Analysis of the isotopologues of CS, CCS, CCCS, HCS+, HCCS+, and H2CS in TMC-1 with the QUIJOTE line survey

Open Access

Fig. 10

Observed transitions of CCC³³S towards TMC-1. The abscissa corresponds to the rest frequency. The ordinate corresponds to the antenna temperature corrected for atmospheric and telescope losses in mK. The derived line parameters are given in Table B.1. The synthetic spectra (red line) are derived from a model with N=6.2x10¹⁰ cm⁻² and T_rot=8 K (see Section 4.4).

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