{
  "id": "2211.00850",
  "version": "v1",
  "published": "2022-11-02T03:40:23.000Z",
  "updated": "2022-11-02T03:40:23.000Z",
  "title": "The dust properties of star-forming galaxies in the first billion years",
  "authors": [
    "Elisabete da Cunha"
  ],
  "comment": "10 pages, 5 figures; invited review to appear in the Proceedings of IAU Symposium 373 - Resolving the rise and fall of star formation in galaxies",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "The Atacama Large Millimetre/Sub-millimetre Array (ALMA) is obtaining the deepest observations of early galaxies ever achieved at (sub-)millimetre wavelengths, and detecting the dust emission of young galaxies in the first billion years of cosmic history, well in the epoch of reionization. Here I review some of the latest results from these observations, with special focus on the REBELS large programme, which targets a sample of 40 star-forming galaxies at z~7. ALMA detects significant amounts of dust in very young galaxies, and this dust might have different properties to dust in lower-redshift galaxies. I describe the evidence for this, and discuss theoretical/modelling efforts to explain the dust properties of these young galaxies. Finally, I describe two additional surprising results to come out of the REBELS survey: (i) a new population of completely dust-obscured galaxies at z~7, and (ii) the prevalence of spatial offsets between the ultraviolet and infrared emission of UV-bright, high-redshift star-forming galaxies.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2022-11-02T03:40:23.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "dust properties",
      "first billion",
      "young galaxies",
      "atacama large millimetre/sub-millimetre array",
      "alma detects significant amounts"
    ],
    "tags": [
      "review article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}