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Record W4402651416 · doi:10.1051/0004-6361/202449609

<i>Euclid</i> preparation

2024· article· en· W4402651416 on OpenAlexaff
Ben Aussel, Sandor Kruk, Mike Walmsley, M. Castellano, Christopher J. Conselice, Michele Delli Veneri, H. Domínguez Sánchez, Pierre–Alain Duc, J. H. Knapen, Ulrike Kuchner, Antonio La Marca, B. Margalef-Bentabol, F. R. Marleau, Grant M. Stevens, Yoshiki Toba, C. Tortora, Lingyu Wang, K. Jahnkę, B. Altieri, A. Amara, S. Andreon, N. Auricchio, Marco Baldi, S. Bardelli, R. Bender, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, J. Carretero, Santiago Casas, S. Cavuoti, A. Cimatti, G. Congedo, L. Conversi, Y. Copin, F. Courbin, H. M. Courtois, M. Cropper, A. Da Silva, H. Degaudenzi, A. M. Di Giorgio, J. Dinis, F. Dubath, X Dupac, S. Dusini, M. Farina, S. Farrens, S. Ferriol, S. Fotopoulou, M. Frailis, E. Franceschi, P. Franzetti, M. Fumana, S. Galeotta, B. Garilli, B. Gillis, C. Giocoli, A. Grazian, F. Grupp, S. V. H. Haugan, W. Holmes, I. Hook, F. Hormuth, A. Hornstrup, P. Hudelot, E. Keihänen, S. Kermiche, A. Kiessling, M. Kilbinger, B. Kubik, M. Kümmel, M. Kunz, H. Kurki‐Suonio, R. Laureijs, S. Ligori, P. B. Lilje, V. Lindholm, I. Lloro, E. Maiorano, O. Mansutti, O. Marggraf, K. Markovič, N. Martinet, F. Marulli, R. Massey, S. Maurogordato, E. Medinaceli, S. Mei, Y. Mellier, M. Meneghetti, E. Merlin, G. Meylan, M. Moresco, L. Moscardini, E. Munari, S.-M Niemi, C. Padilla Aranda, Carmencita D. Padilla, F. Pasian, K. Pedersen, Will J. Percival, V. Pettorino, S. Pires, G. Polenta, M. Poncet, L. Popa, L. Pozzetti, F. Raison, R. Rébolo, A. Renzi, Jason Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, R. P. Saglia, D. Sapone, B. Sartoris, M. Schirmer, Peter Schneider, A. Secroun, G. Seidel, S. Serrano, C. Sirignano, G. Sirri, L. Stančo, Jean‐Luc Starck, P. Tallada-Crespí, A.N Taylor, Harry I. Teplitz, I. Tereno, R. Toledo-Moreo, F. Torradeflot, I. Tutusaus, E. A. Valentijn, L. Valenziano, T. Vassallo, A. Veropalumbo, Yun Wang, J. Weller, A. Zacchei, G. Zamorani, J. Zoubian, E. Zucca, A. Biviano, M. Bolzonella, A. Boucaud, E. Bozzo, C. Burigana, D. Di Ferdinando, R. Farinelli, J Gracia-Carpio, G. Mainetti, S. Marcin, N. Mauri, C. Neissner, Achille Nucita, Z. Sakr, V. Scottez, M. Tenti, Matteo Viel, M. Wiesmann, Y. Akrami, V. Allevato, S Anselmi, C. Baccigalupi, M. Ballardini, S. Borgani, Alejandro S. Borlaff, H. Bretonnière, S Bruton, R. Cabanac, Antonello Calabrò, A Cappi, C. S. Carvalho, G. Castignani, T. Castro, G Cañas-Herrera, K. C. Chambers, J. Coupon, O. Cucciati, S. Davini, G. De Lucia, G. Desprez, S. Di Domizio, H. Dole, A. Díaz‐Sánchez, J.A. Escartin Vigo, S. Escoffier, I. Ferrero, F. Finelli⋆, L. Gabarra, K. Ganga, J. García-Bellido, E. Gaztañaga, Koshy George, F. Giacomini, G. Gozaliasl, A. Gregorio, D. Guinet, A Hall, H. Hildebrandt, A. Jiménez Muñoz, J. J. E. Kajava, V. Kansal, D. Karagiannis, C. C. Kirkpatrick, L. Legrand, A. Loureiro, J. F. Macías–Pérez, M. Magliocchetti, M. Martinelli, C. J. A. P. Martins, S Matthew, M. Maturi, L. Maurin, R. B. Metcalf, M. Migliaccio, P Monaco, G. Morgante, S. Nadathur, N. A. Walton, Austin Peel, A Pezzotta, V. Popa, C. Porciani, D. Potter, M. Pöntinen, P. Reimberg, P.-F Rocci, Ariel G. Sánchez, Aurel Schneider, E. Sefusatti, M. Sereno, P. Šimon, A. Spurio Mancini, S. A. Stanford, J. Steinwagner, G. Testera, M. Tewes, Romain Teyssier, Sune Toft, S. Tosi, A. Troja, M. Tucci, C. Valieri, J. Väliviita, D. Vergani, I. A. Zinchenko

