Among the science challenges of the Extremely Large Telescopes (ELTs),four object types are studied for performance with a 50 m ELT withadaptive optics (AO), Euro50. Emphasis is on planetary systems and verydistant objects. For planetary systems and their evolution, we examinehigh resolution imaging of the nuclei of comets and high-resolutionimaging, photometry and low and intermediate resolution spectroscopy ofKuiper-Belt objects. Imaging of Earth-like planets is discussed. Thevery high contrast imaging necessary for these purposes is discussedtogether with the relevant error sources. Finally, photometry andclassification of supernovae is discussed and examined. The performanceof a 50 m AO ELT is compared to corresponding data obtainable w...
We present an overview of the science case for a 50-100m Extremely Large Telescope. This was the sub...
International audienceAdaptive Optics systems, today available on 8-10m class telescopes are playing...
Adaptive Optics (AO) has become a key technology for the largest ground- based telescopes currently ...
We present an overview of the science case for a 50-100 m Extremely Large Telescope. A summary of th...
Some leading science programs undertaken with Very Large Telescopes and challenges driving the progr...
ELT science drivers stress aperture, Strehl ratio, PSF definition andstability, field of view, wavel...
ELT science drivers stress aperture, Strehl ratio, PSF definition and stability, field of view, wave...
Programmes driving ELT design are discussed. The nature and evolution of circum-stellar shells and p...
Highlights from the science case for an extremely large telescope are presented. As an introduction,...
With Euro50 as a convenient telescope laboratory, the Euro50 team has continued development aiming a...
We present an overview of the science case for a 50-100m Extremely Large Telescope. This was the sub...
The Euro50 is an extremely large telescope for optical and infrared wavelength with a 50 m primary m...
A number of Extremely Large Telescopes for visual-infrared and adjacent wavelengths are in various d...
The science case for the next generation of Extremely Large Telescopes (ELTs) covers a huge range of...
The European Extremely Large Telescope (E-ELT) is the most ambitious of the ELTs being planned. With...
We present an overview of the science case for a 50-100m Extremely Large Telescope. This was the sub...
International audienceAdaptive Optics systems, today available on 8-10m class telescopes are playing...
Adaptive Optics (AO) has become a key technology for the largest ground- based telescopes currently ...
We present an overview of the science case for a 50-100 m Extremely Large Telescope. A summary of th...
Some leading science programs undertaken with Very Large Telescopes and challenges driving the progr...
ELT science drivers stress aperture, Strehl ratio, PSF definition andstability, field of view, wavel...
ELT science drivers stress aperture, Strehl ratio, PSF definition and stability, field of view, wave...
Programmes driving ELT design are discussed. The nature and evolution of circum-stellar shells and p...
Highlights from the science case for an extremely large telescope are presented. As an introduction,...
With Euro50 as a convenient telescope laboratory, the Euro50 team has continued development aiming a...
We present an overview of the science case for a 50-100m Extremely Large Telescope. This was the sub...
The Euro50 is an extremely large telescope for optical and infrared wavelength with a 50 m primary m...
A number of Extremely Large Telescopes for visual-infrared and adjacent wavelengths are in various d...
The science case for the next generation of Extremely Large Telescopes (ELTs) covers a huge range of...
The European Extremely Large Telescope (E-ELT) is the most ambitious of the ELTs being planned. With...
We present an overview of the science case for a 50-100m Extremely Large Telescope. This was the sub...
International audienceAdaptive Optics systems, today available on 8-10m class telescopes are playing...
Adaptive Optics (AO) has become a key technology for the largest ground- based telescopes currently ...