LAM oca fermilab

INSU


CeSAM

Refereed papers :
  • Guennou et al., 2010, A&A 523, 21 : Photometric redshifts along lines of sight of clusters in the z=[0.4,0.9] interval
  • Guennou et al., 2012, A&A, 537, 64 : Intracluster light in clusters of galaxies at redshifts 0.4<z<0.9
  • Guennou L., et al., 2013, A&A, 561, 112 : Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4-0.9] redshift range  
  • Guennou L., et al., 2014, A&A, 566, 149 : The mass profile and dynamical status of the z˜0.8 galaxy cluster LCDCS0504  
  • Murphy et al., ApJ, in revision : Analyzing deep HST Imagery of 10 hig-redshift galaxy cluster with weak lensing.  
  • Martinet et al., A&A, accepted, astroph: 1412.5821: The evolution of the cluster optical galaxy luminosity function between z=0.4 and 0.9 in the DAFT/FADA survey  

Conference presentations :
  • Guennou et al., Poster at GLCW: An alternative method to constrain dark energy: Weak Lensing Tomography in the Direction of Rich Clusters
  • Murphy et al. , Poster  at GLCW: "Weak Lensing with the Hubble Space Telescope"
  • Mazure et al.,Poster at "CL J2010: from Massive Galaxy Formation to Dark Energy",Japan, 2010: GALAXY CLUSTER SEARCHES IN THE CFHTLS AND APPLICATIONS
  • Durret et al.,Poster at "Galaxy clusters: observations, physics, and cosmology",Garching, 2010: "First results of the FADA (French American DArk energy) Survey"
  • Guennou, L. et al.,2012, SF2A, 465G: X-ray aspects of the DAFT/FADA clusters
  • Martinet, N., et al., 2013, SFsA, 367 M: Optical study of the DAFT/FADA galaxy cluster survey
  • Several presentations at the SESTO 2014 conference: The evolution of galaxy clusters and cluster galaxies in the epoch of large optical/IR surveys: http://www.sexten-cfa.eu/images/stories/conferenze2014/evogalclu/talks/EvoGalaClu_programwithtalks.pdf