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High-resolution ALMA Imaging for a Gravitationally Lensed Quasar at z = 6.5: Constraining the Active Galactic Nucleus Contribution to Galactic-scale Dust Heating

  • Authors: Minghao Yue, Xiaohui Fan, Anna-Christina Eilers, Jinyi Yang, Feige Wang, Jianwei Lyu, James W. Nightingale, Ann Zabludoff, Ran Wang

Minghao Yue et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 1.

The clean image for the continuum emission of J0439+1634. The image is produced using the CASA task tclean using Briggs weighting (with robust = 0.5). The beam size is ﹩0\mathop{.}\limits{^{\prime\prime} }078\times 0\mathop{.}\limits{^{\prime\prime} }040﹩, shown as the white ellipse at the lower left corner. The 1σ sensitivity is 0.02 mJy beam−1. The two bright blobs are the lensed images of the quasar host galaxy’s central region, and the diffused emission shows the lensed arc of the quasar host galaxy.

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