Cluster galaxies at redshift 1.4

Computer Science

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Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies, Galaxy Groups, Clusters, And Superclusters, Large Scale Structure Of The Universe, Origin, Formation, Evolution, Age, And Star Formation

Scientific paper

We present new and partly preliminary results on the galaxy populations in the massive, X-ray luminous cluster XMMU J2235-2557 at redshift 1.39. We use high-quality optical and NIR data to study the luminosity function of cluster galaxies at different wavelengths (restframe ~3500, 6500, 9000 Å), confirming previous results at lower redshifts showing that the redshift evolution of the characteristic luminosity M* of the luminosity function is consistent with passive evolution of a stellar population formed at redshift z>2. We build a restframe U-R vs R color-magnitude diagram from high-resolution z- and H-band images of XMMU J2235-2557 within R~700 kpc, finding a tight red sequence already in place. When compared to models of elliptical galaxy formation [1], the slope and location of the red sequence indicate a formation redshift of z~3 for the bulk of the stars in red sequence galaxies, at least brighter than M*+1. Spectral energy distribution fitting of multicolor data sampling the restframe ~2700-9000 Å wavelength range consistently indicates that cluster members on the red sequence are already massive galaxies hosting evolved stellar populations.

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