“…To make the thermodynamic calculation manageable, the species coexisting in the equilibrium CLSR system were determined by considering the following rules: (I) the proportion of the atoms in the system, (II) the Gibbs free energy of formation of the compound and (III) previous experience with similar systems [18,19]. At the initial stage, the equilibrium calculations were performed with typical compositions including H 2 , CO, CO 2 , H 2 O, CH 4 , C 2 H 2 , C 2 H 5 , C 2 H 4 , C 2 H 6 , C 3 H 8 , C 3 H 6 , C 3 H 8 O 3 , C 4 H 6 , C 4 H 8 , CH 2 O, CH 3 OH, CH 3 HCO, NH 3 , NH 2 , and N 2 .…”