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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 1.

Smoothed (Gaussian with r = 1.5 pix) HST negative images of the 3C 220.3 system. Images (left to right) have effective wavelengths of 606 nm, 814 nm, and 1.60 μm. Images are 9″ on a side, with north up and east to the left. System components are labeled in the center panel. The bright spot to the left of the galaxy A core in F814W is a cosmic ray which could not be removed during image drizzling (C. Leipski 2014, private communication). The 2021 Binospec slit (20″ × 1″) placement is shown in blue in panel (a) with the red box (1″ × 1″) marking the center of the slit.

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