A population of red candidate massive galaxies ~600 Myr after the Big Bang-Reference-Cited by-同舟云学术

A population of red candidate massive galaxies ~600 Myr after the Big Bang

Published:2023-02-22 Issue:7956 Volume:616 Page:266-269
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Labbé Ivo^ORCID,van Dokkum Pieter^ORCID,Nelson Erica^ORCID,Bezanson Rachel^ORCID,Suess Katherine A.^ORCID,Leja Joel^ORCID,Brammer Gabriel^ORCID,Whitaker Katherine^ORCID,Mathews Elijah,Stefanon Mauro,Wang Bingjie^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

https://www.nature.com/articles/s41586-023-05786-2.pdf

Reference65 articles.

1. Glazebrook, K. et al. A massive, quiescent galaxy at a redshift of 3.717. Nature 544, 71–74 (2017).

2. Riechers, D. A. et al. Rise of the Titans: gas excitation and feedback in a binary hyperluminous dusty starburst galaxy at z ~ 6. Astrophys. J. 907, 62 (2021).

3. Stefanon, M. et al. Galaxy stellar mass functions from z ~ 10 to z ~ 6 using the deepest Spitzer/infrared array camera data: no significant evolution in the stellar-to-halo mass ratio of galaxies in the first gigayear of cosmic time. Astrophys. J. 922, 29 (2021).

4. Brammer, G. & Matharu, J. gbrammer/grizli: Release 2021. Zenodo https://zenodo.org/record/7767790#.ZCRGM-zMJxY (2021).

5. Schaerer, D. & de Barros, S. The impact of nebular emission on the ages of z ≈ 6 galaxies. Astron. Astrophys. 502, 423–426 (2009).

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