Long-term photometric follow-up of TOI-2095 from ZTF (z band) and TJO (R band). Left panels: photometric time-series and joint best fitted model computed using GP adopting a quasi-periodic kernel (black line). The 1σ uncertainty regions of the fit are shown in light blue. The residuals of the fit are shown at the bottom panels. Right panels: GLS periodogram (Zechmeister & Kürster 2009) for each photometric data set. The vertical green line shows the fitted rotational period of the star. The horizontal lines represent the FAP levels of 10% (red dotted line) and 1% (blue dashed line).