Showing 1–20 of 216 results
/ Date/ Name
Jul 17, 2012Planck intermediate results. VI: The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clustersJul 19, 2012Planck intermediate results. VII. Statistical properties of infrared and radio extragalactic sources from the Planck Early Release Compact Source Catalogue at frequencies between 100 and 857 GHzJan 11, 2011Planck early results. XXI. Properties of the interstellar medium in the Galactic planeJan 11, 2011Planck Early Results XXIV: Dust in the diffuse interstellar medium and the Galactic haloJan 11, 2011Planck Early Results: Thermal dust in Nearby Molecular CloudsJul 17, 2018Planck 2018 results. XII. Galactic astrophysics using polarized dust emissionJul 17, 2018Planck 2018 results. IV. Diffuse component separationMar 30, 1999The 2dF Galaxy Redshift Survey: Spectral Types and Luminosity FunctionsApr 26, 1999Constraining the equation of state of the Universe from Distant Type Ia Supernovae and Cosmic Microwave Background AnisotropiesMay 22, 1995The Stromlo-APM Redshift Survey III. Redshift Space Distortions, Omega and BiasAug 17, 1994A comparison of the evolution of the density field in perturbation theory and numerical simulations - II Counts in cells analysisDec 30, 2002The 2dF Galaxy Redshift Survey: the luminosity function of cluster galaxiesDec 3, 2001The 2dF Galaxy Redshift Survey: The dependence of galaxy clustering on luminosity and spectral typeMar 5, 1996Power Spectrum Analysis of the Stromlo-APM Redshift SurveyMar 9, 2001A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift SurveyOct 30, 2000Simulations of galaxy formation in a cosmological volumeJun 10, 2001Radio sources in the 2dF Galaxy Redshift Survey - II. Local radio luminosity functions for AGN and star-forming galaxies at 1.4 GHzMay 11, 2000Clustering of Galaxy Clusters in CDM UniversesMar 26, 1993The Imprint of Gravitational Waves on the Cosmic Microwave BackgroundMar 24, 2006A model for the metallicity evolution of damped Lyman-alpha systems