Showing 1–20 of 68 results
/ Date/ Name
Dec 17, 2005The Luminosity-Weighted or `Marked' Correlation FunctionOct 3, 2013PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1Mar 8, 2011Properties of Dark Matter Haloes and their Correlations: the Lesson from Principal Component AnalysisNov 1, 2012Measures of galaxy environment -- II. Rank-ordered mark correlationsJan 25, 2010Are Brightest Halo Galaxies Central Galaxies?Oct 29, 2012The Spatial Distribution of Dust and Stellar Emission of the Magellanic CloudsJul 21, 2007Satellite Luminosities in Galaxy GroupsMay 8, 2008Central and Satellite Colors in Galaxy Groups: A Comparison of the Halo Model and SDSS Group CatalogsJun 20, 2011The Emission by Dust and Stars of Nearby Galaxies in the Herschel KINGFISH SurveyMar 2, 2015Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2Nov 24, 2008Galaxy Zoo: Disentangling the Environmental Dependence of Morphology and ColourNov 3, 2011Galaxy Zoo: The Environmental Dependence of Bars and Bulges in Disc GalaxiesMay 2, 2008A Halo Model of Galaxy Colors and Clustering in the SDSSJul 21, 2009Less than 10 percent of star formation in z=0.6 massive galaxies is triggered by major interactionsMay 11, 2011Ameliorating Systematic Uncertainties in the Angular Clustering of Galaxies: A Study using SDSS-IIINov 16, 2012The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: the low redshift sampleFeb 27, 2012The clustering of galaxies at z~0.5 in the SDSS-III Data Release 9 BOSS-CMASS sample: a test for the LCDM cosmologyDec 17, 2013The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samplesOct 21, 2008Evaluating and Improving Semi-analytic modelling of Dust in Galaxies based on Radiative Transfer CalculationsSep 16, 2010How does galaxy environment matter? The relationship between galaxy environments, colour and stellar mass at 0.4 < z < 1 in the Palomar/DEEP2 survey