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Cited article:

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A SEARCH FOR C II 158 μm LINE EMISSION IN HCM 6A, A Lyα EMITTER AT z = 6.56

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The reliability of [C ii] as an indicator of the star formation rate

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https://doi.org/10.1111/j.1365-2966.2011.19223.x

Detectability of [Cii] 158 μm Emission from High‐Redshift Galaxies: Predictions for ALMA andSPICA

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The Astrophysical Journal 647 (1) 60 (2006)
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CiiRadiative Cooling of the Diffuse Gas in the Milky Way

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Mid-IR emission of galaxies in the Virgo cluster III. The data

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Astronomy & Astrophysics 406 (3) 867 (2003)
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The [Cii] 158 Micron Line Deficit in Ultraluminous Infrared Galaxies Revisited

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Far‐Infrared Photometry of a Statistical Sample of Late‐Type Virgo Cluster Galaxies

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