SIMBAD references

We present various time series analysis methods to analyse multiple-sector observations of bright active galactic nucleus from the Transiting Exoplanet Survey Satellite (TESS) and examine whether issues such as gaps and noise in these data can be mitigated. We determine variability time-scales and search for quasi-periodicity using these methods and assess any differences. In this paper, we present an analysis of the $\approx$ 300-d TESS observation of a blazar 3C 371 using power spectrum density, structure-function, and weighted wavelet Z-transform approaches. To reduce the effect of gaps and noise, Continuous auto-regressive moving averages, Bartlett periodogram, and wavelet decomposition methods are used. We have also used recurrence analysis to account for the non-linearity present in the data and to quantify variability or periodicity as the recurrent state. Considering the entirety of the TESS observations, we derive the variability time-scale to be around 4.5 d. Sector-wise analysis found variability time-scales in the range of 3.0-7.0 d, values that are found to be consistent using different methods. When analysing multiple sectors together, significant variability, which could be quasi-periodic oscillations, of duration 3-6 d in individual segments, is detected. These may be attributed to the kink instabilities developed in the jet or the existence of mini-jets inside a jet undergoing precession. We find that these methods, when applied appropriately, can be used to study the variability in TESS data. The noise present in these TESS observations can be minimized using Bartlett's periodogram and wavelet decomposition to recover the real stochastic variability.