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In this paper we employ a core-sampling analysis to find characteristic scales for the large- and the superlarge-scale structure (LSS and SLSS, respectively) in the Las Campanas Redshift Survey (LCRS). With this method, we show that the spatial distribution of galaxies can be roughly characterized as a superposition of three different populations of structural elements: the richest and most stable...

Large- and superlarge-scale structure in the Las Campanas Redshift Survey