Fig. 3.
Spectra obtained from the line survey observations toward NGC 1068, IC 342, and NGC 253 at 84–88 GHz. A broad feature at ∼86.0 GHz in the spectra of NGC 1068 is caused by the baseline fluctuation.
Spectra obtained from the line survey observations toward NGC 1068, IC 342, and NGC 253 at 84–88 GHz. A broad feature at ∼86.0 GHz in the spectra of NGC 1068 is caused by the baseline fluctuation.
