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Nigro, C. Righi, D. Baack, D. Dominis Prester, D. Dorner, D. Elsaesser, D. Fidalgo, D. Galindo, D. Green, D. Guberman, D. Hadasch, D. Hrupec, D. Lelas, D. Mazin, D. Miceli, D. Morcuende, D. Ninci, D. Paneque, D. Sobczynska, D. Strom, D. Zari\\'c, E. Bernardini, E. Colombo, E. Do Souto Espi\\~neira, E. Lindfors, E. Molina, E. Moretti, E. Prandini, F. Dazzi, F. Di Pierro, F. Leone, F. Longo, F. Tavecchio, G. Bonnoli, G. Busetto, G. Ceribella, G. Ferrara, G. Maneva, G. Vanzo, H. Kubo, I. Puljak, I. Vovk, I. \\v{S}nidari\\'c, J. A. Barrio, J. Becerra Gonz\\'alez, J. Besenrieder, J. Cortina, J. Delgado, J. Herrera, J. Hoang, J. Kushida, J. L. Contreras, J. M. Miranda, J. M. Paredes, J. Palacio, J. Rico, J. Sitarek, J. van Scherpenberg, K. Ishio, K. Mannheim, K. Nilsson, K. Nishijima, K. Noda, K. Satalecka, L. A. Antonelli, L. Bellizzi, L. Foffano, L. Font, L. Maraschi, L. Nogu\\'es, L. Saha, MAGIC collaboration: V. A. Acciari, M. Delfino, M. Doro, M. Garczarczyk, M. Gaug, M. L\\'opez, M. Makariev, M. Mallamaci, M. Manganaro, M. Mariotti, M. Mart\\'inez, M. Minev, M. Nievas Rosillo, M. N\\\"othe, M. Palatiello, M. Peresano, M. Persic, M. Rib\\'o, M. Strzys, M. Teshima, M. V\\'azquez Acosta, M. V. Fonseca, M. Will, N. Godinovi\\'c, N. Sahakyan, N. Torres-Alba, O. Blanch, P. Da Vela, P. G. Prada Moroni, P. Majumdar, P. Munar-Adrover, P. Pe\\~nil, P. Temnikov, R. Carosi, R. J. Garc\\'ia L\\'opez, R. L\\'opez-Coto, R. Mirzoyan, R. Paoletti, S. Ansoldi, S. Cikota, S. Covino, S. Gallozzi, S. Gasparyan, S. Inoue, S. Lombardi, S. Masuda, S. M. \\c{C}olak, S. Mi\\'canovi\\'c, S. Paiano, S. Tsujimoto, T. Hassan, T. Saito, T. Schweizer, T. Suri\\'c, T. Terzi\\'c, U. Barres de Almeida, U. Colin, V. D'Elia, V. Fallah Ramazani, V. Moreno, V. Neustroev, W. Bednarek, W. Bhattacharyya, W. Rhode, Y. Chai, Y. Iwamura","submitted_at":"2019-03-30T01:59:36Z","abstract_excerpt":"We present a measurement of the extragalactic background light (EBL) based on a joint likelihood analysis of 32 gamma-ray spectra for 12 blazars in the redshift range z = 0.03 to 0.944, obtained by the MAGIC telescopes and Fermi-LAT. The EBL is the part of the diffuse extragalactic radiation spanning the ultraviolet, visible and infrared bands. Major contributors to the EBL are the light emitted by stars through the history of the universe, and the fraction of it which was absorbed by dust in galaxies and re-emitted at longer wavelengths. 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