Frey, S. (author), Zhang, Y. (author), Perger, K. (author), An, T. (author), Gabányi, K. (author), Gurvits, L. (author), Hwang, C. Y. (author), Koptelova, E. (author), Paragi, Z. (author), Fogasy, J. (author) Context. The existence of accreting supermassive black holes of up to billions of solar masses at early cosmological epochs (in the context of this work, redshifts z & 6) requires very fast growth rates that are challenging to explain. The presence of a relativistic jet can be a direct indication of activity and accretion status in active...
journal article 2024