Larry D. Bradley
High-redshift Galaxy Candidates at z = 9–10 as Revealed by JWST Observations of WHL0137-08
Bradley, Larry D.; Coe, Dan; Brammer, Gabriel; Furtak, Lukas J.; Larson, Rebecca L.; Kokorev, Vasily; Andrade-Santos, Felipe; Bhatawdekar, Rachana; Bradač, Maruša; Broadhurst, Tom; Carnall, Adam; Conselice, Christopher J.; Diego, Jose M.; Frye, Brenda; Fujimoto, Seiji; Hsiao, Tiger Y.-Y; Hutchison, Taylor A.; Jung, Intae; Mahler, Guillaume; McCandliss, Stephan; Oguri, Masamune; Postman, Marc; Sharon, Keren; Trenti, M.; Vanzella, Eros; Welch, Brian; Windhorst, Rogier A.; Zitrin, Adi
Authors
Dan Coe
Gabriel Brammer
Lukas J. Furtak
Rebecca L. Larson
Vasily Kokorev
Felipe Andrade-Santos
Rachana Bhatawdekar
Maruša Bradač
Tom Broadhurst
Adam Carnall
Christopher J. Conselice
Jose M. Diego
Brenda Frye
Seiji Fujimoto
Tiger Y.-Y Hsiao
Taylor A. Hutchison
Intae Jung
Dr Guillaume Mahler guillaume.mahler@durham.ac.uk
Academic Visitor
Stephan McCandliss
Masamune Oguri
Marc Postman
Keren Sharon
M. Trenti
Eros Vanzella
Brian Welch
Rogier A. Windhorst
Adi Zitrin
Citation
Bradley, L. D., Coe, D., Brammer, G., Furtak, L. J., Larson, R. L., Kokorev, V., …Zitrin, A. (2023). High-redshift Galaxy Candidates at z = 9–10 as Revealed by JWST Observations of WHL0137-08. Astrophysical Journal, 955(1), Article 13. https://doi.org/10.3847/1538-4357/acecfe
| Journal Article Type | Article |
|---|---|
| Acceptance Date | Aug 1, 2023 |
| Online Publication Date | Sep 12, 2023 |
| Publication Date | Sep 12, 2023 |
| Deposit Date | Feb 26, 2024 |
| Publicly Available Date | Feb 26, 2024 |
| Journal | The Astrophysical Journal |
| Print ISSN | 0004-637X |
| Electronic ISSN | 1538-4357 |
| Publisher | American Astronomical Society |
| Peer Reviewed | Peer Reviewed |
| Volume | 955 |
| Issue | 1 |
| Article Number | 13 |
| DOI | https://doi.org/10.3847/1538-4357/acecfe |
| Keywords | Space and Planetary Science; Astronomy and Astrophysics |
| Public URL | https://durham-repository.worktribe.com/output/2286787 |
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Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
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