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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 1.

Reconstructed optical depth τ as a function of γ-ray energy in four redshift bins: top left (0.01 <z <  0.03), top right (0.03 <z <  0.102), bottom left (0.102 <z <  0.4), and bottom right (0.4 < z <  0.95). Blue data points show the results of this work, with vertical error bars indicating 1σ statistical uncertainties and horizontal bars representing the energy binning. Predictions from EBL models are overplotted for comparison: Y. Inoue et al. (2013), A. Franceschini & G. Rodighiero (2017), A. Saldana-Lopez et al. (2021), and J. D. Finke et al. (2022).

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