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Record W4415171102 · doi:10.1051/0004-6361/202452468

<i>Euclid</i> preparation

2025· article· en· W4415171102 on OpenAlexaff
A. Humphrey, P. A. C. Cunha, Laura Bisigello, C. Tortora, M. Bolzonella, L. Pozzetti, M. Baes, B. R. Granett, A. Amara, N Auricchio, C. Baccigalupi, Marco Baldi, S. Bardelli, C. Bodendorf, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, S. Casas, M. Castellano, G. Castignani, C. Colodro-Conde, G. Congedo, Christopher J. Conselice, Y. Copin, F. Courbin, H. M. Courtois, H. Degaudenzi, G. De Lucia, J. Dinis, F. Dubath, X. Dupac, S. Dusini, M. Farina, S. Ferriol, M. Frailis, E. Franceschi, S. Galeotta, Koshy George, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, W. Holmes, I. Hook, A. Hornstrup, Benjamin Joachimi, 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, D. Maino, E Maiorano, O. Mansutti, O Marggraf, N. Martinet, F. Marulli, R. Massey, H. J. McCracken, E. Medinaceli, S. Mei, M. Melchior, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, L. Moscardini, E. Munari, R. Nakajima, S.-M Niemi, J.W Nightingale, C. Padilla Aranda, S. Paltani, F. Pasian, K. Pedersen, S. Pires, G. Polenta, M. Poncet, L. A. Popa, F. Raison, A. Renzi, J. D. Silverman, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. P. Saglia, Z. Sakr, Ariel G. Sánchez, D. Sapone, R. Scaramella, M. Scodeggio, A. Secroun, E. Sefusatti, S Serrano, C. Sirignano, L. Stanco, J. Steinwagner, A. N. Taylor, I Tereno, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, L. Valenziano, T. Vassallo, A. Veropalumbo, Y Wang, J. Weller, G. Zamorani, E. Zucca, A. Biviano, A. Boucaud, E. Bozzo, C. Burigana, M. Calabrese, R. Farinelli, N. Mauri, V Scottez, M. Tenti, Matteo Viel, M. Wiesmann, Y. Akrami, V. Allevato, S Anselmi, M. Ballardini, Alain Blanchard, S. Borgani, S Bruton, R. Cabanac, A Calabrò, G Cañas-Herrera, A. Cappi, T. Castro, K. C. Chambers, S. Contarini, J. Coupon, O. Cucciati, G. Desprez, A. Díaz‐Sánchez, S. Di Domizio, J.A. Escartin Vigo, S. Escoffier, A.G Ferrari, Pedro G. Ferreira, I. Ferrero, F. Fornari, L. Gabarra, J. García-Bellido, E. Gaztanaga, F. Giacomini, G. Gozaliasl, A. Gregorio, A Hall, H. Hildebrandt, J Hjorth, J. J. E. Kajava, V. Kansal, A. Loureiro, G. Maggio, M. Magliocchetti, C. J. A. P. Martins, S Matthew, L. Maurin, R. B. Metcalf, Pierluigi Monaco, Chiara Moretti, G. Morgante, N. A. Walton, J. Odier, L. Patrizii, M. Pöntinen, V. Popa, C. Porciani, D. Potter, I Risso, P.-F Rocci, M Sahlén, Aurel Schneider, M. Sereno, Pardis Simon, C. Tao, G. Testera, Romain Teyssier, Sune Toft, S. Tosi, A. Troja, M. Tucci, C Valieri, J. Väliviita, D. Vergani, G Verza

Bibliographic record

VenueAstronomy and Astrophysics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsSaint Mary's University
FundersNorsk RomsenterNational Astronomical Observatory of JapanEuropean Space AgencyAgenzia Spaziale ItalianaMinisterio de Ciencia, Innovación y UniversidadesÖsterreichische ForschungsförderungsgesellschaftFundação para a Ciência e a TecnologiaMagyar Tudományos AkadémiaDeutsches Zentrum für Luft- und RaumfahrtAgenția Spațială RomânăAcademy of FinlandCoordenação de Aperfeiçoamento de Pessoal de Nível SuperiorNational Aeronautics and Space AdministrationNvidia
KeywordsGalaxyPhotometry (optics)BroadbandRedshiftPipeline (software)Sky

Abstract

fetched live from OpenAlex

The Euclid Space Telescope will image about 14 000 deg2 of the extragalactic sky at visible and near-infrared wavelengths, providing a dataset of unprecedented size and richness that will facilitate a multitude of studies into the evolution of galaxies. Although spectroscopy will also be available for some of the galaxies, in the vast majority of cases the main source of information will come from broadband images and data products thereof (i.e. photometry). Therefore, there is a pressing need to identify or develop scalable yet reliable methodologies to estimate the redshift and physical properties of galaxies using broadband photometry from Euclid. Optionally, such methods could also include ground-based optical photometry. To address this need, we present a novel method developed as part of a ‘data challenge’ within the Euclid Collaboration to estimate the redshift, stellar mass, star-formation rate, specific star-formation rate, E(B − V), and age of galaxies using mock Euclid and ground-based photometry. The main novelty of our property-estimation pipeline is its use of the CatBoost implementation of gradient-boosted regression-trees together with chained regression and an intelligent, automatic optimisation of the training data. The pipeline also includes a computationally efficient method to estimate prediction uncertainties, and, in the absence of ground-truth labels, it provides accurate predictions for metrics of model performance up to z ~ 2. We applied our pipeline to several datasets consisting of mock Euclid broadband photometry and mock ground-based ugriz photometry, with the objective of evaluating the performance of our methodology for estimating the redshift and physical properties of galaxies detected in the Euclid Wide Survey. The statistical metrics of prediction residuals vary depending on which mock catalogue and filters are tested. Nonetheless, the quality of our photometric redshift and physical property estimates are highly competitive overall, validating our modelling approach. However, at z ≳ 3.5, the relative sparsity of galaxies resulted in unreliable redshift and physical property estimates, which we argue could be mitigated by building catalogues with better sampling of z ≳ 3.5 galaxies or by switching to the use of spectral energy distribution fitting in this regime. We also find that the inclusion of ground-based optical photometry significantly improves the quality of the property estimation, highlighting the importance of combining Euclid data with ancillary ground-based data from such surveys as the Vera C. Rubin Observatory Legacy Survey of Space and Time and UNIONS.

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)0.003
metaresearch head score (Gemma)0.011
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesInsufficient payload (model declined to judge)
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 score0.906
Threshold uncertainty score0.314

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.011
Meta-epidemiology (narrow)0.0020.001
Meta-epidemiology (broad)0.0010.002
Bibliometrics0.0030.005
Science and technology studies0.0010.001
Scholarly communication0.0040.002
Open science0.0040.003
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.0940.162

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 head0.216
Teacher spread0.212 · 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.

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".

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Citations2
Published2025
Admission routes1
Has abstractyes

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