Fig. 16.
Top: standard deviation versus R magnitude for TFA (black dots) and TFAW (red dots) of a set of 6485 TFRM-PSES light curves. Blue line corresponds to the sum of the scintillation, photon, background and read-out noises. Bottom: decrease of the standard deviations for the same set of light curves due to the application of TFAW compared to TFA. Both TFA and TFAW results were obtained using 250 template stars. The red line corresponds to the zero correction level.
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