LiteBIRD satelliteCitation formats

  • Authors:
  • LiteBIRD collaboration

Standard

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

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 proceedingConference contributionpeer-review

Harvard

LiteBIRD collaboration 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

APA

LiteBIRD collaboration (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

Vancouver

LiteBIRD collaboration. 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). https://doi.org/10.1117/12.2563050

Author

LiteBIRD collaboration. / 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).

Bibtex

@inproceedings{8723a4147be84e6cbf6e6dae022c708f,
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 = "{LiteBIRD collaboration} and 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 V. Chan and K. Cheung and D. Curtis and C. Dickinson and M. Dobbs and S. Duff and Gao, {J. R.} and D. Herman and Hill, {C. A.} and Kuo, {C. L.} and Lee, {A. T.} and B. Maffei and T. Matsumura and J. Montgomery and Murphy, {J. A.} and F. Noviello and G. Pisano and M. Remazeilles and M. Russell and D. Scott and A. Suzuki and E. Taylor and Thompson, {K. L.} and C. Tucker",
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. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.; Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave ; Conference date: 14-12-2020 Through 22-12-2020",
year = "2020",
month = dec,
day = "15",
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",

}

RIS

TY - GEN

T1 - LiteBIRD satellite

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

AU - LiteBIRD collaboration

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 - Chan, V.

AU - Cheung, K.

AU - Curtis, D.

AU - Dickinson, C.

AU - Dobbs, M.

AU - Duff, S.

AU - Gao, J. R.

AU - Herman, D.

AU - Hill, C. A.

AU - Kuo, C. L.

AU - Lee, A. T.

AU - Maffei, B.

AU - Matsumura, T.

AU - Montgomery, J.

AU - Murphy, J. A.

AU - Noviello, F.

AU - Pisano, G.

AU - Remazeilles, M.

AU - Russell, M.

AU - Scott, D.

AU - Suzuki, A.

AU - Taylor, E.

AU - Thompson, K. L.

AU - Tucker, C.

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. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.

PY - 2020/12/15

Y1 - 2020/12/15

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 -