Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 8.

Parameter posterior distributions for 1ES 1959+650 assuming a variability time of 35 minutes to link the radius and the Doppler boost. Additionally, there exists a large uncertainty on the minimum electron Lorentz factor ﹩{\gamma }_{\min }﹩.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse