Machine learning applications in studies of the physical properties of active galactic nuclei based on photometric observations

Open Access

Fig. 11

W1–W2 magnitudes as a function of W2–W3 magnitudes for sources in the training sample with low (red dots) and high (blue dots) λ_Edd, The low and high samples are separated by the median value of the λ_Edd distribution, 0.1.

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