Theoretical investigation of the A¹Π–X¹Σ⁺, B¹Σ⁺–X¹Σ⁺, C¹Σ⁺–X¹Σ⁺, and E¹Π–X¹Σ⁺ transitions of the

The spectrum of carbon monoxide is important for astrophysical media, such as planetary atmospheres, interstellar space, exoplanetary and stellar atmospheres; it also important in plasma physics, laser physics and combustion. Interpreting its spectral signature requires a deep and thorough understanding of its absorption and emission properties. A new accurate spectroscopic model for the ground and electronically-excited states of the CO molecule computed at the aug-cc-pV5Z <i>ab initio</i> CASSCF/MRCI+Q level is reported. Detailed investigation of the A¹Π-X¹Σ⁺, B¹Σ⁺-X¹Σ⁺, C¹Σ⁺-X¹Σ⁺, and E¹Π-X¹Σ⁺ band systems is presented consisting of calculated potential energy curves as well as permanent and transition dipole moment curves. The B¹Σ⁺ and C¹Σ⁺ states are characterized by having multiple avoided crossings which are diabatized to obtain an accurate electronic structure model. The results are validated by comparing our computed spectra with various high-resolution spectroscopy experiments. To the best of our knowledge, this is the first systematic theoretical spectroscopic study of highly excited states of the CO molecule.