arXiv (All)
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NOEMA probes the [CII] and dust content in a 2175Å UV Bump Galaxy at $z=7.1$
The detection of the $2175$Å UV bump at $z>6$ challenges existing models of dust formation, suggesting rapid formation of small carbonaceous dust grains within the first billion years of cosmic time. We present the results of the first direct attempt at linking far-infrared (FIR) observations to the
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