Beck, D.

AU - Beckman, S.

AU - Bermejo, J.

AU - De Bernardis, P.

AU - Bersanelli, M.

AU - Bonis, J.

AU - Borrill, J.

AU - Boulanger, F.

AU - Bounissou, S.

AU - Brilenkov, M.

AU - Brown, M.

AU - Bucher, M.

AU - Calabrese, E.

AU - Campeti, P.

AU - Carones, A.

AU - Casas, F. J.

AU - Challinor, A.

AU - Chan, V.

AU - Cheung, K.

AU - Chinone, Y.

AU - Cliche, J. F.

AU - Colombo, L.

AU - Columbro, F.

AU - Cubas, J.

AU - Cukierman, A.

AU - Curtis, D.

AU - D'alessandro, G.

AU - Dachlythra, N.

AU - De Petris, M.

AU - Dickinson, C.

AU - Diego-Palazuelos, P.

AU - Dobbs, M.

AU - Dotani, T.

AU - Duband, L.

AU - Duff, S.

AU - Duval, J. M.

AU - Ebisawa, K.

AU - Elleflot, T.

AU - Eriksen, H. K.

AU - Errard, J.

AU - Essinger-Hileman, T.

AU - Finelli, F.

AU - Flauger, R.

AU - Franceschet, C.

AU - Fuskeland, U.

AU - Galloway, M.

AU - Ganga, K.

AU - Gao, J. R.

AU - Genova-Santos, R.

AU - Gerbino, M.

AU - Gervasi, M.

AU - Ghigna, T.

AU - Gjerløw, E.

AU - Gradziel, M. L.

AU - Grain, J.

AU - Grupp, F.

AU - Gruppuso, A.

AU - Gudmundsson, J. E.

AU - De Haan, T.

AU - Halverson, N. W.

AU - Hargrave, P.

AU - Hasebe, T.

AU - Hasegawa, M.

AU - Hattori, M.

AU - Henrot-Versillé, S.

AU - Herman, D.

AU - Herranz, D.

AU - Hill, C. A.

AU - Hilton, G.

AU - Hirota, Y.

AU - Hivon, E.

AU - Hlozek, R. A.

AU - Hoshino, Y.

AU - De La Hoz, E.

AU - Hubmayr, J.

AU - Ichiki, K.

AU - Iida, T.

AU - Imada, H.

AU - Ishimura, K.

AU - Ishino, H.

AU - Jaehnig, G.

AU - Kaga, T.

AU - Kashima, S.

AU - Katayama, N.

AU - Kato, A.

AU - Kawasaki, T.

AU - Keskitalo, R.

AU - Kisner, T.

AU - Kobayashi, Y.

AU - Kogiso, N.

AU - Kogut, A.

AU - Kohri, K.

AU - Komatsu, E.

AU - Komatsu, K.

AU - Konishi, K.

AU - Krachmalnicoff, N.

AU - Kreykenbohm, I.

AU - Kuo, C. L.

AU - Kushino, A.

AU - Lamagna, L.

AU - Lanen, J. V.

AU - Lattanzi, M.

AU - Lee, A. T.

AU - Leloup, C.

AU - Levrier, F.

AU - Linder, E.

AU - Louis, T.

AU - Luzzi, G.

AU - Maciaszek, T.

AU - Maffei, B.

AU - Maino, D.

AU - Maki, M.

AU - Mandelli, S.

AU - Martinez-Gonzalez, E.

AU - Masi, S.

AU - Matsumura, T.

AU - Mennella, A.

AU - Migliaccio, M.

AU - Minami, Y.

AU - Mitsuda, K.

AU - Montgomery, J.

AU - Montier, L.

AU - Morgante, G.

AU - Mot, B.

AU - Murata, Y.

AU - Murphy, J. A.

AU - Nagai, M.

AU - Nagano, Y.

AU - Nagasaki, T.

AU - Nagata, R.

AU - Nakamura, S.

AU - Namikawa, T.

AU - Natoli, P.

AU - Nerval, S.

AU - Nishibori, T.

AU - Nishino, H.

AU - Noviello, F.

AU - O'sullivan, C.

AU - Ogawa, H.

AU - Oguri, S.

AU - Ohsaki, H.

AU - Ohta, I. S.

AU - Okada, N.

AU - Pagano, L.

AU - Paiella, A.

AU - Paoletti, D.

AU - Patanchon, G.

AU - Peloton, J.

AU - Piacentini, F.

AU - Pisano, G.

AU - Polenta, G.

AU - Poletti, D.

AU - Prouvé, T.

AU - Puglisi, G.

AU - Rambaud, D.

AU - Raum, C.

AU - Realini, S.

AU - Reinecke, M.

AU - Remazeilles, M.

AU - Ritacco, A.

AU - Roudil, G.

AU - Rubino-Martin, J. A.

AU - Russell, M.

AU - Sakurai, H.

AU - Sakurai, Y.

AU - Sandri, M.

AU - Sasaki, M.

AU - Savini, G.

AU - Scott, D.

AU - Seibert, J.

AU - Sekimoto, Y.

AU - Sherwin, B.

AU - Shinozaki, K.

AU - Shiraishi, M.

AU - Shirron, P.

AU - Signorelli, G.

AU - Smecher, G.

AU - Stever, S.

AU - Stompor, R.

AU - Sugai, H.

AU - Sugiyama, S.

AU - Suzuki, A.

AU - Suzuki, J.

AU - Svalheim, T. L.

AU - Switzer, E.

AU - Takaku, R.

AU - Takakura, H.

AU - Takakura, S.

AU - Takase, Y.

