| Title: |
RUBIES Spectroscopically Confirms the High Number Density of Quiescent Galaxies from 2 < z< 5 |
| Authors: |
Yunchong Zhang; Anna de Graaff; David J. Setton; Sedona H. Price; Rachel Bezanson; Claudia del P. Lagos; Sam E. Cutler; Ian McConachie; Nikko J. Cleri; Olivia R. Cooper; Rashmi Gottumukkala; Jenny E. Greene; Michaela Hirschmann; Gourav Khullar; Ivo Labbe; Joel Leja; Michael V. Maseda; Jorryt Matthee; Tim B. Miller; Themiya Nanayakkara; Katherine A. Suess; Bingjie Wang; Katherine E. Whitaker; Christina C. Williams |
| Source: |
The Astrophysical Journal, Vol 997, Iss 2, p 252 (2026) |
| Publisher Information: |
IOP Publishing |
| Publication Year: |
2026 |
| Collection: |
Directory of Open Access Journals: DOAJ Articles |
| Subject Terms: |
Extragalactic astronomy; Galaxies; High-redshift galaxies; Quenched galaxies; Astrophysics; QB460-466 |
| Description: |
We present the number density of massive ( ${\mathrm{log}}({M}_{* }/{M}_{\odot })\gt 10.3$ ) quiescent galaxies at 2 < z < 5 using JWST NIRSpec PRISM spectra. This work relies on spectra from RUBIES, which provides excellent data quality and an unparalleled, well-defined targeting strategy to robustly infer physical properties and number densities. We identify quiescent galaxy candidates within RUBIES through principal component analysis and construct a final sample using star formation histories derived from spectrophotometric fitting of the NIRSpec PRISM spectra and NIRCam photometry. By inverting the RUBIES selection function, we correct for survey incompleteness and calculate the number density of massive quiescent galaxies at these redshifts, providing the most complete spectroscopic estimates prior to cosmic noon to date. We find that early massive quiescent galaxies are surprisingly common (≳10 ^−5 Mpc ^−3 by 4 < z < 5), which is consistent with previous studies based on JWST photometry alone and/or in smaller survey areas. We compare our number densities with predictions from six state-of-the-art cosmological galaxy formation simulations. At z > 3, most simulations fail to produce enough massive quiescent galaxies, suggesting the treatment of feedback and/or the channels for early efficient formation are incomplete in most galaxy evolution models. |
| Document Type: |
article in journal/newspaper |
| Language: |
English |
| Relation: |
https://doi.org/10.3847/1538-4357/ae24e1; https://doaj.org/toc/1538-4357; https://doaj.org/article/9380886f2687443cadf301e3aa754047 |
| DOI: |
10.3847/1538-4357/ae24e1 |
| Availability: |
https://doi.org/10.3847/1538-4357/ae24e1; https://doaj.org/article/9380886f2687443cadf301e3aa754047 |
| Accession Number: |
edsbas.CC20E6C2 |
| Database: |
BASE |