Too many quiescent late-type galaxies or a matter of misclassification?

arXiv:2607.24664 · astro-ph.GA · Submitted 2026-07-27 · Read on arXiv

J. L. Tous, S. I. Raimundo, H. Domínguez Sánchez

astro-ph.GA

Submitted: 2026-07-27

Comments: Accepted for publication in MNRAS Letters, 6 pages, 3 figures

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Dust Attenuation — 1× in this paper · explained in 2 episodes
• Galaxy Quenching — 1× in this paper · explained in 3 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Revisiting the SFR-Mass relation at z=0 with detailed deep learning based morphologies
• Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$

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