“…The procedures employed needed the knowledge of the axial rotational constant C 0 of both parent species; however, C 0 for SD 3 þ was determined at low precision by IR spectroscopy [16], therefore it has been followed the method suggested by Halonen and Mills [32] to derive its value from the rotational constants of the asymmetric species SHD 2 þ . First, the moments of inertia I a z , I b z , I c z , which are corrected for the harmonic part of the contribution of zero-point vibrations (see Section 3.3), were calculated for SHD 2 þ , then the relation…”