The Early Maturity of High-Redshift Galaxies: Insights from sSFR, M/L and SFHs at z~7-14
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2025
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| author | Santini, P. Castellano, M. Calabrò, A. Fontana, A. Merlin, E. Bevacqua, D. Bergamini, P. Boquien, M. Cantarella, S. Ciesla, L. Ferrara, A. Finkelstein, S. L. Fortuni, F. Gandolfi, G. Gasparetto, T. Giallongo, E. Grogin, N. A. Guida, S. T. Koekemoer, A. M. Menci, N. Napolitano, L. Paris, D. Pentericci, L. Perez-Diaz, B. Stoyanova, B. Treu, T. |
| author_facet | Santini, P. Castellano, M. Calabrò, A. Fontana, A. Merlin, E. Bevacqua, D. Bergamini, P. Boquien, M. Cantarella, S. Ciesla, L. Ferrara, A. Finkelstein, S. L. Fortuni, F. Gandolfi, G. Gasparetto, T. Giallongo, E. Grogin, N. A. Guida, S. T. Koekemoer, A. M. Menci, N. Napolitano, L. Paris, D. Pentericci, L. Perez-Diaz, B. Stoyanova, B. Treu, T. |
| contents | The James Webb Space Telescope (JWST) has revealed an unexpected excess of UV-bright galaxies at z>10, unaccounted for by extrapolations from pre-JWST observations and theoretical models. Understanding the physical properties and star formation histories (SFHs) of high-redshift systems is key to distinguishing between the proposed scenarios. We identified and analysed a sample of 2420 robust candidates at z~7-14 drawn from the ASTRODEEP-JWST dataset over ~0.2 deg^2, and modelled their properties with non-parametric SFHs to derive the specific star formation rate (sSFR) and stellar population properties. We find that the median sSFR and M/L remain roughly constant across the probed redshift range. We show that this result is robust against potential systematics unless a hidden population of dust-enshrouded starbursts, undetectable in current data, exists at these redshifts. In any case, the absence of observed high-sSFR systems at the highest redshifts suggests that any dust-free starburst phase must be short-lived. The observed sSFR evolution is in tension with most theoretical models, making it a key quantity for discriminating among competing scenarios. The sample shows a wide range of physical conditions and galaxy classes, including systems with low sSFRs and high mass-to-light ratios (M/L) up to z~10, indicative of already-evolved galaxies only a few hundred Myr after the Big Bang, and different degrees of dust attenuation. We finally reconstructed the assembly histories of two sub-samples, namely the highest-M/L galaxies at z~7-8, which appear to have formed the bulk of their stars at least 500 Myr before observation, implying progenitors observable as UV-bright sources at z>20, and the full sample of z>11 galaxies, which formed through stochastic SFHs, remaining UV-faint for most of their early evolution, before undergoing recent (~50 Myr old) episodes of major growth. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_09139 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The Early Maturity of High-Redshift Galaxies: Insights from sSFR, M/L and SFHs at z~7-14 Santini, P. Castellano, M. Calabrò, A. Fontana, A. Merlin, E. Bevacqua, D. Bergamini, P. Boquien, M. Cantarella, S. Ciesla, L. Ferrara, A. Finkelstein, S. L. Fortuni, F. Gandolfi, G. Gasparetto, T. Giallongo, E. Grogin, N. A. Guida, S. T. Koekemoer, A. M. Menci, N. Napolitano, L. Paris, D. Pentericci, L. Perez-Diaz, B. Stoyanova, B. Treu, T. Astrophysics of Galaxies The James Webb Space Telescope (JWST) has revealed an unexpected excess of UV-bright galaxies at z>10, unaccounted for by extrapolations from pre-JWST observations and theoretical models. Understanding the physical properties and star formation histories (SFHs) of high-redshift systems is key to distinguishing between the proposed scenarios. We identified and analysed a sample of 2420 robust candidates at z~7-14 drawn from the ASTRODEEP-JWST dataset over ~0.2 deg^2, and modelled their properties with non-parametric SFHs to derive the specific star formation rate (sSFR) and stellar population properties. We find that the median sSFR and M/L remain roughly constant across the probed redshift range. We show that this result is robust against potential systematics unless a hidden population of dust-enshrouded starbursts, undetectable in current data, exists at these redshifts. In any case, the absence of observed high-sSFR systems at the highest redshifts suggests that any dust-free starburst phase must be short-lived. The observed sSFR evolution is in tension with most theoretical models, making it a key quantity for discriminating among competing scenarios. The sample shows a wide range of physical conditions and galaxy classes, including systems with low sSFRs and high mass-to-light ratios (M/L) up to z~10, indicative of already-evolved galaxies only a few hundred Myr after the Big Bang, and different degrees of dust attenuation. We finally reconstructed the assembly histories of two sub-samples, namely the highest-M/L galaxies at z~7-8, which appear to have formed the bulk of their stars at least 500 Myr before observation, implying progenitors observable as UV-bright sources at z>20, and the full sample of z>11 galaxies, which formed through stochastic SFHs, remaining UV-faint for most of their early evolution, before undergoing recent (~50 Myr old) episodes of major growth. |
| title | The Early Maturity of High-Redshift Galaxies: Insights from sSFR, M/L and SFHs at z~7-14 |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2512.09139 |