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Mapping the Extended Lyα Emission within the Circumgalactic Medium of Quasars Hosted by Dusty Starbursts with CubeCarve

  • Authors: Kevin Hall, Hai Fu

Kevin Hall and Hai Fu 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 1.

Finder chart for each SMG–QSO composite system. Middle panel: KiDS gri tricolor image of the field centered at the position of the Herschel 250 μm source. The red-dashed circle corresponds to its positional uncertainty (﹩12\mathop{.}\limits{^{\prime\prime} }5﹩). Top panel: We provide the ALMA 870 μm continuum maps of each Herschel-detected source. Each panel is ﹩4\mathop{.}\limits{^{\prime\prime} }\times 4\mathop{.}\limits{^{\prime\prime} }﹩, and we indicate its location relative to the KiDS image as a white box. Additionally, the ellipse in the lower-right corner represents the shape of the CLEAN beam. Bottom panel: We present the pseudo-g-band images of the field as seen through KCWI and MUSE.

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