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A VLBA-resolved Jet Associated with Super-Eddington Accretion in a Radio-loud Quasar at z = 3.4

  • Authors: Sakiko Obuchi, Ingyin Zaw, Kazuhiro Hada, Kohei Ichikawa, Joseph D. Gelfand

Sakiko Obuchi et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 1.

The VLBA images of ID830 at 1.6 GHz (left), 4.9 GHz (middle), and 8.2 GHz (right) with natural weighting. The negative and positive contours are shown as the red dashed and solid white lines, respectively. The contour levels are at −1, 1, 2, 3, 4, 8, ..., 2n times the 3σ rms noise level. The white ellipse in each panel represents the beam size. The core and jet components (J1–J3) are also labeled in the figure.

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