Abstract
The extragalactic background light (EBL), a diffuse photon field in the optical and infrared range, is a record of radiative processes over the universe's history. Spectral measurements of blazars at very high energies (>100 GeV) enable the reconstruction of the spectral energy distribution (SED) of the EBL, as the blazar spectra are modified by redshift- A nd energy-dependent interactions of the gamma-ray photons with the EBL. The spectra of 14 VERITAS-detected blazars are included in a new measurement of the EBL SED that is independent of EBL SED models. The resulting SED covers an EBL wavelength range of 0.56-56 μm, and is in good agreement with lower limits obtained by assuming that the EBL is entirely due to radiation from cataloged galaxies.
| Original language | English |
|---|---|
| Article number | 150 |
| Number of pages | 0 |
| Journal | Astrophysical Journal |
| Volume | 885 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 10 Nov 2019 |
Authors (Note for portal: view the doc link for the full list of authors)
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- Abeysekara, AU;Archer, A;Benbow, W;Bird, R;Brill, A;Brose, R;Buchovecky, M;Calderon-Madera, D;Christiansen, JL;Cui, W;Daniel, MK;Falcone, A;Feng, Q;Fernandez-Alonso, M;Finley, JP;Fortson, L;Furniss, A;Gent, A;Giuri, C;Gueta, O;Hanna, D;Hassan, T;Hervet, O;Holder, J;Hughes, G;Humensky, TB;Johnson, CA;Kaaret, P;Kertzman, M;Kieda, D;Krause, M;Krennrich, F;Kumar, S;Lang, MJ;Maier, G;Moriarty, P;Mukherjee, R;Nievas-Rosillo, M;O'Brien, S;Ong, RA;Pfrang, K;Pohl, M;Prado, RR;Pueschel, E;Quinn, J;Ragan, K;Reynolds, PT;Ribeiro, D;Richards, GT;Roache, E;Rovero, AC;Sadeh, I;Santander, M;Sembroski, GH;Shahinyan, K;Sushch, I;Svraka, T;Weinstein, A;Wells, RM;Wilcox, P;Wilhelm, A;Williams, DA;Williamson, TJ;Zitzer, B
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