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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 .

  • Provider: AAS Journals

Caption: Figure 7.

Parameter posterior distributions for 1ES 1959+650 without imposing a variability constraint. The magnetic field, the electron luminosity, and the electron index are well constrained. In contrast, the other parameters remain somewhat unconstrained due to the high uncertainty in the position of the peak energy of the synchrotron bump.

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