4.7 Article

Using [CII] 158 μm Emission from Isolated ISM Phases as a Star Formation Rate Indicator

Journal

ASTROPHYSICAL JOURNAL
Volume 886, Issue 1, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/ab4da5

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Funding

  1. NASA Headquarters under the NASA Earth and Space Science Fellowship Program [80NSSC18K1107]
  2. NASA [NNX15AI08H]

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The brightest observed emission line in many star-forming galaxies is the ?m line, making it detectable up to z;?;7. In order to better understand and quantify the

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