A NEW NETWORK FOR HIGHER-TEMPERATURE GAS-PHASE CHEMISTRY. I. A PRELIMINARY STUDY OF ACCRETION DISKS IN ACTIVE GALACTIC NUCLEI

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A KINETIC DATABASE FOR ASTROCHEMISTRY (KIDA) (2012, background): “For higher temperatures, one should adapt an expanded gas-phase network developed by Harada et al. (2010), which can be utilized up to gas temperatures of 800 K.”
Detection of HCN, HCO+, and HNC in the Mrk 231 molecular outflow. Dense molecular gas in the AGN wind (2011, background): “Harada et al. (2010) have shown that HCN abundances may reach 10−6 in regions whereT >∼ 300 K.”
THE 2014 KIDA NETWORK FOR INTERSTELLAR CHEMISTRY (2015, background): “Despite the fact that we added reactions from Harada et al. (2010) for higher temperature conditions, including reactions with activation energy, and reverse reactions, we have not done any additional checks on its appropriateness for temperatures larger than 300 K.”
H$_2$ formation on interstellar dust grains: the viewpoints of theory, experiments, models and observations (2017, background): “The H 2 formation rate however determines the abundance of atomic hydrogen, which is involved in many destruction reactions with activation barriers ( Harada et al., 2010 ).”
Complex organic molecules in protoplanetary disks (2013, methodology): “To render the network suitable for protoplanetary disk chemistry, we have added reactions and rate coefficients applicable at higher temperatures (Harada et al. 2010, 2012).”