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Fig. 3


Data, model and residuals for patch q = 208 of the LPC camera during the 2016-10-A baseline. For clarity only the night of 2016-10-08 is shown and the median of the residual rows has been subtracted from all panels, removing small normalization differences due to keeping the mi fixed. Panel a: photometric time-series for the stars in patch q = 208 during the night of 2016-10-08 as a function of local sidereal time after subtracting the transmission and intrapixel corrections Tnk and f(xit, yit). For clarity the mean magnitude mi has also been removed. Panel b: the atmospheric corrections cqt obtained from solving Eq. (2). Panel c: the residuals after subtracting the atmospheric corrections.

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