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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 1.

Swift-UVOT+SARA spectral energy distribution of the two high-z sources. The (solid line) power-law templates are fitted for each source with a clearly seen dropout toward the shorter wavelengths. In addition, the (dashed line) galaxy template fits to these objects are presented. The redshift estimates provided by the latter fits suggest z = 1.5 for each source. The details of the fitting method and the inference of these results are described in Sections 4 and 5, respectively.

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