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19952013
most citedCOSMOS Photometric Redshifts with 30-bands for 2-deg2

1.2k citations · 4.1k across the 47 of their papers we have counts for

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11 papers · 1 filter

astro-ph200810 cited

The VVDS-VLA Deep Field - IV: Radio-optical properties

S. Bardelli, E. Zucca, M. Bolzonella +51

(abridged) We use the 1.4 GHz VIMOS-VLA Deep Survey and the optical VVDS and the CFHT-LS to compare the properties of radio loud galaxies with respect to the whole population of op…

astro-ph200835 cited

Eddington ratios of faint AGN at intermediate redshift: Evidence for a population of half-starved black holes

I. Gavignaud, L. Wisotzki, A. Bongiorno +51

We use one of the deepest spectroscopic samples of broad line active galactic nuclei (AGN) currently available, extracted from the VIMOS VLT Deep Survey (VVDS), to compute MgII and…

astro-ph20081 cited

Dark energy constraints and correlations with systematics from CFHTLS weak lensing, SNLS supernovae Ia and WMAP5

M. Kilbinger, K. Benabed, J. Guy +15

We combine measurements of weak gravitational lensing from the CFHTLS-Wide survey, supernovae Ia from CFHT SNLS and CMB anisotropies from WMAP5 to obtain joint constraints on cosmo…

astro-ph20081.2k cited

COSMOS Photometric Redshifts with 30-bands for 2-deg2

O. Ilbert, P. Capak, M. Salvato +60

We present accurate photometric redshifts in the 2-deg2 COSMOS field. The redshifts are computed with 30 broad, intermediate, and narrow bands covering the UV (GALEX), Visible-NIR…

astro-ph200816 cited

Comparisons between isothermal and NFW mass profiles for strong-lensing galaxy clusters

Chenggang Shu, Binglu Zhou, Matthias Bartelmann +3

While both isothermal and NFW-based mass models for galaxy clusters are widely adopted in strong-lensing studies, they cannot easily be distinguished based solely on observed posit…

astro-ph2008162 cited

The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey

B. Garilli, O. Le Fèvre, L. Guzzo +44

The VVDS-Wide survey has been designed with the general aim of tracing the large-scale distribution of galaxies at z~1 on comoving scales reaching ~100Mpc/h, while providing a good…