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The VIMOS VLT Deep Survey: the group catalogue
O. Cucciati, C. Marinoni, A. Iovino +39
[Abridged] We present a homogeneous and complete catalogue of optical groups identified in the purely flux limited (17.5<=I<=24.0) VIMOS-VLT Deep Survey (VVDS). We use mock catalog…
Resolved maps of stellar mass and SED of galaxies from optical/NIR imaging and SPS models
Stefano Zibetti, Stephane Charlot, Hans-Walter Rix
We report on the method developed by Zibetti, Charlot and Rix (2009) to construct resolved stellar mass maps of galaxies from optical and NIR imaging. Accurate pixel-by-pixel colou…
Polycyclic Aromatic Hydrocarbons in Galaxies at z~0.1: the Effect of Star Formation and AGN
Matthew J. O'Dowd, David Schiminovich, Benjamin D. Johnson +8
We present the analysis of the Polycyclic Aromatic Hydrocarbon (PAH) spectra of a sample of 92 typical star forming galaxies at 0.03 < z < 0.2 observed with the Spitzer IRS. We com…
Tracers of stellar mass-loss. I. Optical and near-IR colours and surface brightness fluctuations
Rosa A. Gonzalez-Lopezlira, Gustavo Bruzual-A., Stephane Charlot +2
We present optical and IR integrated colours and SBF magnitudes, computed from stellar population synthesis models that include emission from the dusty envelopes surrounding TP-AGB…
Resolved stellar mass maps of galaxies. I: method and implications for global mass estimates
Stefano Zibetti, Stephane Charlot, Hans-Walter Rix
(Abridged) We introduce a novel technique to construct spatially resolved maps of stellar mass surface density in galaxies based on optical and near IR imaging. We use optical/NIR…
The Vimos VLT Deep Survey: Stellar mass segregation and large-scale galaxy environment in the redshift range 0.2<z<1.4
M. Scodeggio, D. Vergani, O. Cucciati +49
Hierarchical models of galaxy formation predict that the properties of a dark matter halo depend on the large-scale environment surrounding the halo. As a result of this correlatio…