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Popesso, Paola (2006): The RASS-SDSS galaxy cluster survey.: Correlating X-ray and optical properties of galaxy clusters.. Dissertation, LMU München: Fakultät für Physik

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Figure

Fig. 3. The Composite LF in the fi ve Sloan bands calculated within 1 Mpc h−1 aperture and with a global background correction
Fig. 6. 1, 2 and 3σ contours of the best fi t Schechter parameters forthe bright component of the Composite LF
Fig. 7. Distribution of the Schechter parameters1 Mpcdistribution ofSchechter luminosity function to the galaxies in the whole availableto the value of the corresponding bright component of the Compositeters
Fig. 9. Dwarf to Giant Ratio (DGR) as a function of the cluster radiiin the 5 wavebands
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