The Large Interferometer For Exoplanets (LIFE) is a proposed space-based mid-infrared nulling interferometer featuring an array of formation-flying collectors and a central beam combiner. Its primary objective is the direct detection of dozens of temperate, terrestrial exoplanets and the investigation of their atmospheres to understand their composition and identify potential biosignatures. To get a realistic performance estimate of LIFE and derive technical requirements, a comprehensive understanding of all major noise sources impacting the mission performance is essential. Previous studies on the performance of LIFE have focused on fundamental noise from astrophysical sources and assumed the impact of instrumental noise to be non-dominant. Here, we report on our ongoing effort to explicitly model instrumental noise for LIFE. We consider two different methods: one providing a numerical solution by explicitly propagating the instability-induced errors in Monte Carlo simulations, and one providing an analytical solution using a second-order approximation of the leakage from instrumental instability noise. We give an overview of the two methods and argue in favor of the numerical method to support the efforts of the LIFE initiative in the ongoing concept phase, due to its flexibility for different observatory architectures, its fidelity in modeling the correlation of errors and fewer limitations concerning the parameter space of potential errors sources.
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