All the files are provided as .cti files, which can be directly read by Cantera, 
a chemical kinetic software. http://www.cantera.org/docs/sphinx/html/index.html

Each .cti files contains:
(1) a list of species
(2) NASA polynomial of all the species
(3) temperature dependent reaction coefficients

CNOH_reaction_network.cti : modified based on the Venot et al. (2012) network. 
P_Reaction_Set.cti : modified P/H/O reaction network based on the Twaroski (1995) network.
my_silane_v2.cti : modifed Si/H/O reaction network based on the Miller et al. (2004) network. 

P_Reaction_Set_Simlified.cti : simplified P/H/O reaction network for hydrogen rich environment. 
my_silane_v2_simplified.cti : simplied Si/H/O reaction network for hydrogen rich environment.  


References: 
(1) Venot, O., He ́brard, E., Agu ́ndez, M., Dobrijevic, M., Selsis, F., Hersant, F., Iro, N., Bounaceur, R., Oct. 2012. A chemical model for the atmosphere
of hot Jupiters. A&A546, A43.

(2) Twarowski, A., 1995. Reduction of a phosphorus oxide and acid reaction set. Combustion and flame 102 (1), 41–54.

(3) Miller, T., Wooldridge, M., Bozzelli, J., 2004. Computational modeling of the sih 3+ o 2 reaction and silane combustion. Combustion and flame
137 (1), 73–92.

(4) Wang, D., Lunine, J., Mousis, O., 2016. Modeling the disequilibrium species for Jupiter and Saturn: Implications for Juno and Saturn entry probe, Icarus, submitted. 
 