Showing 1–20 of 26 results
/ Date/ Name
Jun 22, 2010VLT LBG Redshift Survey II: Interactions between galaxies and the IGM at z ~3Mar 17, 2010The VIMOS VLT Deep Survey: Star Formation Rate Density of Lya emitters from a sample of 217 galaxies with spectroscopic redshifts 2<z<6.6Apr 16, 2012The VLT LBG Redshift Survey - III. The clustering and dynamics of Lyman-break galaxies at z ~ 3Jul 12, 2016Probing the intra-group medium of a z = 0.28 galaxy groupNov 29, 2011The WIRCam Deep Survey I: Counts, colours and mass-functions derived from near-infrared imaging in the CFHTLS deep fieldsMay 24, 2018A cosmic dance at z~3: Detecting the host galaxies of the dual AGN system LBQS0302-0019 and Jil with HAWK-I+GRAALMar 6, 20194MOST: Project overview and information for the First Call for ProposalsMar 15, 2016The 2QDES Pilot : The luminosity and redshift dependence of quasar clusteringFeb 20, 2013X-Ray Groups of Galaxies in the Aegis Deep and Wide FieldsApr 16, 2013The VLT LBG Redshift Survey - IV. Gas and galaxies at z ~ 3 in observations and simulationsOct 15, 2020The nature of sub-millimetre galaxies I: A comparison of AGN and star-forming galaxy SED fitsSep 14, 2018Quasar Sightline and Galaxy Evolution (QSAGE) Survey - I. The Galaxy Environment of OVI Absorbers up to z=1.4 around PKS 0232-04Sep 5, 2011The Star Formation Rate Density and Dust Attenuation Evolution over 12 Gyr with the VVDS SurveysSep 19, 2014The evolution of star formation activity in galaxy groupsSep 20, 2012Sub-millimetre source identifications and the micro-Jansky source population at 8.4 GHz in the William Herschel Deep FieldAug 19, 2011Submillimetre observations of X-ray active galactic nuclei in the William Herschel Deep FieldNov 5, 2015Non-linearity and environmental dependence of the star forming galaxies Main SequenceMar 17, 2007Anomalous SZ Contribution to 3 Year WMAP DataNov 16, 2023Quasar Sightline and Galaxy Evolution (QSAGE) -- III. The mass-metallicity and fundamental metallicity relation of $z \approx$ 2.2 galaxiesOct 8, 2013The WIRCam Deep Survey II: Mass Selected Clustering