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Record W4417474333 · doi:10.1051/0004-6361/202555402

<i>Euclid</i> preparation

2025· article· en· W4417474333 on OpenAlexaff
I Risso, A Veropalumbo, E. Branchini, Edoardo Maragliano, S. de la Torre, E Sarpa, P. Monaco, B. R. Granett, S. Lee, Graeme E. Addison, S Bruton, C. Carbone, G. Lavaux, K. Markovič, G. Parimbelli, F Passalacqua, Will J. Percival, C. Scarlata, E. Sefusatti, Marco Bonici, F Oppizzi, N. Aghanim, A. Amara, A Amara, S. Andreon, N Auricchio, C. Baccigalupi, M. Baldi, A. Balestra, S Bardelli, Pietro Battaglia, A. Biviano, A Bonchi, D. Bonino, M. Brescia, J Brinchmann, S. Camera, V Capobianco, V.F Cardone, J. Carretero, S. Casas, M Castellano, G. Castignani, S. Cavuoti, K. C. Chambers, A. Cimatti, C. Colodro-Conde, G. Congedo, C.J. Conselice, L. Conversi, F Courbin, H. M. Courtois, M. Crocce, A da Silva, H Degaudenzi, G. De Lucia, A. M. Di Giorgio, H. Dole, M. Douspis, F. Dubath, C.A.J Duncan, X. Dupac, S Dusini, S. Escoffier, M. Farina, R. Farinelli, F Faustini, S. Ferriol, F Finelli, S. Fotopoulou, N. Fourmanoit, M. Frailis, E. Franceschi, M Fumana, S. Galeotta, K. George, W Gillard, B Gillis, C. Giocoli, J. Gracia-Carpio, A. Grazian, F Grupp, L. Guzzo, S. V. H. Haugan, W. N. Holmes, F. Hormuth, P. Hudelot, A. Bongiorno, M. Jhabvala, B. Joachimi, E Keihänen, S. Kermiche, A. Kiessling, M. Kilbinger, B. Kubik, M Kümmel, M. Kunz, H Kurki-Suonio, A.M.C Le Brun, P. Liebing, S. Ligori, P.B. Lilje, V. Lindholm, I. Lloro, G. Mainetti, D. Maino, E Maiorano, O. Mansutti, S. Marcin, O. Marggraf, M. Martinelli, N. Martinet, F. Marulli, R Massey, S. Maurogordato, E. Medinaceli, S. Mei, M Melchior, Y. Mellier, E. Merlin, G. Meylan, A Mora, M. Moresco, L. Moscardini, R Nakajima, C Neissner, S.-M Niemi, J.W Nightingale, Carmencita D. Padilla, S. Paltani, F. Pasian, K. Pedersen, V. Pettorino, S. Pires, G Polenta, M. Poncet, L.A. Popa, R Rebolo, R. Rebolo, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M Roncarelli, E. Rossetti, R. Saglia, Z. Sakr, D Sapone, B. Sartoris, J.A Schewtschenko, P. Schneider, T. Schrabback, M. Scodeggio, A. Secroun, G. Seidel, M. Seiffert, S Serrano, Patrice Simon, C Sirignano, G. Sirri, L. Stanco, J. Steinwagner, C. Surace, P. Tallada-Crespí, A.N. Taylor, I Tereno, N Tessore, Sune Toft, F. Torradeflot, I Tutusaus, L Valenziano, J Valiviita, T. Vassallo, D. Vibert, J Weller, G. Zamorani, F. M. Zerbi, E Zucca, V. Allevato, M Ballardini, M Bolzonella, E. Bozzo, C. Burigana, R. Cabanac, A. Cappi, D. Di Ferdinando, J.A. Escartin Vigo, L. Gabarra, W.G. Hartley, J. Martín-Fleitas, S Matthew, N. Mauri, R. B. Metcalf, M. Pöntinen, C Porciani, V. Scottez, M Sereno, M. Tenti, M. Viel, M. Wiesmann, Y. Akrami, S Alvi, I.T Andika, M. Archidiacono, F. Atrio‐Barandela, S. Àvila, A. Balaguera-Antolínez, Christophe Benoıst, Daniele Bertacca, M. Béthermin, L Blot, H. Böhringer, S Borgani, Michael D. Brown, B. Camacho Quevedo, F Caro, C. S. Carvalho, T. Castro, F Cogato, A.R. Cooray, S. Davini, F. De Paolis, A. Díaz‐Sánchez, J.J Diaz, S. Di Domizio, J. M. Diego, Paola Dimauro, A Enia, Yiming Fang, A.G Ferrari, A. Finoguenov, A. Fontana, A. A. Franco, K. Ganga, J. García-Bellido, V. Gautard, E. Gaztanaga, F. Giacomini, F. Gianotti, G. Gozaliasl, María Guidi, C. M. Gutiérrez, A. J. Hall, Shoubaneh Hemmati, Alex Hall, H Hildebrandt, J. Hjorth, Shahab Joudaki, J. J. E. Kajava, Yongshui Kang, Vinay Kansal, D. Karagiannis, K. Kiiveri, C. Kirkpatrick, Sergey Kruk, V. Le Brun, J Le Graet, L Legrand, M Lembo, Francesca Lepori, G. Leroy, G.F Lesci, L. Leuzzi, T.I Liaudat, A. Loureiro, J. F. Macías–Pérez, M. Magliocchetti, F. Mannucci, C.J.A.P. Martins, Louis Maurin, M. Miluzio, Claudio Moretti, G. Morgante, K Naidoo, A. Navarro-Alsina, K Paterson, L Patrizii, Alice Pisani, D. Potter, S Quai, M Radovich, P.-F Rocci, S Sacquegna, M Sahlén, D. B. Sanders, A. Schneider, D Sciotti, E. Sellentin, L. C. Smith, Jenny G. Sorce, K Tanidis, Chihiro Tao, G. Testera, R Teyssier, Sébastien Tosi, A Troja, M. Tucci, C. Valieri, A. Venhola, D. Vergani, G Verza, N.A. Walton

