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Record W4399366338 · doi:10.1088/1475-7516/2024/06/011

Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRD

2024· article· en· W4399366338 on OpenAlexaff
C. Leloup, G. Patanchon, Josquin Errard, C. Franceschet, Jon E. Gudmundsson, S. Henrot–Versillé, Hiroaki Imada, H. Ishino, T. Matsumura, Giuseppe Puglisi, W. Wang, Alexandre Adler, J. Aumont, R. Aurlien, C. Baccigalupi, M. Ballardini, A. J. Banday, R. B. Barreiro, N. Bartolo, A. Basyrov, M. Bersanelli, D. Blinov, M. Bortolami, Thejs Brinckmann, P. Campeti, A. Carones, F. Carralot, F. J. Casas, K. Cheung, Lionel Clermont, F. Columbro, G. Conenna, A. Coppolecchia, F. Cuttaia, Nadia Dachlythra, G. D’Alessandro, P. de Bernardis, T. de Haan, M. De Petris, S. Della Torre, P. Diego-Palazuelos, H. K. Eriksen, F. Finelli⋆, U. Fuskeland, G. Galloni, M. Galloway, Marc Georges, M. Gerbino, M. Gervasi, R.T. Génova-Santos, T. Ghigna, S. Giardiello, C. Gimeno-Amo, E. Gjerløw, A. Gruppuso, M. Hazumi, L. T. Hergt, D. Herranz, E. Hivon, D. Hoang, Baptiste Jost, Kazunori Kohri, N. Krachmalnicoff, A. T. Lee, M Lembo, François Levrier, A.I. Lonappan, M. López-Caniego, J. F. Macías–Pérez, E. Martínez-González, S. Masi, S. Matarrese, S. Micheli, M. Monelli, L. Montier, G. Morgante, B. Mot, L. Mousset, Toshiya Namikawa, P. Natoli, A. Novelli, F. Noviello, Ippei Obata, Kimihide Odagiri, L. Pagano, A. Paiella, D. Paoletti, G. Pascual-Cisneros, V. Pavlidou, F. Piacentini, G. Piccirilli, G. Pisano, G. Polenta, N. Raffuzzi, M. Remazeilles, A. Ritacco, A. Rizzieri, M. Ruiz-Granda, Y. Sakurai, Maresuke Shiraishi, S. L. Stever, Yusuke Takase, Konstantinos Tassis, L. Terenzi, K. Thompson, M. Tristram, L. Vacher, P. Vielva, I. K. Wehus, G. Weymann-Despres, M. Zannoni, Yu-Feng Zhou

Bibliographic record

VenueJournal of Cosmology and Astroparticle Physics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAdvanced Optical Sensing Technologies
Canadian institutionsUniversity of British Columbia
FundersAgencia Estatal de InvestigaciónCentre National de la Recherche ScientifiqueVetenskapsrådetSwedish National Space AgencyJapan Society for the Promotion of ScienceNational Aeronautics and Space AdministrationCentre National d’Etudes SpatialesMinistry of Education, Culture, Sports, Science and TechnologyU.S. Department of EnergyJapan Aerospace Exploration AgencyEuropean CommissionDeutsche Forschungsgemeinschaft
KeywordsPhysicsFar side of the MoonBeam (structure)AstronomyParticle physicsOptics

Abstract

fetched live from OpenAlex

Abstract We present a study of the impact of a beam far side-lobe lack of knowledge on the measurement of the Cosmic Microwave Background B -mode signal at large scale. Beam far side-lobes induce a mismatch in the transfer function of Galactic foregrounds between the dipole and higher multipoles which degrads the performances of component separation methods. This leads to foreground residuals in the CMB map. It is expected to be one of the main source of systematic effects in future CMB polarization observations. Thus, it becomes crucial for all-sky survey missions to take into account the interplays between beam systematic effects and all the data analysis steps. LiteBIRD is the ISAS/JAXA second strategic large-class satellite mission and is dedicated to target the measurement of CMB primordial B modes by reaching a sensitivity on the tensor-to-scalar ratio r of σ ( r ) ≤ 10 -3 assuming r = 0. The primary goal of this paper is to provide the methodology and develop the framework to carry out the end-to-end study of beam far side-lobe effects for a space-borne CMB experiment. We introduce uncertainties in the beam model, and propagate the beam effects through all the steps of the analysis pipeline, most importantly including component separation, up to the cosmological results in the form of a bias δr . As a demonstration of our framework, we derive requirements on the calibration and modeling for the LiteBIRD 's beams under given assumptions on design, simulation, component separation method and allocated error budget. In particular, we assume a parametric method of component separation with no mitigation of the far side-lobes effect at any stage of the analysis pipeline. We show that δr is mostly due to the integrated fractional power difference between the estimated beams and the true beams in the far side-lobes region, with little dependence on the actual shape of the beams, for low enough δr . Under our set of assumptions, in particular considering the specific foreground cleaning method we used, we find that the integrated fractional power in the far side-lobes should be known at the level of ∼ 10 -4 , to achieve the required limit on the bias δr < 1.9 × 10 -5 . The framework and tools developed for this study can be easily adapted to provide requirements under different design, data analysis frameworks and for other future space-borne experiments, such as PICO or CMB-Bharat. We further discuss the limitations of this framework and potential extensions to circumvent them.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: Theoretical or conceptual
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.328
Threshold uncertainty score0.220

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.021
GPT teacher head0.329
Teacher spread0.308 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designTheoretical or conceptual
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations8
Published2024
Admission routes1
Has abstractyes

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