We report a detection of galaxy-QSO cross-correlation w_{GQ} in the Sloan Digital Sky Survey (SDSS) Early Data Release (EDR) over 0.2-30 arc-minute scales. We cross-correlate galaxy samples of different mean depths r'=19-22 (z_G =0.15-0.35) with the main QSO population (i'_Q <19.2) at \zbar_Q \simeq 1.6. We find positive detection in most cases (except for the faintest QSOs as expeceted) with up to 8-sigma significance. The amplitude of the signal on arc-minute scales is about 20% at z_G=0.15 decreasing to 10% at z_G =0.35 This is a few times larger than currently expected from structure formation LCDM models o but confirms, at a higher significance, previous measurements by several groups. The shape and redshift evolution agrees well with ...
The aim of this thesis is to analyze statistically the available QSO, LRG, galaxy and cluster sample...
International audienceVia the magnification bias, gravitational lensing by large-scale structures ca...
Gravitational lensing predicts an enhancement of the density of bright, distant QSOs around foregrou...
We report a highly significant (> 10 sigma) spatial correlation between galaxies with S-350 mu m a p...
We report a highly significant (>10sigma) spatial correlation between galaxies with S350 mum >= 30 m...
We use the 2dF QSO Redshift Survey, to investigate whether QSOs are detectably gravitationally lense...
We cross-correlate QSOs from the 2dF Survey with galaxy groups. The galaxy samples are limited to B ...
We calculate the angular cross-correlation function between background QSOs and foreground galaxies ...
This is the first in a series of papers on the weak lensing effect caused by clusters of galaxies in...
This is the first in a series of papers on the weak lensing effect caused by clusters of galaxies in...
We review observations and gravitational lensing theory related to the magnification of background Q...
Correlations between the magnification or polarization of background sources, induced by gravitation...
We present an 8 sigma detection of cosmic magnification measured by the variation of quasar density ...
We detect a positive angular correlation between bright, high-redshift QSOs and foreground galaxies....
Via the magnification bias, gravitational lensing by large-scale structures causes angular cross-co...
The aim of this thesis is to analyze statistically the available QSO, LRG, galaxy and cluster sample...
International audienceVia the magnification bias, gravitational lensing by large-scale structures ca...
Gravitational lensing predicts an enhancement of the density of bright, distant QSOs around foregrou...
We report a highly significant (> 10 sigma) spatial correlation between galaxies with S-350 mu m a p...
We report a highly significant (>10sigma) spatial correlation between galaxies with S350 mum >= 30 m...
We use the 2dF QSO Redshift Survey, to investigate whether QSOs are detectably gravitationally lense...
We cross-correlate QSOs from the 2dF Survey with galaxy groups. The galaxy samples are limited to B ...
We calculate the angular cross-correlation function between background QSOs and foreground galaxies ...
This is the first in a series of papers on the weak lensing effect caused by clusters of galaxies in...
This is the first in a series of papers on the weak lensing effect caused by clusters of galaxies in...
We review observations and gravitational lensing theory related to the magnification of background Q...
Correlations between the magnification or polarization of background sources, induced by gravitation...
We present an 8 sigma detection of cosmic magnification measured by the variation of quasar density ...
We detect a positive angular correlation between bright, high-redshift QSOs and foreground galaxies....
Via the magnification bias, gravitational lensing by large-scale structures causes angular cross-co...
The aim of this thesis is to analyze statistically the available QSO, LRG, galaxy and cluster sample...
International audienceVia the magnification bias, gravitational lensing by large-scale structures ca...
Gravitational lensing predicts an enhancement of the density of bright, distant QSOs around foregrou...