In this work, we report on the high-resolution infrared spectrum of CCH+ (3Π) recorded in the range 3066-3184 cm-1 by means of leak-out spectroscopy. This spectral range covers the fundamental of the CH stretching mode and a highly excited bending vibrational mode. Based on this data (385 ro-vibrational lines), accurate spectroscopic descriptions of the ground and the two vibrationally excited states of CCH+ were obtained. Besides the band origins, spin-orbit coupling constants, rotational constants, centrifugal distortion constants, and Λ-doubling constants for the ground and excited vibrational states have been derived. This effective Hamiltonian analysis allowed a search for pure rotational lines of CCH+ in its electronic and vibrational ground state using a two-color millimeterwave-infrared scheme. We observed all rotational transitions from J″ = 2 up to J″ = 6 within the Ω = 2 lowest-energy fine-structure component with resolved hyperfine splittings. This data has already guided the first detection of CCH+ in space toward the Orion Bar photodissociation region and has the potential to support further astronomical searches for CCH+ either through radio or infrared spectroscopy, for example, with the James Webb Space Telescope.
Steenbakkers et al. (Mon,) studied this question.