Showing 21–40 of 65 results
/ Date/ Name
Nov 22, 2007The Effect of Primordial Non--Gaussianity on the Topology of Large-Scale StructureJul 10, 2003On Dark Matter Annihilation in the Local GroupAug 31, 1999PSCz-1.2 Jy Comparison: A Spherical Harmonics ApproachOct 2, 2014Large-scale peculiar velocities through the galaxy luminosity function at z ~ 0.1Mar 19, 2015Growth rate of cosmological perturbations at z ~ 0.1 from a new observational testNov 4, 2013Cosmology with massive neutrinos I: towards a realistic modeling of the relation between matter, haloes and galaxiesJun 16, 2005Local Supercluster Dynamics: External Tidal Impact of the PSCz sample traced by Optimized Numerical Least Action MethodMay 24, 2019Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSSMar 24, 2011A cross-correlation study of the Fermi-LAT $γ$-ray diffuse extragalactic signalAug 2, 2003IRAS PSCz v.s. 1.2-Jy Velocity and Density Fields: A Spherical Harmonics ComparisonJul 24, 2012A direct probe of cosmological power spectra of the peculiar velocity field and the gravitational lensing magnification from photometric redshift surveysJun 30, 2011A new method for the determination of the growth rate from galaxy redshift surveysFeb 19, 2012Gaia: a Window to Large Scale FlowsMar 19, 2015Tomography of the Fermi-LAT gamma-ray diffuse extragalactic signal via cross-correlations with galaxy catalogsJun 10, 2013The Hot and Energetic Universe: The missing baryons and the warm-hot intergalactic mediumMar 5, 2012Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveysSep 6, 2017Tomographic imaging of the Fermi-LAT gamma-ray sky through cross-correlations: A wider and deeper lookMay 3, 2005$γ$-ray flux from Dark Matter Annihilation in Galactic CausticsNov 11, 2004The Gaussian cell two-point "energy-like" equation: Application to large scale galaxy redshift and peculiar motion surveysAug 14, 2020Biasing relation, environmental dependencies and estimation of the growth rate from star forming galaxies