Figure 2 from 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

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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 2.

Continuum measurements from the literature and this work with the best-fit modified blackbody dust emission model. The effect of the CMB is accounted for as prescribed by Da Cunha et al. (2013), and the data points at ν > 10³ GHz are not used for the fit. The FIR luminosity, integrated over the shaded orange area, is not significantly affected by this choice.

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