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Despite the ever-growing number of exoplanets discovered and the extensiveanalyses carried out to find their potential satellites, only two exomooncandidates, Kepler-1625b-i and Kepler-1708 b-i, have been discovered to date. Aconsiderable amount of effort has been invested in the development ofalgorithms for modelling, searching, and detecting exomoons in exoplanetarylight curves. In this work, we incorporate moon handling capabilities into thestate-of-the-art and publicly available code, the Transit and Light CurveModeller (TLCM). The code is designed for the analysis of transiting exoplanetsystems with the inclusion of a wavelet-based noise handling algorithm. Here wepresent an updated version of TLCM that is capable of modelling a coplanarplanet-moon system on an elliptical orbit around its host, accounting formutual eclipses between the two bodies (and neglecting perturbative effects) --a so-called photodynamic model. The key benefit of this framework is theability for a joint analysis of multiple planet-moon transits. We demonstratethe necessity of this software on a case study of Kepler-1625b. Similarly toprior works, we conclude that there is no firm evidence of an exomoon in thatsystem, by showing that temporally correlated noise can mimic apparent lunartransits.

Modelling the Light Curves of Transiting Exomoons: a Zero-order Photodynamic Agent Added to the Transit and Light Curve Modeller