Massive galaxy formation caught in action at z ∼ 5 with JWST

Shuowen Jin*, Nikolaj B. Sillassen, Georgios E. Magdis, Aswin P. Vijayan, Gabriel B. Brammer, Vasily Kokorev, John R. Weaver, Raphael Gobat, Clara Giménez-Arteaga, Francesco Valentino, Malte Brinch, Carlos Gómez-Guijarro, Marko Shuntov, Sune Toft, Thomas R. Greve, David Blanquez Sese

*Corresponding author for this work

Research output: Contribution to journalJournal articleResearchpeer-review

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Abstract

We report the discovery of a compact group of galaxies, CGG-z5, at z ∼ 5.2 in the EGS field covered by the JWST/CEERS survey. CGG-z5 was selected as the highest overdensity of galaxies at z >  2 in recent JWST public surveys and it consists of six candidate members lying within a projected area of 1.5″ × 3″ (10×20 kpc2). All group members are HST/F435W and HST/F606W dropouts while securely detected in the JWST/NIRCam bands, yielding a narrow range of robust photometric redshifts 5.0 <  z <  5.3. The most massive galaxy in the group has a stellar mass log(M*/M)≈9.8, while the rest are low-mass satellites (log(M*/M)≈8.4–9.2). While several group members were already detected in the HST and IRAC bands, the low stellar masses and the compactness of the structure required the sensitivity and resolution of JWST for its identification. To assess the nature and evolutionary path of CGG-z5, we searched for similar compact structures in the EAGLE simulations and followed their evolution with time. We find that all the identified structures merge into a single galaxy by z = 3 and form a massive galaxy (log(M*/M)> 11) at z ∼ 1. This implies that CGG-z5 could be a “proto-massive galaxy” captured during a short-lived phase of massive galaxy formation.
Original languageEnglish
Article numberL11
JournalAstronomy and Astrophysics
Volume670
Number of pages8
ISSN0004-6361
DOIs
Publication statusPublished - 2023

Keywords

  • Galaxies: groups: individual: CGG-z5
  • Galaxies: high-redshift
  • Galaxy: evolution
  • Galaxy: formation
  • Infrared: galaxies

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