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Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaître-Tolman-Bondi model

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Academic year: 2021

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Fig. 1. Upper panel: present-time (t = t 0 ) matter density parameters in the standard ( Λ CDM, black line) and the void (GBH)  cosmologi-cal models (red and cyan lines)
Table 1. Rest-frame 100 μm 1/V max luminosity function assuming the ΛCDM cosmological model
Table 4. Rest-frame 160 μ m 1 / V max luminosity function assuming the Λ CDM cosmological model.
Table 5. Rest-frame 160 μm 1/V max luminosity function assuming the CGBH cosmological model
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