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A Close Quasar Pair in a Massive Galaxy Merger at z = 5.7

  • Authors: Minghao Yue, Xiaohui Fan, Anna-Christina Eilers, Feige Wang, Jinyi Yang, Robert A. Simcoe

Minghao Yue et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 5.

The [C II] spectra of example pixels and their best-fit Gaussian emission line model (Section 2.2). For each pixel, we use a Gaussian profile to fit the [C II] line flux, velocity, and velocity dispersion (Figure 1).

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