Application of Convolutional Neural Networks to time domain astrophysics. 2D image analysis of OGLE light curves

Open Access

Fig. 3

Examples of DA for CEP, DST, and ELL are shown. The first column represents the original LC, while the other columns represent different modifications of the LC. At the top of each image, we display the fraction of the total number of observation $(n_{o b s}^{'})$ $\[\left(n_{o b s}^{\prime}\right)\]$ , and the offset in phase (ϕ′).

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