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A Multiwavelength Portrait of the 3C 220.3 Lensed System

  • Authors: Sóley Ó. Hyman, Belinda J. Wilkes, S. P. Willner, Joanna Kuraszkiewicz, Mojegan Azadi, D. M. Worrall, Adi Foord, Simona Vegetti, Matthew L. N. Ashby, Mark Birkinshaw, Christopher Fassnacht, Martin Haas, Daniel Stern

Sóley Ó. Hyman et al 2024 The Astrophysical Journal 974 .

  • Provider: AAS Journals

Caption: Figure 4.

Negative images of the 3C 220.3 system. Left to right are visible (HST F606W+F814W), Chandra X-ray (0.5–8 keV, 0.″25 × 0.″25 subpixel binned, Gaussian smoothed with r = 1 pix), and VLA 9.0 GHz. Images are 12.″6 × 10.″5. Extraction regions shown, defined in Table 3, are 1 (galaxy A, green circle), 3 (galaxy B, blue circle), 5 (extended galaxy, cyan ellipse), 6 (Einstein ring, annulus between magenta and cyan ellipses), and 7 and 8 (NW and SE radio lobes, red ellipses). Region 9 (Table 3, not shown in this figure) measures the X-ray emission from the full source to allow comparison with lower-resolution X-ray data on this source.

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