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsSaint Mary's UniversityPerimeter InstituteUniversity of Waterloo
FundersStaatssekretariat für Bildung, Forschung und InnovationFundação para a Ciência e a TecnologiaNorsk RomsenterAgenția Spațială RomânăNational Astronomical Observatory of JapanAgenzia Spaziale ItalianaMagyar Tudományos AkadémiaNational Aeronautics and Space AdministrationEuropean Space AgencyAlfred P. Sloan Foundation
KeywordsPhysicsAstrophysicsGalaxySpiral galaxyLenticular galaxyGalaxy formation and evolutionAstronomyArtificial intelligenceComputer science

Abstract

fetched live from OpenAlex

The Euclid mission is expected to image millions of galaxies at high resolution, providing an extensive dataset with which to study galaxy evolution. Because galaxy morphology is both a fundamental parameter and one that is hard to determine for large samples, we investigate the application of deep learning in predicting the detailed morphologies of galaxies in Euclid using Zoobot, a convolutional neural network pretrained with 450 000 galaxies from the Galaxy Zoo project. We adapted Zoobot for use with emulated Euclid images generated based on Hubble Space Telescope COSMOS images and with labels provided by volunteers in the Galaxy Zoo: Hubble project. We experimented with different numbers of galaxies and various magnitude cuts during the training process. We demonstrate that the trained Zoobot model successfully measures detailed galaxy morphology in emulated Euclid images. It effectively predicts whether a galaxy has features and identifies and characterises various features, such as spiral arms, clumps, bars, discs, and central bulges. When compared to volunteer classifications, Zoobot achieves mean vote fraction deviations of less than 12% and an accuracy of above 91% for the confident volunteer classifications across most morphology types. However, the performance varies depending on the specific morphological class. For the global classes, such as disc or smooth galaxies, the mean deviations are less than 10%, with only 1000 training galaxies necessary to reach this performance. On the other hand, for more detailed structures and complex tasks, such as detecting and counting spiral arms or clumps, the deviations are slightly higher, of namely around 12% with 60 000 galaxies used for training. In order to enhance the performance on complex morphologies, we anticipate that a larger pool of labelled galaxies is needed, which could be obtained using crowd sourcing. We estimate that, with our model, the detailed morphology of approximately 800 million galaxies of the Euclid Wide Survey could be reliably measured and that approximately 230 million of these galaxies would display features. Finally, our findings imply that the model can be effectively adapted to new morphological labels. We demonstrate this adaptability by applying Zoobot to peculiar galaxies. In summary, our trained Zoobot CNN can readily predict morphological catalogues for Euclid images.

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)0.008
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: none
Teacher disagreement score0.181
Threshold uncertainty score0.606

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.008
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.002
Science and technology studies0.0010.001
Scholarly communication0.0020.002
Open science0.0030.002
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.1810.157

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 head0.208
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 designBench or experimental
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

Citations15
Published2024
Admission routes1
Has abstractyes

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