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Modeling Blazar Broadband Emission with a Convolutional Neural Network. I. Synchrotron Self-Compton Model

Authors: D. Bégué, N. Sahakyan, H. Dereli-Bégué, P. Giommi, S. Gasparyan, M. Khachatryan, A. Casotto, A. Pe'er

D. Bégué et al 2024 The Astrophysical Journal 963 .

Caption: Figure 5.

The same SED of 1ES 1959+650 as presented in Figure 4, but fitted with a model where R is constrained by a variability of 35 minutes.