Unveiling dust, molecular gas, and high star-formation efficiency in extremely UV bright star-forming galaxies at z ∼ 2.1–3.6
We analysed the Atacama Large Millimetre/submillimetre Array (ALMA) far-infrared (FIR), 1.3 mm, dust continuum and CO emission of 12 starburst galaxies at z ∼ 2.1 ‑ 3.6 selected for their extreme brightness in the rest-frame UV, with absolute magnitudes of ‑23.4 to ‑24.7. We also analysed their Very Large Telescope (VLT) High Acuity Wide field K
Dessauges-Zavadsky, M. et al.
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2025