Two years of multiwavelength monitoring separate the accretion disk and jet emission of the high-redshift blazar 4C 71.07, yielding extreme disk and jet luminosities and a black hole mass of about 1.6 billion solar masses.
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The beamed jet and quasar core of the distant blazar 4C 71.07
Two years of multiwavelength monitoring separate the accretion disk and jet emission of the high-redshift blazar 4C 71.07, yielding extreme disk and jet luminosities and a black hole mass of about 1.6 billion solar masses.