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A blazar in the epoch of reionization

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arxiv 2407.07236 v2 pith:PG3ISD5X submitted 2024-07-09 astro-ph.GA astro-ph.HE

classification astro-ph.GAastro-ph.HE
keywords blackblazarj0410-0139jetsquasarsuniverseearlyepoch
verification ladder T0 review T1 audit T2 compute T3 formal
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Relativistic jets are thought to play a crucial role in the formation and evolution of massive galaxies and supermassive black holes. Blazars, which are quasars with jets aligned along our line of sight, provide insights into the jetted population and have been observed up to redshifts of z=6.1. Here, we report the discovery and multi-wavelength characterization of the blazar VLASS J041009.05-013919.88 at z=7 (Universe's age ~750 Myr), powered by a ~7x10^8 Msun black hole. The presence of this high-redshift blazar implies a large population of similar but unaligned jetted sources in the early Universe. Our findings suggest two possible scenarios: in one, the jet in J0410-0139 is intrinsically low-power but appears highly luminous due to relativistic beaming, suggesting that most UV-bright quasars at this redshift host jets. Alternatively, if J0410-0139 represents an intrinsically powerful radio source, there should be hundreds to thousands of radio-quiet quasars at z~7 with properties similar to J0410-0139, a prediction in tension with observed quasar densities based on their UV luminosity function. These results support the hypothesis that rapid black hole growth in the early Universe may be driven by jet-enhanced or obscured super-Eddington accretion, potentially playing a key role in forming massive black holes during the epoch of reionization.

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Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Detection of the cosmological evolution of the Doppler factor for blazars jets

    astro-ph.HE 2025-01 conditional novelty 6.0 of 10

    Blazar jets appear to have Doppler factors that increase with redshift, δ ∝ (1+z)^{0.8-1.1}, implying more numerous high-redshift jetted AGN.

  2. Prospects for measuring neutrino mass with 21-cm forest

    astro-ph.CO 2025-01 conditional novelty 6.0 of 10

    Using an analytic halo model, the authors forecast that 21-cm forest observations with SKA-LOW could constrain the total neutrino mass to about 0.1 eV, potentially distinguishing neutrino mass hierarchies.

  3. The host galaxies of radio-loud quasars at z>5 with ALMA

    astro-ph.GA 2024-11 conditional novelty 6.0 of 10

    New ALMA data on z>5 radio-loud quasars show synchrotron emission contributes roughly 10% to near 100% of the observed 1 mm continuum in at least four hosts, so dust-based star formation and gas masses for such object...

  4. Spectral Energy Distribution Modeling of BL Lacertae During a Large Submillimeter Outburst and Low X-Ray Polarization State

    astro-ph.HE 2024-11 conditional novelty 4.0 of 10

    A two-zone leptonic jet model fits the 2023 broadband SED of BL Lacertae and its SSC-dominated X-rays are consistent with the IXPE low-polarization upper limit.

  5. Multidisciplinary Science in the Multimessenger Era

    astro-ph.HE 2025-02 unverdicted novelty 3.0 of 10

    A community white paper recommending an NNSA-style end-to-end integration of astrophysics, nuclear, plasma, atomic, and computational sciences to maximize return from time-domain and multimessenger facilities.

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