Issue |
A&A
Volume 694, February 2025
|
|
---|---|---|
Article Number | A215 | |
Number of page(s) | 7 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/202452368 | |
Published online | 18 February 2025 |
ALMA observations of super-early galaxies: Attenuation-free model predictions
1
Scuola Normale Superiore, Piazza dei Cavalieri 7, 56126 Pisa, Italy
2
Leiden Observatory, Leiden University, NL-2300 RA Leiden, Netherlands
3
Observatoire de Genève, 1290 Versoix, Switzerland
4
Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, Jagtvej 128, København N DK-2200, Denmark
⋆ Corresponding author; andrea.ferrara@sns.it
Received:
25
September
2024
Accepted:
14
January
2025
The abundance and blue color of the super-early (redshift z > 10) luminous galaxies discovered by the James Webb Space Telescope (JWST) can be explained if radiation-driven outflows have ejected their dust on kiloparsec-scales. To test this hypothesis, we predict the Atacama Large Millimeter Array (ALMA) detectability of this extended dust component. Based on the observed properties of the galaxy, its observed continuum flux at 88 μm, F88, depends on the dust-to-stellar mass ratio, ξd, and on the extent of the dust distribution, rd. When this is applied to the most distant known galaxy, GS-z14-0 at z = 14.32, the fiducial model (ξd = 1/529) predicts F88fid = 14.9 μJy and a dust extent rd = 1.4 kpc. If the galaxy is very dust rich (ξd = 1/40), F88max = 40.1 μJy. These values are lower (F88fid = 9.5 μJy) if the dust is predominantly made of large grains such as those that form in supernova ejecta. Forthcoming ALMA observations might come very close to constraining the fiducial predictions of the outflow-based attenuation-free model. Other super-early galaxies are predicted to be fainter at 88 μm, mostly because their star formation rate is lower than that of GS-z14-0, with fiducial fluxes in the range 2 − 5.2 μJy.
Key words: galaxies: high-redshift
© The Authors 2025
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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