Behind the dust veil: A panchromatic view of an optically dark galaxy at z = 4.82
Journal article, 2025

Optically dark dusty star-forming galaxies (DSFGs) play an essential role in massive galaxy formation at early cosmic time; however, their nature remains elusive. Here, we present a detailed case study of all the baryonic components of a z = 4.821 DSFG, XS55. Selected from the ultra-deep COSMOS-XS 3 GHz map with a red SCUBA-2 450 μm/850 μm colour, XS55 was followed up with ALMA 3 mm line scans and spectroscopically confirmed to be at z = 4.821 via detections of the CO(5-4) and [CI](1-0) lines. JWST/NIRCam imaging reveals that XS55 is a F150W drop-out with a red F277W/F444W colour and a complex morphology: a compact central component embedded in an extended structure with a likely companion. XS55 is tentatively detected in X-rays with both Chandra and XMM-Newton, suggesting an active galactic nucleus nature. By fitting a panchromatic spectral energy distribution spanning from near-infrared to radio wavelengths, we reveal that XS55 is a massive main-sequence galaxy with a stellar mass of M∗ = (5 ± 1)×1010 M⊙ and a star formation rate of SFR = 540 ± 177 M⊙ yr- 1. The dust of XS55 is optically thick in the far-infrared with a surprisingly cold dust temperature of Tdust = 33 ± 2 K, making XS55 one of the coldest DSFGs at z > 4 known to date. This work unveils the nature of a radio-selected F150W drop-out, suggesting the existence of a population of DSFGs hosting active black holes embedded in optically thick dust.

Galaxies: general

Galaxies: ISM

Galaxies: active

Author

Nikolaj B. Sillassen

Technical University of Denmark (DTU)

Cosmic Dawn Center (DAWN)

S. Jin

Technical University of Denmark (DTU)

Cosmic Dawn Center (DAWN)

Georgios E. Magdis

Niels Bohr Institute

Technical University of Denmark (DTU)

Cosmic Dawn Center (DAWN)

J. Hodge

Leiden University

Raphael Gobat

Pontificia Universidad Católica de Valparaíso

Emanuele Daddi

University Paris-Saclay

Kirsten Knudsen

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Alexis Finoguenov

University of Helsinki

E. Schinnerer

Max Planck Society

Wei Hao Wang

Academia Sinica

Zhen Kai Gao

Academia Sinica

J. R. Weaver

University of Massachusetts

H. Algera

National Astronomical Observatory of Japan

Academia Sinica

Hiroshima University

Irham T. Andika

Max Planck Society

Technical University of Munich

Malte Brinch

University of Valparaíso

C. C. Chen

Academia Sinica

R. Cochrane

Columbia University

University of Edinburgh

A. F.M. Enia

Istituto nazionale di astrofisica (INAF)

University of Bologna

A. Faisst

California Institute of Technology (Caltech)

S. Gillman

Cosmic Dawn Center (DAWN)

Technical University of Denmark (DTU)

Carlos Gomez-Guijarro

University Paris-Saclay

Ghassem Gozaliasl

University of Helsinki

Aalto University

Christopher C. Hayward

Flatiron Institute

V. Kokorev

The University of Texas at Austin

Maya Merchant

Cosmic Dawn Center (DAWN)

Niels Bohr Institute

Francesca Rizzo

University of Groningen

Margherita Talia

Istituto nazionale di astrofisica (INAF)

University of Bologna

F. Valentino

Cosmic Dawn Center (DAWN)

Technical University of Denmark (DTU)

David Blánquez-Sesé

Cosmic Dawn Center (DAWN)

Technical University of Denmark (DTU)

Anton M. Koekemoer

Space Telescope Science Institute (STScI)

Benjamin Magnelli

University Paris-Saclay

R. Michael Rich

University of California

Marko Shuntov

Cosmic Dawn Center (DAWN)

Niels Bohr Institute

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 693 A309

The Origin and Fate of Dust in Our Universe

Knut and Alice Wallenberg Foundation (KAW 2019.0443), 2020-06-01 -- 2023-05-31.

Knut and Alice Wallenberg Foundation (KAW 2020.0081), 2021-07-01 -- 2026-06-30.

Subject Categories (SSIF 2025)

Other Physics Topics

Astronomy, Astrophysics, and Cosmology

DOI

10.1051/0004-6361/202452932

More information

Latest update

2/19/2025