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Preprint Sep 2026

From stardust to interstellar grain growth in the first galaxies: a cosmological transition in dust evolution near z ~ 8.9

When and how did dust begin to shape galaxies? Motivated by the identification of an apparent redshift break in galaxy dust masses, suggesting substantially lower dust masses at $z \gtrsim 9$, we investigate dust enrichment during the first billion years of cosmic history. We aim to determine whether the observed evolu...

D. Burgarella, T. Bakx, Raffaella Schneider et al. · 0 citations
Review Oct 2026

Dust at cosmic dawn: unveiling the onset of dust and obscured star formation at $z\gtrsim8$

Although less than 1 percent of the baryonic mass budget of a galaxy, cosmic dust profoundly alters the multi-wavelength appearance of galaxies across cosmic time. The (sub)millimeter wavelength regime is uniquely capable of weighing these dust reservoirs, and revealing the total extent of galaxy evolution that remains...

H. Algera, T. Bakx, M. Aravena et al. · 0 citations
Review Open access Dec 2025

How much gas and dust is in the z=5.7 Lyman-break galaxy HZ10? ALMA Bands 10 to 4 and JWST/NIRSpec study of its interstellar medium

A complete overview of the stellar, gas and dust contents of galaxies is key to understanding their assembly at early times. However, an estimation of molecular and atomic gas reservoirs at high redshift relies on various indirect tracers, while robust dust mass measurements require multiband far-infrared continuum obs...

H. Algera, R. Herrera-Camus, M. Aravena et al. · 0 citations

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