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A Powerful Radio-loud Quasar at the End of Cosmic Reionization

2018/07/06 by Eduardo Bañados, Eduardo Banados, C. L. Carilli +9 · 5 citations
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #COSMIC cancer database #Galaxies: Formation, Evolution, Phenomena #Galaxy #Physics #Quasar #Radio Astronomy Observations and Technology #Redshift #Reionization #astro-ph.GA

paper · pdf · doi:10.3847/2041-8213/aac511

ApJL accepted on May 8, 2018. See the companion paper by Momjian et al

arxiv created 2018/07/06 · openalex publication_date 2018/07/09 · arxiv updated 2018/07/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06

Abstract

Abstract We present the discovery of the radio-loud quasar PSO J352.4034–15.3373 at z = 5.84 ± 0.02. This quasar is the radio brightest source known, by an order of magnitude, at z ∼ 6 with a flux density in the range of 8–100 mJy from 3 GHz to 230 MHz and a radio loudness parameter . This source provides an unprecedented opportunity to study powerful jets and radio-mode feedback at the highest redshifts, and presents the first real chance to probe deep into the neutral intergalactic medium by detecting 21 cm absorption at the end of cosmic reionization.

Citations

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