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Physical Constraints on the Extended Interstellar Medium of the z = 6.42 Quasar J1148+5251: [C II]158 μm, [N II]205 μm, and [O I]146 μm Observations

  • Authors: Romain A. Meyer, Fabian Walter, Claudia Cicone, Pierre Cox, Roberto Decarli, Roberto Neri, Mladen Novak, Antonio Pensabene, Dominik Riechers, and Axel Weiss

2022 The Astrophysical Journal 927 152.

  • Provider: AAS Journals

Caption: Figure 4.

Continuum-subtracted spectrum of the [N II]205 μm (upper panel) and [O I]146 μm (lower panel). The spectra (black lines, shaded blue) are extracted in r = 1″ apertures centered on the peak of the emission in the velocity-integrated maps (Figure 3) using residual scaling (see Section 2). The 1σ noise level per channel for an r = 1″ aperture is shown in red, and a single-Gaussian fit is shown in orange (the best-fit parameters and uncertainties are in the upper right corners).

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