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A TeV-based Determination of the Local Extragalactic Background Light and Its Consistency with Galaxy Counts and Direct Measurements

  • Authors: J. Baxter, A. Domínguez, J. D. Finke, A. Desai, M. Ajello, A. Banerjee, Dieter Hartmann, Vaidehi S. Paliya

J. Baxter et al 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure 6.

Fraction of the EBL that may remain as a diffuse component in three broad wavelength bands, computed as fdiffuse = (Iγ − IIGL)/Iγ from the reconstructed γ-ray EBL intensities (empirical and physical models) and the IGL. Points are shown at the geometric mean wavelength of each band, with small horizontal offsets for clarity.

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