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A JWST investigation into the bar fraction at redshifts 1 ≤ z ≤ 3

Le Conte, Zoe A; Gadotti, Dimitri A; Ferreira, Leonardo; Conselice, Christopher J; de Sá-Freitas, Camila; Kim, Taehyun; Neumann, Justus; Fragkoudi, Francesca; Athanassoula, E; Adams, Nathan J

A JWST investigation into the bar fraction at redshifts 1 ≤ z ≤ 3 Thumbnail


Authors

Zoe Le Conte zoe.a.le-conte@durham.ac.uk
PGR Student Doctor of Philosophy

Leonardo Ferreira

Christopher J Conselice

Camila de Sá-Freitas

Taehyun Kim

Justus Neumann

E Athanassoula

Nathan J Adams



Abstract

The presence of a stellar bar in a disc galaxy indicates that the galaxy hosts in its main part a dynamically settled disc and that bar-driven processes are taking place in shaping its evolution. Studying the cosmic evolution of the bar fraction in disc galaxies is therefore essential to understand galaxy evolution in general. Previous studies have found, using the Hubble Space Telescope (HST), that the bar fraction significantly declines from the local Universe to redshifts near one. Using the first four pointings from the JWST Cosmic Evolution Early Release Science Survey and the initial public observations for the Public Release Imaging for Extragalactic Research, we extend the studies of the bar fraction in disc galaxies to redshifts 1 ≤ z ≤ 3, that is, for the first time beyond redshift two. We only use galaxies that are also present in the Cosmic Assembly Near-IR Deep Extragalactic Legacy Survey on the Extended Groth Strip and Ultra Deep Survey HST observations. An optimized sample of 368 close-to-face-on galaxies is visually classified to find the fraction of bars in disc galaxies in two redshift bins: 1 ≤ z ≤ 2 and 2 < z ≤ 3. The bar
fraction decreases from ≈ 17.8+5.1 −4.8 per cent to ≈ 13.8+6.5−5.8 per cent (from the lower to the higher redshift bin), but is about twice the bar fraction found using bluer HST filters. Our results show that bar-driven evolution might commence at early cosmic times and that dynamically settled discs are already present at a lookback time of ∼11 Gyr.

Citation

Le Conte, Z. A., Gadotti, D. A., Ferreira, L., Conselice, C. J., de Sá-Freitas, C., Kim, T., …Adams, N. J. (2024). A JWST investigation into the bar fraction at redshifts 1 ≤ z ≤ 3. Monthly Notices of the Royal Astronomical Society, 530(2), 1984-2000. https://doi.org/10.1093/mnras/stae921

Journal Article Type Article
Acceptance Date Mar 28, 2024
Online Publication Date Apr 23, 2024
Publication Date 2024-05
Deposit Date May 9, 2024
Publicly Available Date May 9, 2024
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 530
Issue 2
Pages 1984-2000
DOI https://doi.org/10.1093/mnras/stae921
Public URL https://durham-repository.worktribe.com/output/2435932

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