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Record W4416983271 · doi:10.48550/arxiv.2512.01489

Euclid: The first statistical census of dusty and massive objects in the ERO/Perseus field

2025· preprint· en· W4416983271 on OpenAlexaff
G. Girardi, A. Grazian, G. Rodighiero, L Bisigello, G. Gandolfi, Eduardo Bañados, S. Belladitta, J. R. Weaver, S. Eales, Christopher C. Lovell, K. I. Caputi, A Enia, Alessandro Bianchetti, E. Dalla Bontà, T. Saifollahi, A. Vietri, N. Aghanim, B Altieri, N. Auricchio, H Aussel, C. Baccigalupi, A. Balestra, S Bardelli, P Battaglia, A. Biviano, E. Branchini, M. Brescia, J Brinchmann, S. Camera, V Capobianco, J. Carretero, M. Castellano, G. Castignani, S Cavuoti, K. C. Chambers, C. Colodro-Conde, G. Congedo, Christopher J. Conselice, F Courbin, H. M. Courtois, M. Cropper, H. Degaudenzi, G. De Lucia, A.M Di Giorgio, F. Dubath, X. Dupac, S. Dusini, S. Escoffier, M. Farina, R. Farinelli, F Faustini, S. Ferriol, S. Fotopoulou, E. Franceschi, M. Fumana, S. Galeotta, Koshy George, B. Gillis, C. Giocoli, J. Graciá‐Carpio, F. Grupp, S. V. H. Haugan, W. Holmes, I. Hook, F. Hormuth, P. Hudelot, A. Bongiorno, M. Jhabvala, E Keihänen, S. Kermiche, A. Kiessling, B. Kubik, M Kümmel, M. Kunz, H. Kurki‐Suonio, A.M.C Le Brun, D. Le Mignant, P. Liebing, S. Ligori, P. B. Lilje, I. Lloro, G Mainetti, D. Maino, S Marcin, O Marggraf, M. Martinelli, N. Martinet, R Massey, S. Maurogordato, E. Medinaceli, S. Mei, Y Mellier, E. Merlin, G. Meylan, Antonio M. Mora, M. Moresco, L. Moscardini, R. Nakajima, C. Neissner, S. -M. Niemi, C. Padilla, S. Paltani, F. Pasian, K. Pedersen, W.J Percival, G. Polenta, M. Poncet, L. A. Popa, L. Pozzetti, F. Raison, A. Renzi, J Rhodes, G. Riccio, E. Romelli, M. Roncarelli, E. Rossetti, B. Rusholme, R. Saglia, Z. Sakr, D. Sapone, B. Sartoris, J.A Schewtschenko, Peter Schneider, T. Schrabback, A. Secroun, G. Seidel, M. D. Seiffert, S. Serrano, Patrice Simon, C Sirignano, G. Sirri, L. Stanco, D. Tavagnacco, A. N. Taylor, I. Tereno, F. Torradeflot, I. Tutusaus, L. Valenziano, J. Valiviita, G. Verdoes Kleijn, A Veropalumbo, Y. Wang, F. M. Zerbi, E. Zucca, M. Bolzonella, C. Burigana, L. Gabarra, J Martín-Fleitas, V Scottez

Bibliographic record

VenuearXiv (Cornell University) · 2025
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsPerimeter InstituteUniversity of Waterloo
Fundersnot available
KeywordsGalaxyRedshiftField (mathematics)PopulationSpitzer Space TelescopeStar formationCensusInfrared

Abstract

fetched live from OpenAlex

Our comprehension of the history of star formation at $z>3$ relies on rest-frame UV observations, yet this selection misses the most dusty and massive sources, yielding an incomplete census at early times. Infrared facilities such as Spitzer and the James Webb Space Telescope have revealed a hidden population at $z=3$-$6$ with extreme red colours, named HIEROs (HST-to-IRAC extremely red objects), identified by the criterion $H_{\mathrm{E}}-\mathrm{ch2}>2.25$. Recently, Euclid Early Release Observations (ERO) have made it possible to further study such objects by comparing Euclid data with ancillary Spitzer/IRAC imaging. We investigate a $232$ arcmin$^2$ area in the Perseus field using VIS and NISP photometry, complemented by the four Spitzer channels and ground-based MegaCam bands ($u$, $g$, $r$, ${\rm H}α$, $i$, $z$). Applying the colour cut yields $121$ HIEROs; after removing globular clusters, brown dwarfs, and unreliable cases through visual inspection of multiband cutouts, we obtain a final sample of $42$ robust HIEROs. Photometric redshifts and physical properties are estimated with the SED-fitting code Bagpipes. From the resulting $z_{\mathrm{phot}}$ and $M_*$ values, we compute the galaxy stellar mass function at $3.5

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)0.000
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.006
Threshold uncertainty score0.012

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.025
GPT teacher head0.182
Teacher spread0.157 · 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 designObservational
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

Citations0
Published2025
Admission routes1
Has abstractyes

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Same venuearXiv (Cornell University)→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→