The z=4.31 blazar NVSS J151002+570243 is currently accreting at about 2 to 6 percent of the Eddington limit, implying it grew through an earlier super-Eddington phase from a stellar-mass seed.
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NVSS J151002+570243: accretion and spin of a z > 4 Fermi detected blazar
The z=4.31 blazar NVSS J151002+570243 is currently accreting at about 2 to 6 percent of the Eddington limit, implying it grew through an earlier super-Eddington phase from a stellar-mass seed.