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Record W4407342260 · doi:10.1051/0004-6361/202452018

<i>Euclid</i> preparation

2025· article· en· W4407342260 on OpenAlexaff
N Tessore, Benjamin Joachimi, A. Loureiro, A Hall, G Cañas-Herrera, I. Tutusaus, N Jeffrey, Krishna Naidoo, J.D. McEwen, A. Amara, S. Andreon, N. Auricchio, C. Baccigalupi, Marco Baldi, S. Bardelli, Francis Bernardeau, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, A. Caillat, S. Camera, V. Capobianco, C. Carbone, V. F. Cardone, J. Carretero, Santiago Casas, M. Castellano, G. Castignani, S. Cavuoti, A. Cimatti, G. Congedo, Christopher J. Conselice, L. Conversi, Y. Copin, F. Courbin, H. M. Courtois, M. Cropper, A. Da Silva, H. Degaudenzi, G. De Lucia, J. Dinis, F. Dubath, C.A.J Duncan, X. Dupac, S. Dusini, M. Farina, S. Farrens, F Faustini, S Ferriol, M. Frailis, E. Franceschi, M. Fumana, S. Galeotta, W. Gillard, B. Gillis, C. Giocoli, P. Gómez-Álvarez, A. Grazian, F. Grupp, L. Guzzo, S. V. H. Haugan, Henk Hoekstra, W. A. Holmes, F. Hormuth, A. Hornstrup, P. Hudelot, K. Jahnkę, M. Jhabvala, E. Keihänen, S. Kermiche, A. Kiessling, B. Kubik, M. Kümmel, M. Kunz, H. Kurki‐Suonio, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, G Mainetti, E. Maiorano, O. Mansutti, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R. Massey, E. Medinaceli, S. Mei, M. Melchior, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, J. J. Mohr, M. Moresco, B. Morin, L. Moscardini, E. Munari, R. Nakajima, S.-M Niemi, C. Padilla Aranda, S. Paltani, F. Pasian, Will J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. Popa, F. Raison, A. Renzi, Jason Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. P. Saglia, Z. Sakr, Ariel G. Sánchez, D. Sapone, B. Sartoris, M. Schirmer, Peter Schneider, T. Schrabback, A. Secroun, G. Seidel, M. D. Seiffert, S. Serrano, C. Sirignano, G. Sirri, L. Stančo, J. Steinwagner, P. Tallada-Crespí, A. N. Taylor, I. Tereno, R. Toledo-Moreo, F. Torradeflot, L. Valenziano, T. Vassallo, Yun Wang, J. Weller, G. Zamorani, E. Zucca, A. Biviano, M. Bolzonella, A. Boucaud, E. Bozzo, C. Burigana, M. Calabrese, D. Di Ferdinando, J.A. Escartin Vigo, F. Finelli⋆, J. Gracia-Carpio, S Matthew, N. Mauri, A Pezzotta, M. Pöntinen, V Scottez, A. Spurio Mancini, M. Tenti, Matteo Viel, M. Wiesmann, Y. Akrami, S Anselmi, M. Archidiacono, F. Atrio‐Barandela, A. Balaguera-Antolínez, M. Ballardini, D. Benielli, Alain Blanchard, L Blot, H. Böhringer, S. Borgani, S Bruton, R. Cabanac, Antonello Calabrò, B. Camacho Quevedo, A. Cappi, F Caro, C. S. Carvalho, T. Castro, K. C. Chambers, Asantha Cooray, S. de la Torre, G. Desprez, A. Díaz‐Sánchez, S. Di Domizio, H. Dole, S. Escoffier, A.G Ferrari, Pedro G. Ferreira, I. Ferrero, A. Finoguenov, A. Fontana, F. Fornari, L. Gabarra, K. Ganga, J. García-Bellido, T Gasparetto, E. Gaztañaga, F. Giacomini, F. Gianotti, G. Gozaliasl, C. M. Gutiérrez, W.G Hartley, H. Hildebrandt, J. Hjorth, A. Jiménez Muñoz, Shahab Joudaki, J. J. E. Kajava, V. Kansal, D. Karagiannis, C. C. Kirkpatrick, Sandor Kruk, F. Lacasa, M. Lattanzi, A.M.C Le Brun, J Le Graet, L. Legrand, Julien Lesgourgues, T.I Liaudat, J. F. Macías–Pérez, M. Magliocchetti, F. Mannucci, J Martín-Fleitas, C. J. A. P. Martins, L. Maurin, R. B. Metcalf, M Miluzio, Pierluigi Monaco, A Montoro, Chiara Moretti, G Morgante, Clare Murray, S. Nadathur, N. A. Walton, L. Patrizii, V. Popa, D. Potter, P. Reimberg, I Risso, P.-F Rocci, R. P. Rollins, M Sahlén, E Sarpa, Aurel Schneider, M. Sereno, P. Šimon, K Tanidis, C. Tao, G. Testera, Romain Teyssier, Sune Toft, S. Tosi, A. Troja, M. Tucci, C Valieri, J. Väliviita, D. Vergani, G Verza, P Vielzeuf, Michael D. Brown, E. Sellentin

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicParticle physics theoretical and experimental studies
Canadian institutionsSaint Mary's UniversityPerimeter InstituteUniversity of Waterloo
FundersCentro de Investigaciones Energéticas, Medioambientales y TecnológicasNational Astronomical Observatory of JapanInstitut de Física d'Altes EnergiesNorsk RomsenterUK Space AgencyAgenția Spațială RomânăEuropean Space AgencyAgenzia Spaziale ItalianaAgencia Estatal de InvestigaciónFundação para a Ciência e a TecnologiaMagyar Tudományos AkadémiaGeneralitat de CatalunyaNational Aeronautics and Space AdministrationMinisterio de Ciencia, Innovación y Universidades
KeywordsPhysicsAstrophysicsAstronomy

Abstract

fetched live from OpenAlex

In this paper we present the framework for measuring angular power spectra in the Euclid mission. The observables in galaxy surveys, such as galaxy clustering and cosmic shear, are not continuous fields, but discrete sets of data, obtained only at the positions of galaxies. We show how to compute the angular power spectra of such discrete data sets, without treating observations as maps of an underlying continuous field that is overlaid with a noise component. This formalism allows us to compute the exact theoretical expectations for our measured spectra, under a number of assumptions that we track explicitly. In particular, we obtain exact expressions for the additive biases (‘shot noise’) in angular galaxy clustering and cosmic shear. For efficient practical computations, we introduce a spin-weighted spherical convolution with a well-defined convolution theorem, which allows us to apply exact theoretical predictions to finite-resolution maps, including HEALPix. When validating our methodology, we find that our measurements are biased by less than 1% of their statistical uncertainty in simulations of Euclid’s first data release.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.002
metaresearch head score (Gemma)0.007
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: Not applicable
GenreCandidate signal: Methods · Consensus signal: none
Teacher disagreement score0.109
Threshold uncertainty score0.363

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.007
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.003
Science and technology studies0.0010.001
Scholarly communication0.0030.002
Open science0.0020.003
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.1090.085

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 head0.005
GPT teacher head0.246
Teacher spread0.241 · 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 source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designNot applicable
Domainnot available
GenreMethods

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

Citations6
Published2025
Admission routes1
Has abstractyes

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