Fig. 2.
Observation of UVES on March 19, 2008 example. The linear line is fitted using P1(2.5), P1(3.5), and P1(5.5) line intensities in the OH(8-3) band. The P1(4.5) emission line without absorption by water vapor is indicated with an asterisk. The error bars are the uncertainties of intensities, which are estimated by the S/N given in the UVES dataset.
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