Replacing a standard cooling table with an XGBoost model in an NGC300-like isolated galaxy simulation shifts gas temperatures and creates up to 10-20% differences in some C II emission rates.
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The effects of different cooling and heating function models on a simulated analog of NGC300
Replacing a standard cooling table with an XGBoost model in an NGC300-like isolated galaxy simulation shifts gas temperatures and creates up to 10-20% differences in some C II emission rates.