We present mass estimates for dark matter halos around galaxies from the COMBO-17 survey using weak gravitational lensing. COMBO-17, with photometry in 17 optical filters, provides precise photometric redshifts and spectral classification for objects with $R<24$. This permits to select and sort lens and source galaxies by their redshifts and lens luminosity or color, which bypasses many uncertainties in other weak lensing analyses arising from broadly estimated source and lens redshifts. We study the shear created by dark matter halos around 12 000 galaxy lenses at redshifts $z_\mathrm{d}=0.2{-}0.7$ by fitting the mass normalization of either singular isothermal spheres (SIS) or Navarro-Frenk-White (NFW) profiles to background ...
We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC)...
In my thesis I study the projected density distribution of all (dark+baryonic) matter around various...
Context. Understanding the evolution of the dark matter halos of galaxies after they become part of...
We present mass estimates for dark matter halos around galaxies from the COMBO-17 survey using weak ...
We study the dark matter halos of galaxies with galaxy-galaxy lensing using the COMBO-17 survey. Thi...
We use galaxy-galaxy lensing to study the statistical properties of the dark matter halos of galaxie...
Gravitat ional lensing can be used as a direct probe of the distribut ion of dark matter around gala...
We present a study of the relation between dark matter halo mass and the baryonic content of host ga...
Weak gravitational lensing has become an important tool to study the properties of dark matter halo...
The distortion of the images of faint high-redshift galaxies can be used to probe the intervening ma...
International audienceCosmological simulations predict that galaxies are embedded into triaxial dark...
International audienceWe present the first galaxy-galaxy weak-lensing results using early data from ...
In this review, I discuss the use of galaxy-galaxy weak lensing measurements to study the masses of ...
The distortion of the images of faint high-redshift galaxies can be used to probe the intervening ma...
The dynamical properties of galaxies suggest they live in a cocoon or halo of dark matter, the natur...
We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC)...
In my thesis I study the projected density distribution of all (dark+baryonic) matter around various...
Context. Understanding the evolution of the dark matter halos of galaxies after they become part of...
We present mass estimates for dark matter halos around galaxies from the COMBO-17 survey using weak ...
We study the dark matter halos of galaxies with galaxy-galaxy lensing using the COMBO-17 survey. Thi...
We use galaxy-galaxy lensing to study the statistical properties of the dark matter halos of galaxie...
Gravitat ional lensing can be used as a direct probe of the distribut ion of dark matter around gala...
We present a study of the relation between dark matter halo mass and the baryonic content of host ga...
Weak gravitational lensing has become an important tool to study the properties of dark matter halo...
The distortion of the images of faint high-redshift galaxies can be used to probe the intervening ma...
International audienceCosmological simulations predict that galaxies are embedded into triaxial dark...
International audienceWe present the first galaxy-galaxy weak-lensing results using early data from ...
In this review, I discuss the use of galaxy-galaxy weak lensing measurements to study the masses of ...
The distortion of the images of faint high-redshift galaxies can be used to probe the intervening ma...
The dynamical properties of galaxies suggest they live in a cocoon or halo of dark matter, the natur...
We infer the connection between the stellar mass of galaxies from the Subaru Hyper Suprime-Cam (HSC)...
In my thesis I study the projected density distribution of all (dark+baryonic) matter around various...
Context. Understanding the evolution of the dark matter halos of galaxies after they become part of...