Fig. 12 from Toward Understanding Rich Superclusters

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Toward Understanding Rich Superclusters

Authors: M. Einasto, E. Saar, V. J. Martínez, J. Einasto, L. J. Liivamägi, E. Tago, J.-L. Starck, V. Müller, P. Heinämäki, P. Nurmi, S. Paredes, M. Gramann, and G. Hütsi

Einasto et al. 2008 The Astrophysical Journal 685 83.

Provider: AAS Journals

Caption: Fig. 12.

Differential luminosity function histograms ﹩F=dN/ dM﹩, where M is the absolute magnitude of a galaxy, for galaxies in the supercluster SCl 126; here the solid line shows the luminosity function and the dashed lines indicate the Poisson errors. Black lines show the histogram for the 0.5 mag bins, and gray lines show the histogram for the 0.25 mag bins.

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