skip to main content

gaia data release 3 documentation

10.13 Solar-like rotational modulation

10.13.3 Calibration models

At first order, rotational modulation light curves can be modelled with a simple sinusoidal function. If a significant period P is detected in one of the time series segments defined in Section 10.13.4, then the model

m⁢(t)=am+bm⁢cos⁡(2⁢π⁢tP)+cm⁢sin⁡(2⁢π⁢tP) (10.16)

is fitted to each of the m∈(G,GBP,GRP) time series segments. This produces model coefficients am, bm, and cm for each segment in which a significant period is detected.