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- W2856779319 abstract "We present high angular resolution imaging (23.9 × 11.3 mas, 138.6 × 65.5 pc) of the radio-loud quasar PSO J352.4034−15.3373 at z = 5.84 with the Very Long Baseline Array (VLBA) at 1.54 GHz. This quasar has the highest radio-to-optical flux density ratio at such a redshift, making it the radio-loudest source known to date at z ∼ 6. The VLBA observations presented here resolve this quasar into multiple components with an overall linear extent of 1.62 kpc (028) and with a total flux density of 6.57 ± 0.38 mJy, which is about half of the emission measured at a much lower angular resolution. The morphology of the source is comparable with either a radio core with a one-sided jet or a compact or a medium-size symmetric object (CSO/MSO). If the source is a CSO/MSO, and assuming an advance speed of 0.2c, then the estimated kinematic age is ∼104 years." @default.
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- W2856779319 date "2018-07-09" @default.
- W2856779319 modified "2023-10-18" @default.
- W2856779319 title "Resolving the Powerful Radio-loud Quasar at <i>z</i> ∼ 6" @default.
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- W2856779319 doi "https://doi.org/10.3847/1538-4357/aac76f" @default.
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