Zoe Le Conte zoe.a.le-conte@durham.ac.uk
PGR Student Doctor of Philosophy
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
Authors
Dr Dimitri Gadotti dimitri.a.gadotti@durham.ac.uk
Assistant Professor
Leonardo Ferreira
Christopher J Conselice
Camila de Sá-Freitas
Taehyun Kim
Justus Neumann
Dr Francesca Fragkoudi francesca.fragkoudi@durham.ac.uk
Assistant Professor
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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Copyright Statement
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
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