Euclid Quick Data Release (Q1) XIII. Exploring galaxy properties with a multi-modal foundation model
| dc.contributor.author | Karagiannis, Dionysios | |
| dc.contributor.author | Siudek, Małgorzata | |
| dc.contributor.author | Huertas-Company, Marc | |
| dc.date.accessioned | 2026-08-13T07:21:00Z | |
| dc.date.available | 2026-08-13T07:21:00Z | |
| dc.date.issued | 2026 | |
| dc.description.abstract | Modern astronomical surveys, such as the Euclid mission, produce high-dimensional, multi-modal datasets that include imaging and spectroscopic information for millions of galaxies. These data serve as an ideal benchmark for large, pre-trained multi-modal models, which can leverage vast amounts of unlabelled data. In this work, we present the first exploration of Euclid data with AstroPT, an autoregressive multi-modal foundation model trained on approximately 300000 optical and infrared Euclid images and spectral energy distributions (SEDs) from the first Euclid Quick Data Release. We compare self-supervised pre-training with baseline fully supervised training across several tasks: galaxy morphology classification; redshift estimation; similarity searches; and outlier detection. Our results show that: (a) AstroPT embeddings are highly informative, correlating with morphology and effectively isolating outliers; (b) including infrared data helps to isolate stars, but degrades the identification of edge-on galaxies, which are better captured by optical images; (c) simple fine-tuning of these embeddings for photometric redshift and stellar mass estimation outperforms a fully supervised approach, even when using only 1% of the training labels; and (d) incorporating SED data into AstroPT via a straightforward multi-modal token-chaining method improves photo-z predictions, and allow us to identify potentially more interesting anomalies (such as ringed or interacting galaxies) compared to a model pre-trained solely on imaging data. © The Authors 2026. Open Access article, https://www-edpsciences-org.ezproxy.uwc.ac.za, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.This article is published in open access under the https://www-aanda-org.ezproxy.uwc.ac.za/subscribe-to-open-faqs. mailto:subscribers@edpsciences.org to support open access publication. | |
| dc.identifier.citation | Siudek, M. & Smith, M. & Martínez-Solaeche, G. & Lanusse, F. & ho, Sanh & Angeloudi, E. & Cunha, P. & Domínguez Sánchez, H. & Dunn, Marina & Fu, Yuming & Iglesias-Navarro, P. & Junais, J. & Knapen, J. & Laloux, B. & Mezcua, M. & Roster, William & Stevens, Grant & Vega-Ferrero, Jesús & Sorce, J.. (2026). Euclid Quick Data Release (Q1): XIII. Exploring galaxy properties with a multi-modal foundation model. Astronomy & Astrophysics. 711. A13. 10.1051/0004-6361/202554611. | |
| dc.identifier.uri | https://doi.org/10.1051/0004-6361/202554611 | |
| dc.identifier.uri | https://hdl.handle.net/10566/25145 | |
| dc.language.iso | en | |
| dc.publisher | EDP Sciences | |
| dc.subject | Methods | |
| dc.subject | data analysis | |
| dc.subject | galaxies | |
| dc.subject | general | |
| dc.subject | red shift | |
| dc.title | Euclid Quick Data Release (Q1) XIII. Exploring galaxy properties with a multi-modal foundation model | |
| dc.type | Article |