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsPerimeter InstituteUniversity of Waterloo
FundersFundação para a Ciência e a TecnologiaNorsk RomsenterAgenția Spațială RomânăAgenzia Spaziale ItalianaMagyar Tudományos AkadémiaMinistero dell’Istruzione, dell’Università e della RicercaNational Astronomical Observatory of JapanEuropean CommissionEuropean Space AgencyNational Aeronautics and Space Administration
KeywordsRedshiftGalaxyCorrelation function (quantum field theory)Redshift surveyRedshift-space distortionsMeasure (data warehouse)Galaxy formation and evolution

Abstract

fetched live from OpenAlex

Context. The Euclid galaxy survey is designed to measure the spectroscopic redshift of emission-line galaxies (ELGs) by identifying the H α emission line in their slitless spectra. The efficacy of this approach crucially depends on the signal-to-noise ratio (S/N) of the line, as sometimes noise fluctuations in the spectrum continuum can be misidentified as H α . In addition, other genuine strong emission lines can be mistaken for H α , depending on the redshift of the source. Both effects lead to ambiguities in the redshift measurement that can result in catastrophic redshift errors and the inclusion of ‘interloper’ galaxies in the sample. Aims. This paper forecasts the impact on the galaxy clustering analysis of the expected redshift errors in the Euclid spectroscopic sample. Specifically, it investigates the effect of the redshift interloper contamination on the galaxy two-point correlation function (2PCF) and, in turn, on the inferred growth rate of structure fσ 8 and Alcock–Paczynski (AP) parameters α ∥ and α ⊥ . Methods. This work is based on the analysis of 1000 synthetic spectroscopic catalogues, the EuclidLargeMocks, which mimic the area and selection function of the Euclid Data Release 1 (DR1) sample. We estimated the 2PCF of contaminated catalogues and separated the different contributions, particularly those coming from galaxies with correctly measured redshift and from contaminants. We explored different models of increasing complexity to describe the measured 2PCF at a fixed cosmology, with the aim of identifying the most efficient model to reproduce the data. Finally, we performed a cosmological inference and evaluated the systematic error on the inferred fσ 8 , α ∥ , and α ⊥ values associated with different models. Results. Our results demonstrate that a minimal modelling approach, which only accounts for an attenuation of the clustering signal regardless of the type of contaminants, is sufficient to recover the correct values of fσ 8 , α ∥ , and α ⊥ at DR1. The accuracy and precision of the estimated AP parameters are largely insensitive to the presence of interlopers. The adoption of a minimal modelling induces a 1%–3% systematic error on the growth rate of structure estimation, depending on the considered redshift. However, this error remains smaller than the statistical error expected for the Euclid DR1 analysis.

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)0.014
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: Other · Consensus signal: none
Teacher disagreement score0.241
Threshold uncertainty score0.807

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.014
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0040.006
Science and technology studies0.0010.001
Scholarly communication0.0030.001
Open science0.0020.003
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.2410.169

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 head0.004
GPT teacher head0.207
Teacher spread0.203 · 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
GenreOther

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

Citations1
Published2025
Admission routes1
Has abstractyes

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