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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 6.

Parameter posterior distributions for Mrk 421 during the multiwavelength campaign of 2009. The contours give, from outward to inward, the 20%, 40%, and 75% confidence regions. Apart from the radius R, all parameters are well constrained.

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