Following the novel development and adaptation of the Metric Space Technique (MST), a multi-scale morphological analysis of the Sloan Digital Sky Survey (SDSS) Data Release 5 (DR5) was performed. The technique was adapted to perform a space-scale morphological analysis by filtering the galaxy point distributions with a smoothing Gaussian function, thus giving quantitative structural information on all size scales between 5 and 250 Mpc. The analysis was performed on a dozen slices of a volume of space containing many newly measured galaxies from the SDSS DR5 survey. Using the MST, observational data were compared to galaxy samples taken from N-body simulations with current best estimates of cosmological parameters and from random catalogs. By using the maximal ranking method among MST output functions, we also develop a way to quantify the overall similarity of the observed samples with the simulated samples. © 2009. The American Astronomical Society. All rights reserved.
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Wu, Y., Batuski, D. J., & Khalil, A. (2009). Multi-scale morphological analysis of sdss DR5 survey using the metric space technique. Astrophysical Journal, 707(2), 1160–1167. https://doi.org/10.1088/0004-637X/707/2/1160