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19952007
most citedMeasuring Omega_0 with higher-order Quasar-Galaxy Correlations induced by Weak Lensing

48 citations · 127 across the 10 of their papers we have counts for

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Showing 2007Show all

11 papers · 1 filter

astro-ph200744 cited

Time drift of cosmological redshifts and its variance

Jean-Philippe Uzan, Francis Bernardeau, Yannick Mellier

The contribution of cosmological perturbations to the time drift of the cosmological redshift is derived. It is shown that the dominant correction arises from the local acceleratio…

astro-ph200716 cited

Testing Gravity with the CFHTLS-Wide Cosmic Shear Survey and SDSS LRGs

O. Doré, M. Martig, Y. Mellier +7

General relativity as one the pillar of modern cosmology has to be thoroughly tested if we want to achieve an accurate cosmology. We present the results from such a test on cosmolo…

astro-ph200751 cited

Clustering properties of a type-selected volume-limited sample of galaxies in the CFHTLS

H. J. McCracken, O. Ilbert, Y. Mellier +5

(abridged) We present an investigation of the clustering of i'AB<24.5 galaxies in the redshift interval 0.2<z<1.2. Using 100,000 precise photometric redshifts in the four ultra-dee…

astro-ph2007111 cited

The Masses and Shapes of Dark Matter Halos from Galaxy-Galaxy Lensing in the CFHTLS

Laura C. Parker, Henk Hoekstra, Michael J. Hudson +2

We present the first galaxy-galaxy weak lensing results using early data from the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS). These results are based on ~22 sq. deg. of…

astro-ph200773 cited

The VIMOS VLT Deep Survey: Tracing the galaxy stellar mass assembly history over the last 8Gyr

D. Vergani, M. Scodeggio, L. Pozzetti +46

We selected a mass-limited sample of 4048 objects from the VIMOS VLT Deep Survey in the redshift interval 0.5<z<1.3. We used the amplitude of the 4000 Balmer break (Dn4000) to sepa…

astro-ph200764 cited

The angular correlations of galaxies in the COSMOS field

H. J. McCracken, J. A. Peacock, L. Guzzo +21

We present measurements of the two-point galaxy angular correlation function w(θ) in the COSMOS field. Independent determinations of w(θ) as a function of magnitude limit are prese…