The reliability of [CII] as a SFR indicator Ilse De Looze, Suzanne Madden, Vianney Lebouteiller, Diane Cormier, Frédéric Galliano, Aurély Rémy, Maarten.
Stratospheric Terahertz Observatory (STO) 0.8-meter telescope, 1' resolution @158 um Heterodyne receiver arrays for wide-field [N II] and [C II] spectroscopy,
C + As a Primary Coolant and Tracer of Star Formation Dec 21 st, 2012.
VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/F TIR Similar gas properties in arm and interarm regions. Higher densities and stronger.
VNGS science highlight: PDR models of M51
C + As a Primary Coolant and Tracer of Star Formation
![The reliability of [CII] as a SFR indicator Ilse De Looze, Suzanne Madden, Vianney Lebouteiller, Diane Cormier, Frédéric Galliano, Aurély Rémy, Maarten.](https://static.fdocuments.in/doc/330x215/56649f425503460f94c61cf0/the-reliability-of-cii-as-a-sfr-indicator-ilse-de-looze-suzanne-madden.jpg)
![Stratospheric Terahertz Observatory (STO) 0.8-meter telescope, 1' resolution @158 um Heterodyne receiver arrays for wide-field [N II] and [C II] spectroscopy,](https://static.fdocuments.in/doc/330x215/56649e2e5503460f94b1f090/stratospheric-terahertz-observatory-sto-08-meter-telescope-1-resolution.jpg)
![VNGS science highlight: PDR models of M51 [CII]/[OI]63 ([CII]+[OI]63)/F TIR Similar gas properties in arm and interarm regions. Higher densities and stronger.](https://static.fdocuments.in/doc/330x215/56649edb5503460f94bea5fd/vngs-science-highlight-pdr-models-of-m51-ciioi63-ciioi63f-tir.jpg)
