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Potassium hydroxide (KOH) and sodium hydroxide (NaOH) are expected to occurin the atmospheres of hot rocky super-Earth exoplanets but a lack ofspectroscopic data is hampering their potential detection. Using robustfirst-principles methodologies, comprehensive molecular line lists for KOH andNaOH that are applicable for temperatures up to $T=3500$ K are presented. TheKOH OYT4 line list covers the 0-6000 cm$^{-1}$ (wavelengths $\lambda > 1.67$$\mu$m) range and comprises 38 billion transitions between 7.3 million energylevels with rotational excitation up to $J=255$. The NaOH OYT5 line list coversthe 0 - 9000 cm$^{-1}$ (wavelengths $\lambda > 1.11$ $\mu$m) range and containsalmost 50 billion lines involving 7.9 million molecular states with rotationalexcitation up to $J=206$. The OYT4 and OYT5 line lists are available from theExoMol database at www.exomol.com and should greatly aid the study of hot rockyexoplanets.

ExoMol line lists -- XLI. High-temperature molecular line lists for the alkali metal hydroxides KOH and NaOH