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Fig. 2

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Typical Spectrum of an emitter with a mass of 1.9 × 1010 M. Shown is the spectrum for the fiducial simulation (solid line), the simulation without any peculiar velocities and Hubble flow (dotted line), and a simulation where peculiar velocities were enabled but the Hubble flow was switched off (dashed line). Wavelength is given with respect to the observer’s restframe. For the fiducial simulation, the redshift due to the Hubble flow within the simulation box was ignored.

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