VVDS-SWIRE: Clustering evolution up to z=2 of a spectroscopic sample of galaxies selected from Spitzer IRAC 3.6 and 4.5 microns photometry

S. de la Torre,O. Le Fèvre,Stephane Arnouts,Luigi Guzzo,Duncan Farrah,A. Iovino,Carol J. Lonsdale,B. Meneux,S. J. Oliver,Agnieszka Pollo,I. Waddington,D. Bottini,Fan Fang,B. Garilli,V. Le Brun,D. Maccagni,J. P. Picat,Roberto Scaramella,M. Scodeggio,David L. Shupe,Jason Surace,L. Tresse,G. Vettolani,A. Zanichelli,C. Adami,S. Bardelli,M. Bolzonella,A. Cappi,S. Charlot,Paolo Ciliegi,Thierry Contini,Sébastien Foucaud,P. Franzetti,I. Gavignaud,Olivier Ilbert,H. J. McCracken,Bruno Marano,Christian Marinoni,A. Mazure,R. Merighi,Stephane Paltani,Roser Pello,Lucia Pozzetti,M. Radovich,G. Zamorani,Elena Zucca,M. Bondi,Angela Bongiorno,J. Brinchmann,Olga Cucciati,F. Lamareille,Yannick Mellier,P. Merluzzi,S. Temporin,D. Vergani,C. J. Walcher

VVDS-SWIRE: Clustering evolution up to z=2 of a spectroscopic sample of galaxies selected from Spitzer IRAC 3.6 and 4.5 microns photometry

2007

By combining the VVDS with the SWIRE data, we have built the currently largest spectroscopic sample of galaxies selected in the rest-frame near-infrared. These allow us to investigate, for the first time using spectroscopic redshifts, the clustering evolution of galaxies selected from their rest-frame near-infrared luminosity in the redshift range 0.2

Keywords:

Photometry (optics)
Astrophysics
Galaxy
Cluster analysis
Physics

Correction
Source
Cite
Save
Machine Reading By IdeaReader

References

Citations