Smethurst, R J and Simmons, B D and Géron, T and Dickinson, H and Fortson, L and Garland, I L and Kruk, S and Jewell, S M and Lintott, C J and Makechemu, J S and Mantha, K B and Masters, K L and O’Ryan, D and Roberts, H and Thorne, M R and Walmsley, M and Calabrò, M and Holwerda, B and Kartaltepe, J S and Koekemoer, A M and Lyu, Y and Lucas, R and Pacucci, F and Tarrasse, M (2025) Galaxy Zoo JWST : Up to 75% of discs are featureless at 3 < z < 7. Monthly Notices of the Royal Astronomical Society. ISSN 0035-8711
Full text not available from this repository.Abstract
We have not yet observed the epoch at which disc galaxies emerge in the Universe. While high-z measurements of large-scale features such as bars and spiral arms trace the evolution of disc galaxies, such methods cannot directly quantify featureless discs in the early Universe. Here we identify a substantial population of apparently featureless disc galaxies in the Cosmic Evolution Early Release Science (CEERS) survey by combining quantitative visual morphologies of ∼7000 galaxies from the Galaxy Zoo JWST CEERS project with a public catalogue of expert visual and parametric morphologies. While the highest-redshift featured disc we identify is at zphot = 5.5, the highest-redshift featureless disc we identify is at zphot = 7.4. The distribution of Sérsic indices for these featureless systems suggests that they truly are dynamically cold: disc-dominated systems have existed since at least z ∼ 7.4. We place upper limits on the featureless disc fraction as a function of redshift, and show that up to 75% of discs are featureless at 3.0 < z < 7.4. This is a conservative limit assuming all galaxies in the sample truly lack features. With further consideration of redshift effects and observational constraints, we find the featureless disc fraction in CEERS imaging at these redshifts is more likely $\sim 29-38~{{\%}}$. We hypothesise that the apparent lack of features in a third of high-redshift discs is due to a higher gas fraction in the early Universe, which allows the discs to be resistant to buckling and instabilities.