Add to ORKGThe redshift distribution derived from complete samples suggests that the majority of blue galaxies dominating the faint field counts are moderately low redshift z<1. Additionally, new results in distant clusters suggest the presence of numerous old red galaxies at z≃1. I question whether these observations are consistent with the first results on the predominantly blue population of very faint galaxies background to z≃0.4 clusters as deduced from lensing studies
Published in: Astron. Astrophys. 351 (1999) 433 citations recorded in [Science Citation Index] Abst...
In my thesis I study the projected density distribution of all (dark+baryonic) matter around various...
Context. There is some disagreement about the abundance of faint galaxies in high-redshift clusters,...
The redshift distribution derived from complete samples suggests that the majority of blue galaxies ...
We discuss the results of a series of redshift surveys of faint galaxies and their implications for ...
Cosmological constraints from galaxy clusters rely on accurate measurements of the mass and internal...
From deep optical images of three clusters, selected by virtue of their X-ray luminosity and/or opti...
The results of two new redshift surveys carried out with the Low Dispersion Survey Spectrograph (LDS...
At B magnitudes >~ 24 there is a well-known excess of galaxies (compared to standard models) which i...
Using the multislit LDSS-2 spectrograph on the William Herschel Telescope, we have completed a redsh...
We use weak lensing shear measurements of six $z>0.5$ clusters of galaxies to derive the mean lensin...
We estimate the spatial clustering of faint galaxies in an extensive new redshift survey performed u...
We report results based on 35 new spectroscopic redshifts obtained with the Keck Telescope for field...
We discuss the statistical properties of faint background galaxies detected in a deep Hubble Space T...
15 pages, 10 figures, accepted for publication in MNRASInternational audienceUsing galaxy clusters f...
Published in: Astron. Astrophys. 351 (1999) 433 citations recorded in [Science Citation Index] Abst...
In my thesis I study the projected density distribution of all (dark+baryonic) matter around various...
Context. There is some disagreement about the abundance of faint galaxies in high-redshift clusters,...
The redshift distribution derived from complete samples suggests that the majority of blue galaxies ...
We discuss the results of a series of redshift surveys of faint galaxies and their implications for ...
Cosmological constraints from galaxy clusters rely on accurate measurements of the mass and internal...
From deep optical images of three clusters, selected by virtue of their X-ray luminosity and/or opti...
The results of two new redshift surveys carried out with the Low Dispersion Survey Spectrograph (LDS...
At B magnitudes >~ 24 there is a well-known excess of galaxies (compared to standard models) which i...
Using the multislit LDSS-2 spectrograph on the William Herschel Telescope, we have completed a redsh...
We use weak lensing shear measurements of six $z>0.5$ clusters of galaxies to derive the mean lensin...
We estimate the spatial clustering of faint galaxies in an extensive new redshift survey performed u...
We report results based on 35 new spectroscopic redshifts obtained with the Keck Telescope for field...
We discuss the statistical properties of faint background galaxies detected in a deep Hubble Space T...
15 pages, 10 figures, accepted for publication in MNRASInternational audienceUsing galaxy clusters f...
Published in: Astron. Astrophys. 351 (1999) 433 citations recorded in [Science Citation Index] Abst...
In my thesis I study the projected density distribution of all (dark+baryonic) matter around various...
Context. There is some disagreement about the abundance of faint galaxies in high-redshift clusters,...