AU - Takeda, Y.

AU - Tartari, A.

AU - Taylor, E.

AU - Terao, Y.

AU - Thommesen, H.

AU - Thompson, K. L.

AU - Thorne, B.

AU - Toda, T.

AU - Tomasi, M.

AU - Tominaga, M.

AU - Trappe, N.

AU - Tristram, M.

AU - Tsuji, M.

AU - Tsujimoto, M.

AU - Tucker, C.

AU - Ullom, J.

AU - Vermeulen, G.

AU - Vielva, P.

AU - Villa, F.

AU - Vissers, M.

AU - Vittorio, N.

AU - Wehus, I.

AU - Weller, J.

AU - Westbrook, B.

AU - Wilms, J.

AU - Winter, B.

AU - Wollack, E. J.

AU - Yamasaki, N. Y.

AU - Yoshida, T.

AU - Yumoto, J.

AU - Zannoni, M.

AU - Zonca, A.

N1 - Funding Information: This work is supported in Japan by ISAS/JAXA for Pre-Phase A2 studies, by the acceleration program of JAXA research and development directorate, by the World Premier International Research Center Initiative (WPI) of MEXT, by the JSPS Core-to-Core Program of A. Advanced Research Networks, and by JSPS KAKENHI Grant Numbers JP15H05891, JP17H01115, and JP17H01125. The Italian LiteBIRD phase A contribution is supported by the Italian Space Agency (ASI Grants No. 2020-9-HH.0 and 2016-24-H.1-2018), the National Institute for Nuclear Physics (INFN) and the National Institute for Astrophysics (INAF). The French LiteBIRD phase A contribution is supported by the Centre National d’Etudes Spatiale (CNES), by the Centre National de la Recherche Scientifique (CNRS), and by the Commissariat à l’Energie Atomique (CEA). The Canadian contribution is supported by the Canadian Space Agency. The US contribution is supported by NASA grant no. 80NSSC18K0132. Norwegian participation in LiteBIRD is supported by the Research Council of Norway (Grant No. 263011). The Spanish LiteBIRD phase A contribution is supported by the Spanish Agencia Estatal de Investigación (AEI), project refs. PID2019-110610RB-C21 and AYA2017-84185-P. Funds that support the Swedish contributions come from the Swedish National Space Agency (SNSA/Rymdstyrelsen) and the Swedish Research Council (Reg. no. 2019-03959). The German participation in LiteBIRD is supported in part by the Excellence Cluster ORIGINS, which is funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy (Grant No. EXC-2094 - 390783311). This research used resources of the Central Computing System owned and operated by the Computing Research Center at KEK, as well as resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy. Publisher Copyright: © COPYRIGHT SPIE. Downloading of the abstract is permitted for personal use only.

PY - 2020

Y1 - 2020

N2 - LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. JAXA selected LiteBIRD in May 2019 as a strategic large-class (L-class) mission, with its expected launch in the late 2020s using JAXA's H3 rocket. LiteBIRD plans to map the cosmic microwave background (CMB) polarization over the full sky with unprecedented precision. Its main scientific objective is to carry out a definitive search for the signal from cosmic inflation, either making a discovery or ruling out well-motivated inflationary models. The measurements of LiteBIRD will also provide us with an insight into the quantum nature of gravity and other new physics beyond the standard models of particle physics and cosmology. To this end, LiteBIRD will perform full-sky surveys for three years at the Sun-Earth Lagrangian point L2 for 15 frequency bands between 34 and 448 GHz with three telescopes, to achieve a total sensitivity of 2.16 μK-arcmin with a typical angular resolution of 0.5° at 100 GHz. We provide an overview of the LiteBIRD project, including scientific objectives, mission requirements, top-level system requirements, operation concept, and expected scientific outcomes.

AB - LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. JAXA selected LiteBIRD in May 2019 as a strategic large-class (L-class) mission, with its expected launch in the late 2020s using JAXA's H3 rocket. LiteBIRD plans to map the cosmic microwave background (CMB) polarization over the full sky with unprecedented precision. Its main scientific objective is to carry out a definitive search for the signal from cosmic inflation, either making a discovery or ruling out well-motivated inflationary models. The measurements of LiteBIRD will also provide us with an insight into the quantum nature of gravity and other new physics beyond the standard models of particle physics and cosmology. To this end, LiteBIRD will perform full-sky surveys for three years at the Sun-Earth Lagrangian point L2 for 15 frequency bands between 34 and 448 GHz with three telescopes, to achieve a total sensitivity of 2.16 μK-arcmin with a typical angular resolution of 0.5° at 100 GHz. We provide an overview of the LiteBIRD project, including scientific objectives, mission requirements, top-level system requirements, operation concept, and expected scientific outcomes.

KW - B-mode polarization

KW - Cosmic in ation

KW - Cosmic microwave background

KW - LiteBIRD

KW - Primordial gravi- tational waves

KW - Quantum gravity

KW - Space telescope

UR - http://www.scopus.com/inward/record.url?scp=85099878190&partnerID=8YFLogxK

U2 - 10.1117/12.2563050

DO - 10.1117/12.2563050

M3 - Conference contribution

AN - SCOPUS:85099878190

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

BT - Space Telescopes and Instrumentation 2020

A2 - Lystrup, Makenzie

A2 - Perrin, Marshall D.

PB - SPIE

Y2 - 14 December 2020 through 22 December 2020

ER -

Hazumi M, Ade PAR, Adler A, Allys E, Arnold K, Auguste D et al. LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization. In Lystrup M, Perrin MD, editors, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave. SPIE. 2020. 114432F. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2563050

LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization

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