Centro de Astrofísica U.Porto

Publications of the project “Understanding the Massive Galaxies in the Universe” (PTDC/CTE-AST/66147/2006 & FCOMP-01-0124-FEDER-007118)

The VVDS type-1 AGN sample: The faint end of the luminosity function
Highlights from the VIMOS VLT Deep Survey
The VIMOS-VLT Deep Survey: Mass and light clustering in the Universe during the last 8 billion years
The Fifth Data Release of the Sloan Digital Sky Survey
Bursty stellar populations and obscured active galactic nuclei in galaxy bulges
The VIMOS VLT Deep Survey: The Assembly History of the Stellar Mass in Galaxies: from the Young to the Old Universe
VVDS-SWIRE Clustering evolution from a spectroscopic sample of galaxies with redshift 0.2 < z < 2.1 selected from Spitzer IRAC 3.6 μm and 4.5 μm photometry
UV Star Formation Rates in the Local Universe
A census of metals and baryons in stars in the local Universe
The VIMOS VLT deep survey The K -band follow-up in the 0226-04 field
The Lopsidedness of Present-Day Galaxies: Results from the Sloan Digital Sky Survey
The Sixth Data Release of the Sloan Digital Sky Survey
New insights into the stellar content and physical conditions of star-forming galaxies at z = 2–3 from spectral modelling
Metallicities and Physical Conditions in Star-forming Galaxies at z ~ 1.0-1.5
Galaxies with Wolf-Rayet signatures in the low-redshift Universe - A survey using the Sloan Digital Sky Survey
The VIMOS VLT Deep Survey - Testing the gravitational instability paradigm at z ∼ 1
The VIMOS VLT Deep Survey: Tracing the galaxy stellar mass assembly history over the last 8 Gyr
The VVDS-SWIRE-GALEX-CFHTLS surveys: Physical properties of galaxies at z below 1.2 from photometric data
Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey - I. The evolution of the mass-metallicity relation up to z ∼ 0.9
Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey - II. Extending the mass-metallicity relation to the range z ≈0.89–1.24
Galaxy evolution in Abell 85: I. Cluster substructure and environmental effects on the blue galaxy population
The VVDS-VLA deep field - IV. Radio-optical properties
The VIMOS VLT Deep Survey
Evolution of the major merger rate since z ∼ 1 from spectroscopically confirmed galaxy pairs
SEGUE: A Spectroscopic Survey of 240,000 Stars With g = 14-20
The Seventh Data Release of the Sloan Digital Sky Survey
The Vimos VLT Deep Survey: Stellar mass segregation and large-scale galaxy environment in the redshift range 0.2 < z < 1.4
The GALEX Arecibo SDSS Survey. I. Gas Fraction Scaling Relations of Massive Galaxies and First Data Release