arXiv2018
We have reinvestigated the A$^1Π$$(v=0)$ level of $^{13}$C$^{18}$O\ using new high-resolution spectra obtained via multi-photon laser excitation as well as with synchrotron-based Fourier-transform absorption spectroscopy of the A$^1Π-\textrm{X}^1Σ^+$$(0, 0)$, e$^3Σ^--\textrm{X}^1Σ^+$$(1, 0)$, d$^3Δ-\textrm{X}^1Σ^+$$(4, 0)$, a$'^3Σ^+-\textrm{X}^1Σ^+$$(9, 0)$, and \atX$(11, 0)$ bands. In addition, Fourier-transform emission spectroscopy in the visible range is performed on the ${\rm B}^1Σ^+-{\rm A}^1Π$$(0, 0)$ band. Spectra of the \BX$(0, 0)$ band are measured in order to tie information from the latter emission data to the level structure of A$^1Π$$(v=0)$. The high pressures in the absorption cell at the synchrotron and the high temperatures in the emission discharge permitted monitoring of high rotational quantum levels in A$^1Π$$(v=0)$ up to $J=43$. All information, in total over 900 spectral lines, was included in an effective-Hamiltonian analysis of the A$^1Π(v=0, J)$ levels that are directly perturbed by the e$\,^3Σ^-$$(v=1)$, d$^3\!Δ$$(v=4)$, a$'^3Σ^+$$(v=9)$, d$^3\!Δ$$(v=0)$, I$\,^1Σ^-$$(v=0, 1)$ close-lying levels and the e$\,^3Σ^-$$(v=0,2)$, d$^3\!Δ$$(v=3,5)$, a$'^3Σ^+$$(v=8,10)$ remote levels, as well being indirectly influenced by the a$^3Π$$(v=10, 11)$ state. The influence of nine further perturber levels and their interactions was investigated and are not significant for reproducing the present experimental data. This analysis leads to a much improved description in terms of molecular constants and interaction parameters, compared to previous studies of the same energy region for other CO isotopologues.