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Appendix A: SMA spectra and tables

	Fig. A.1 LSB Spectra (in steps of 500 MHz) of the two hot cores SMA1 (upper) and SMA2 (lower) of NGC 6334I, observed with the Submillimeter Array. Overlaid in red are the XCLASS fits. For more detailed information about each identified spectral line, see Table A.2.
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Appendix B: HIFI fitted curves of all molecules

Examples of selected, fitted spectra for each molecule. In red is the model, in blue are mostly annotations or blended lines. If only few transitions of a molecule are present, they are all shown in the plot. For weeds or molecules with many lines, no quantum numbers are given and only selected frequency ranges over different bands are presented. Heavy blended lines are excluded for simplicity. All intensities are given in units of Kelvin. The quantum numbers refer to upper state – lower state. For absorption lines, this sequence should be read reversed.

The entire observed and simulated spectrum for each HIFI band will be made available online in the CLASS format on the CHESS website (http://www-laog.obs.ujf-grenoble.fr/heberges/hs3f/), as soon as the HIPE 8 reprocessed data are available. Additionally, the modeled spectrum for each molecule (including isotopologues and vibrationally excited states) can be loaded. It should be noticed that for the simulated spectrum of only one molecule, the blending by other molecules is not taken into account. This results in a deviation for the fits of absorption lines when a nearby emission line contributes to the continuum. In XCLASS, at first all the emission components are calculated and then the absorption components.

	Fig. B.1 XCLASS fits of chemical species in the HIFI spectrum of NGC 6334I.
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	Fig. B.2 XCLASS fits of chemical species in the HIFI spectrum of NGC 6334I. continued.
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	Fig. B.2 continued.
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© ESO, 2012