JWST Reveals a Surprisingly High Fraction of Galaxies Being Spiral-like at $0.5\leq z\leq4$

TL;DR

This study uses JWST images to identify a surprisingly high fraction of spiral galaxies from redshift 0.5 to 4, revealing early formation of spiral arms and disks in the universe.

Contribution

It provides the first large-scale visual identification of spiral galaxies at high redshift using JWST, showing a higher spiral fraction than previously observed with HST.

Findings

Spiral fraction decreases from 48% at z~0.75 to 8% at z~2.75.

Detected possible spiral features at z>3.

High spiral fraction suggests early formation of spiral arms and disks.

Abstract

Spiral arms are one of the most important features used to classify the morphology of local galaxies. The cosmic epoch when spiral arms first appeared contains essential clues to the evolution of disk galaxies. In this letter, we used James Webb Space Telescope (JWST) images from the Cosmic Evolution Early Release Science Survey to visually identify spiral galaxies with redshift $0.5\leq z\leq4$ and stellar mass $\geq10^{10}\; M_\odot$. Out of 873 galaxies, 216 were found to have a spiral structure. The spiral galaxies in our sample have higher star formation rates (SFRs) and larger sizes than non-spiral galaxies. We found the observed spiral fraction decreases from 48% at $z\sim0.75$ to 8% at $z\sim2.75$. These fractions are higher than the fractions observed with the Hubble Space Telescope (HST). We even detect possible spiral-like features at redshifts $z>3$. We artificially redshifted low redshift galaxies to high redshifts and re-inspected them to evaluate observational effects. By varying the input spiral fraction of the redshifted sample, we found that the input fraction of $\sim35$% matches the observed fraction at $z=2-3$ the best. We are able to rule out spiral fractions being $<20$% (2$\sigma$) and $<10$% (3$\sigma$) for real galaxies at $z\sim3$. This fraction is surprisingly high and implies that the formation of spiral arms, as well as disks, was earlier in the universe.