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. Note, Gt-n-propanol) ground state present in the spectral scan of Orion KL from the IRAM-30 m telescope and the ALMA interferometer. Column 1 indicates the species, Column 2 gives the transition, Column 3 the predicted frequency, Column 4 upper level energy, Column 5 the line strength, Column 6 observed frequency at the peak channel of the line (relative to a v LS R of +8.0 km s ?1, Col. 7 temperature at the peak channel of the line (main beam temperature for the IRAM data), and Column 8 shows blends with other molecular species and comments