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In this work, I examine the environmental dependence of galaxy age, stellar velocity dispersion and stellar mass in the LOWZ sample of the Sloan Digital Sky Survey Data Release 10 (SDSS DR10). I measure the projected local density Σ5, divide the LOWZ sample into subsamples with a redshift binning size of Δz = 0.02 and analyze the environmental dependence of galaxy age, stellar velocity dispersion...
Using two volume-limited Main galaxy samples of the Sloan Digital Sky Survey Data Release 10 (SDSS DR10), we study u-band luminosity dependence of galaxy clustering by cluster analysis. Statistical results of two volume-limited Main galaxy samples are the same: luminous galaxies in Mu preferentially form isolated galaxies, close pairs and small groups at all scales, whereas faint galaxies in M...
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