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Future virialized structures: an analysis of superstructures in the SDSS DR7

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Academic year: 2020

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Table 1. Galaxy samples in the SDSS-DR7. In all cases z ≥ 0.04 and the apparent magnitude in the r band is in the range 14.5 ≤ r ≤ 17.5
Figure 1. A slice of the luminosity density map for sample S2. The Carte- Carte-sian system used is associated with the equatorial coordinate system, with the z-axis towards the north celestial pole
Figure 2. Distribution of the mass overdensity of the superstructures identi- identi-fied in the simulation box, for different values of the luminosity overdensity parameter (D T = 4.5, 5.5 and 9, in the top left-hand, top right-hand and  bot-tom left-hand
Figure 4. Histograms representing the luminosity (a) and volume (b) distributions of FVSs
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