LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB
The LiteBIRD Collaboration: A.I. Lonappan et al.
| Autores: | , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/374199 |
| Acceso en línea: | http://hdl.handle.net/10261/374199 |
| Access Level: | acceso abierto |
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LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB |
| title |
LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB |
| spellingShingle |
LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB Lonappan, Anto I. |
| title_short |
LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB |
| title_full |
LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB |
| title_fullStr |
LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB |
| title_full_unstemmed |
LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB |
| title_sort |
LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB |
| dc.creator.none.fl_str_mv |
Lonappan, Anto I. Diego-Palazuelos, P. Ruiz Granda, Miguel Martínez-González, Enrique Vielva, Patricio Barreiro, R. Belén Casas-Reinares, F. J. Gimeno-Amo, C. Pascual Cisneros, Guillermo LiteBIRD Collaboration |
| author |
Lonappan, Anto I. |
| author_facet |
Lonappan, Anto I. Diego-Palazuelos, P. Ruiz Granda, Miguel Martínez-González, Enrique Vielva, Patricio Barreiro, R. Belén Casas-Reinares, F. J. Gimeno-Amo, C. Pascual Cisneros, Guillermo LiteBIRD Collaboration |
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author |
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Diego-Palazuelos, P. Ruiz Granda, Miguel Martínez-González, Enrique Vielva, Patricio Barreiro, R. Belén Casas-Reinares, F. J. Gimeno-Amo, C. Pascual Cisneros, Guillermo LiteBIRD Collaboration |
| author2_role |
author author author author author author author author author |
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Japan Society for the Promotion of Science Ministry of Education, Culture, Sports, Science and Technology (Japan) Canadian Space Agency Centre National de la Recherche Scientifique (France) Centre National D'Etudes Spatiales (France) German Research Foundation Agenzia Spaziale Italiana Istituto Nazionale di Astrofisica Istituto Nazionale di Fisica Nucleare European Commission Research Council of Norway European Research Council Agencia Estatal de Investigación (España) Ministerio de Ciencia, Innovación y Universidades (España) National Science Foundation (US) NASA Swedish National Space Agency Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72] |
| description |
The LiteBIRD Collaboration: A.I. Lonappan et al. |
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2024 |
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2024 2024 2024 |
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info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
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article |
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http://hdl.handle.net/10261/374199 |
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http://hdl.handle.net/10261/374199 |
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IOP Publishing |
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LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMBLonappan, Anto I.Diego-Palazuelos, P.Ruiz Granda, MiguelMartínez-González, EnriqueVielva, PatricioBarreiro, R. BelénCasas-Reinares, F. J.Gimeno-Amo, C.Pascual Cisneros, GuillermoLiteBIRD CollaborationThe LiteBIRD Collaboration: A.I. Lonappan et al.We explore the capability of measuring lensing signals in LiteBIRD full-sky polarization maps. With a 30 arcmin beam width and an impressively low polarization noise of 2.16 μK-arcmin,LiteBIRD will be able to measure the full-sky polarization of the cosmic microwave background (CMB) very precisely. This unique sensitivity also enables the reconstruction of a nearly full-sky lensing map using only polarization data, even considering its limited capability to capture small-scale CMB anisotropies. In this paper, we investigate the ability to construct a full-sky lensing measurement in the presence of Galactic foregrounds, finding that several possible biases from Galactic foregrounds should be negligible after component separation by harmonic-space internal linear combination. We find that the signal-to-noise ratio of the lensing is approximately 40 using only polarization data measured over 80% of the sky. This achievement is comparable to Planck's recent lensing measurement with both temperature and polarization and represents a four-fold improvement over Planck's polarization-only lensing measurement. The LiteBIRD lensing map will complement the Planck lensing map and provide several opportunities for cross-correlation science, especially in the northern hemisphere.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 Canadian contribution is supported by the Canadian Space Agency. 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 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). 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). Norwegian participation in LiteBIRD is supported by the Research Council of Norway (Grant No. 263011) and has received funding from the European Research Council (ERC) under the Horizon 2020 Research and Innovation Programme (Grant agreement No. 772253 and 819478). The Spanish LiteBIRD phase A contribution is supported by the Spanish Agencia Estatal de Investigación (AEI), project refs. PID2019-110610RB-C21, PID2020-120514GB-I00, ProID2020010108 and ICTP20210008. Funds that support contributions from Sweden come from the Swedish National Space Agency (SNSA/Rymdstyrelsen) and the Swedish Research Council (Reg. no. 2019-03959). The US contribution is supported by NASAgrant no. 80NSSC18K0132. We also acknowledge the support from H2020-MSCA-RISE2020 European grant (Marie Sklodowska-Curie Research and Innovation Staff Exchange), JSPS KAKENHI Grant No. JP20H05859 and No. JP22K03682. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility located at Lawrence Berkeley National Laboratory.Peer reviewedIOP PublishingJapan Society for the Promotion of ScienceMinistry of Education, Culture, Sports, Science and Technology (Japan)Canadian Space AgencyCentre National de la Recherche Scientifique (France)Centre National D'Etudes Spatiales (France)German Research FoundationAgenzia Spaziale ItalianaIstituto Nazionale di AstrofisicaIstituto Nazionale di Fisica NucleareEuropean CommissionResearch Council of NorwayEuropean Research CouncilAgencia Estatal de Investigación (España)Ministerio de Ciencia, Innovación y Universidades (España)National Science Foundation (US)NASASwedish National Space AgencyConsejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202420242024info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/374199reponame:DIGITAL.CSIC. 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