TY - JOUR

T1 - Galaxy Zoo JWST

T2 - Up to 75% of discs are featureless at 3 < z < 7

AU - Smethurst, R J

AU - Simmons, B D

AU - Géron, T

AU - Dickinson, H

AU - Fortson, L

AU - Garland, I L

AU - Kruk, S

AU - Jewell, S M

AU - Lintott, C J

AU - Makechemu, J S

AU - Mantha, K B

AU - Masters, K L

AU - O’Ryan, D

AU - Roberts, H

AU - Thorne, M R

AU - Walmsley, M

AU - Calabrò, M

AU - Holwerda, B

AU - Kartaltepe, J S

AU - Koekemoer, A M

AU - Lyu, Y

AU - Lucas, R

AU - Pacucci, F

AU - Tarrasse, M

PY - 2025/3/28

Y1 - 2025/3/28

N2 - 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.

AB - 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.

U2 - 10.1093/mnras/staf506

DO - 10.1093/mnras/staf506

M3 - Journal article

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

ER -