We present a study of 17 LAEs at redshift 2 <z <3 gravitationally lensed by massive early-type galaxies (ETGs) at a mean redshift of approximately 0.5. Using a fully Bayesian grid-based technique, we model the gravitational lens mass distributions with elliptical power-law profiles and reconstruct the ultraviolet (UV)-continuum surface-brightness distributions of the background sources using pixellated source models. We find that the deflectors are close to, but not consistent with isothermal models in almost all cases, at the 2 sigma level. We take advantage of the lensing magnification (typically mu similar or equal to 20) to characterize the physical and morphological properties of these LAE galaxies. From reconstructing the ultraviolet ...
We present a new sample of strong gravitational lens systems where both the foreground lenses and ba...
A large statistical sample of z~3 galaxies has been efficiently UV-color-selected, and confirmed spe...
Published in: Astron. Astrophys. 351 (1999) 433 citations recorded in [Science Citation Index] Abst...
We present a study of 17 LAEs at redshift 2 <z <3 gravitationally lensed by massive early-type...
Lyman-alpha is one of the most important tools for studying star-forming regions in young galaxies. ...
We explore the properties of high-redshift Lyman-alpha emitters (LAE), and their link with the Lyman...
We explore the onset of star formation in the early Universe, exploiting the high-redshift observati...
Context. Faint galaxies are theorised to have played a major role, perhaps the dominant role, in rei...
We discuss the statistical properties of faint background galaxies detected in a deep Hubble Space T...
We have used the first matched set of GALEX and SDSS data to investigate the properties of a sample ...
We introduce a framework for simultaneously investigating the structure and luminosity evolution of ...
International audienceWe present optical and near-infrared spectroscopy obtained at Keck, Very Large...
We investigate the strongly lensed (mu similar or equal to x10-100) Lyman continuum (LyC) galaxy, du...
We report the discovery of a new Einstein cross at redshift z_S = 2.701 based on Lyman-alpha emissio...
We present a new sample of strong gravitational lens systems where both the foreground lenses and ba...
A large statistical sample of z~3 galaxies has been efficiently UV-color-selected, and confirmed spe...
Published in: Astron. Astrophys. 351 (1999) 433 citations recorded in [Science Citation Index] Abst...
We present a study of 17 LAEs at redshift 2 <z <3 gravitationally lensed by massive early-type...
Lyman-alpha is one of the most important tools for studying star-forming regions in young galaxies. ...
We explore the properties of high-redshift Lyman-alpha emitters (LAE), and their link with the Lyman...
We explore the onset of star formation in the early Universe, exploiting the high-redshift observati...
Context. Faint galaxies are theorised to have played a major role, perhaps the dominant role, in rei...
We discuss the statistical properties of faint background galaxies detected in a deep Hubble Space T...
We have used the first matched set of GALEX and SDSS data to investigate the properties of a sample ...
We introduce a framework for simultaneously investigating the structure and luminosity evolution of ...
International audienceWe present optical and near-infrared spectroscopy obtained at Keck, Very Large...
We investigate the strongly lensed (mu similar or equal to x10-100) Lyman continuum (LyC) galaxy, du...
We report the discovery of a new Einstein cross at redshift z_S = 2.701 based on Lyman-alpha emissio...
We present a new sample of strong gravitational lens systems where both the foreground lenses and ba...
A large statistical sample of z~3 galaxies has been efficiently UV-color-selected, and confirmed spe...
Published in: Astron. Astrophys. 351 (1999) 433 citations recorded in [Science Citation Index] Abst...