molecules:ism:inden

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molecules:ism:inden [2021/05/27 11:12] muellermolecules:ism:inden [2021/05/27 11:14] (current) mueller
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 submitted a report somewhat earlier but that appeared later on the\\ submitted a report somewhat earlier but that appeared later on the\\
 **[[https://doi.org/10.3847/2041-8213/abfd3a|Discovery of the pure polycyclic aromatic hydrocarbon indene (//c//-C<sub>9</sub>H<sub>8</sub>) with GOTHAM observations of TMC-1]]**\\ **[[https://doi.org/10.3847/2041-8213/abfd3a|Discovery of the pure polycyclic aromatic hydrocarbon indene (//c//-C<sub>9</sub>H<sub>8</sub>) with GOTHAM observations of TMC-1]]**\\
-//Astrophys. J. Lett.// ** **, (2021), in press.\\ +//Astrophys. J. Lett.// **913**, Art. No. L18 (2021).\\ 
-The observations were obtained in the course of the line survey Green Bank Telescope Observations of TMC-1: Hunting for Aromatic Molecules. The data were recorded with very high resolution which resolves, at least in part, the complex velocity structure . No individual lines were detected, as usually in this survey. Stacking of all lines of all four major velocity components, however, yielded a signal slighly above 5σ. Note, however, that this method becomes questionable with weak lines as those of indene. As can be seen in Fig. 4 of the previous paper, TMC-1 is not line poor anymore at 1 cm wavelength on the level of the indene lines; the situation **may** be slightly better at longer wavelengths.+The observations were obtained in the course of the line survey Green Bank Telescope Observations of TMC-1: Hunting for Aromatic Molecules. The data were recorded with very high resolution which resolves, at least in part, the complex velocity structure . No individual lines were detected, as usually in this survey. Stacking of all lines of all four major velocity components, however, yielded a signal slighly above 5σ. Note, however, that this method becomes questionable with weak lines as those of indene. As can be seen in Fig. 4 of the previous paper, TMC-1 is not line poor anymore at 1 cm wavelength on the level of the indene lines; the situation **may** be slightly better at longer wavelengths. The derived column densities of the two reports agree.\\
  
  
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