Accès ouvert déclaré
2025
article
A simulation framework for the LiteBIRD instruments
M Tomasi, L. Pagano, C Baccigalupi, A. J. Banday, M. Bortolami, G. Galloni, M. Galloway, T. Ghigna, S. Giardiello, E. Hivon, N Krachmalnicoff, S. Micheli, Y. Nagano, G. Patanchon, D. Poletti, Giuseppe Puglisi, N. Raffuzzi, M. Reinecke, Yusuke Takase, G. Weymann-Despres, Debabrata Adak, Erwan Allys, J. Aumont, R. Aurvik, M. Ballardini, R. B. Barreiro, N. Bartolo, S. Basak, M. Bersanelli, A Besnard, T Brinckmann, Erminia Calabrese, P. Campeti, E. Carinos, A. Carones, F. J. Casas, Kmc Cheung, M Citran, Lionel Clermont, F Columbro, Gabriele Coppi, A Coppolecchia, F. Cuttaia, Bo Peng, P de Bernardis, E. de la Hoz, Mario de Lucia, S Della Torre, P. Diego-Palazuelos, H. K. Eriksen, Thomas Essinger-Hileman, C Franceschet, U Fuskeland, M. Gerbino, M. Gervasi, C. Gimeno-Amo, E. Gjerløw, A. Gruppuso, M. Hazumi, S Henrot-Versillé, L. T. Hergt, Baptiste Jost, Kimiko KOHRI, L. Lamagna, T. Lari, M. Lattanzi, C. Leloup, F. Levrier, A.I. Lonappan, M. López-Caniego, G. Luzzi, J. F. Macías–Pérez, B. Maffei, E. Martínez-González, S. Masi, S. Matarrese, T. Matsumura, L. Montier, G. Morgante, L. Mousset, Ryo Nagata, F. Noviello, Ippei Obata, Antonio Occhiuzzi, A Paiella, D. Paoletti, G Pascual-Cisneros, F Piacentini, Michele Pinchera, G Polenta, L. Porcelli, M Remazeilles, A. Ritacco, A. Rizzieri, J. A. Rubiño-Martín, M. Ruiz-Granda, J. Sanghavi, V. Sauvage, Maresuke Shiraishi, G. Signorelli, S. L. Stever, R. M. Sullivan, Konstantinos Tassis, L. Terenzi, L. Vacher, B. Van Tent, P. Vielva, I. K. Wehus, M. Zannoni, Yanqiu Zhou
0Citations signalées, ce qui n’est pas une note de qualité
81Institutions déclarées
13Pays d’affiliation déclarés
Rattachement africain : it, fr, no, jp, gb, de, es, in, us, be, ca, nl, gr.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
Abstract LiteBIRD , the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission focused on primordial cosmology and fundamental physics. In this paper, we present the LiteBIRD Simulation Framework (LBS), a Python package designed for the implementation of pipelines that model the outputs of the data acquisition process from the three instruments on the LiteBIRD spacecraft: LFT (Low-Frequency Telescope), MFT (Mid-Frequency Telescope), and HFT (High-Frequency Telescope). LBS provides several modules to simulate the scanning strategy of the telescopes, the measurement of realistic polarized radiation coming from the sky (including the Cosmic Microwave Background itself, the Solar and Kinematic dipole, and the diffuse foregrounds emitted by the Galaxy), the generation of instrumental noise and the effect of systematic errors, like pointing wobbling, non-idealities in the Half-Wave Plate, et cetera . Additionally, we present the implementation of a simple but complete pipeline that showcases the main features of LBS. We also discuss how we ensured that LBS lets people develop pipelines whose results are accurate and reproducible. A full end-to-end pipeline has been developed using LBS to characterize the scientific performance of the LiteBIRD experiment. This pipeline and the results of the first simulation run are presented in Puglisi et al. (2025).
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé, mais le titre doit être comparé manuellement.
- Titre Crossref
- A simulation framework for the
<i>LiteBIRD</i>
instruments
- Date Crossref
- 01/11/2025
- Éditeur
- IOP Publishing
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.
Les institutions déclarées
University of MilanIstituto Nazionale di Fisica Nucleare, Sezione di MilanoCentre National de la Recherche ScientifiqueUniversity of FerraraUniversité Paris-SaclayInstitut d'Astrophysique SpatialeIstituto Nazionale di Fisica Nucleare, Sezione di FerraraUniversity of Rome Tor VergataScuola Internazionale Superiore di Studi AvanzatiUniversity of TriesteIstituto Nazionale di Fisica Nucleare, Sezione di TriesteInstitute for Fundamental Physics of the UniverseUniversité Toulouse III - Paul SabatierUniversité Fédérale de Toulouse Midi-PyrénéesInstitut de Recherche en Astrophysique et PlanétologieUniversity of OsloHigh Energy Accelerator Research OrganizationKavli Institute for the Physics and Mathematics of the UniverseInternational Center for Quantum-field Measurement Systems for Studies of the Universe and ParticlesThe University of TokyoCardiff UniversityUniversity of WalesInstitut d'Astrophysique de ParisSorbonne UniversitéSapienza University of RomeOkayama UniversityUniversité Paris CitéKaichi International UniversityTokyo International UniversityIstituto Nazionale di Fisica Nucleare, Sezione di Milano BicoccaUniversity of Milano-BicoccaUniversity of CataniaIstituto Nazionale di Fisica Nucleare, Sezione di CataniaOsservatorio Astrofisico di CataniaMax Planck Institute for AstrophysicsUniversity of OxfordInstitut National de Physique Nucléaire et de Physique des ParticulesLaboratoire de Physique des 2 Infinis Irène Joliot-CurieInstituto de Astrofísica de CanariasUniversité Paris Sciences et LettresÉcole Normale Supérieure - PSLLaboratoire de Physique de l'Ecole Normale SupérieureBologna Research AreaNational Institute for AstrophysicsInstituto de Física de CantabriaUniversity of PaduaIstituto Nazionale di Fisica Nucleare, Sezione di PadovaOsservatorio Astronomico di PadovaIndian Institute of Science Education and Research ThiruvananthapuramExcellence Cluster OriginsLawrence Berkeley National LaboratoryUniversity of ManchesterUniversity of California, BerkeleyUniversity of LiègeIstituto Nazionale di Fisica Nucleare, Sezione di Roma IIstituto Nazionale di Fisica Nucleare, Sezione di PisaInternational Computer Science InstituteGoddard Space Flight CenterIstituto Nazionale di Fisica Nucleare, Sezione di BolognaThe Graduate University for Advanced Studies, SOKENDAIJapan Aerospace Exploration AgencyInstitute of Space and Astronautical ScienceUniversity of British ColumbiaUniversity of San DiegoUniversity of California San DiegoEuropean Space Astronomy CentreUniversidad Europea de MadridAgenzia Spaziale ItalianaLaboratoire de Physique Subatomique et de CosmologieUniversité Grenoble AlpesGran Sasso Science InstituteIstituto Nazionale di Fisica NucleareIstituto Nazionale di Fisica Nucleare, Laboratori Nazionali di FrascatiUniversidad de La LagunaUniversidad de CantabriaDelta Institute for Theoretical PhysicsLudwig-Maximilians-Universität MünchenSuwa Red Cross HospitalUniversity of PisaUniversity of CreteFoundation for Research and Technology Hellas
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Simulation Techniques and Applications