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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 20.

The total spectra of the [C II]158 μm line, with (first row) and without (second row) residual scaling, extracted in r = 2″ and r = 4″ apertures (the first and second columns, respectively), in the PdBI data. The single-Gaussian (+continuum) fits to both data sets are shown in orange. In the absence of residual scaling, the continuum flux drops away from the [C II]158 μm line in the larger apertures (see the text for details). Even though no continuum was subtracted in the UV plane, the continuum flux approaches ∼ 0 mJy at the band edges in the r = 4″ aperture (without residual scaling), creating the illusion of a broad emission line.

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