Fig. 8
Result of the spectral line survey of the high-mass star-forming region Orion KL between 325 to 360 GHz using the myXCLASSFit function. Here, we used 24 molecules in conjunction with 245 isotopologues. In panel a) the whole spectral line survey (back) is shown together with the result of myXCLASSFit function (red). Panels b), c) and d) show fit examples around 332.5 GHz, 338.15 GHz, and 358.0 GHz, respectively.
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