Figure 2 from New High-z BL Lacs Using the Photometric Method with Swift and SARA

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New High-z BL Lacs Using the Photometric Method with Swift and SARA

Authors: A. Kaur, A. Rau, M. Ajello, A. Domínguez, V. S. Paliya, J. Greiner, D. H. Hartmann, and P. Schady

2018 The Astrophysical Journal 859 80.

Provider: AAS Journals

Caption: Figure 2.

Spectral energy distribution of 3FGL J1155.4-3417 using the 3FGL and 3FHL catalogs. The black line is a power-law fit to the 3FHL data, which is absorbed by the EBL, utilizing Domínguez et al. (2011).

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