One of the prominent science goal of the ELTs will be to study the physics and mass assembly of galaxies at very high redshifts. Here, we present the galaxy evolution science case for EAGLE, which is a NIR multi-integral field spectrograph for the E-ELT currently under phase A study. We summarize results of simulations conducted to derive high-level requirements. In particular, we show how we have derived the specifications for the ensquared energy that the AO system needs to provide to reach the scientific goals of the instrument. Finally, we present future strategies to conduct galaxy surveys with EAGLE
We study present-day galaxy clustering in the EAGLE cosmological hydrodynamical simulation. EAGLE’s ...
EAGLE is a Phase A study of a multi-IFU, near-IR spectrometer for the European Extremely Large Teles...
We present dust-attenuated and dust emission fluxes for sufficiently resolved galaxies in the EAGLE ...
International audienceOne of the prominent science goal of the ELTs will be to study the physics and...
International audienceOne of the prominent science goal of the ELTs will be to study the physics and...
International audienceOne of the prominent science goal of the ELTs will be to study the physics and...
International audienceOne of the prominent science goal of the ELTs will be to study the physics and...
One of the prominent science goal of the ELTs will be to study the physics and mass assembly of...
One of the prominent science goal of the ELTs will be to study the physics and mass assembly of...
10m-class telescopes such as the VLT and the Keck Telescope have allowed tremendous progress on the ...
EAGLE is an instrument under consideration for the European Extremely Large Telescope (E-ELT). EAGLE...
EAGLE is an instrument under consideration for the European Extremely Large Telescope (E-ELT). EAGLE...
We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE...
We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly...
Future galaxy surveys will map the galaxy distribution in the redshift interval 0.5 −15.4 and a flu...
We study present-day galaxy clustering in the EAGLE cosmological hydrodynamical simulation. EAGLE’s ...
EAGLE is a Phase A study of a multi-IFU, near-IR spectrometer for the European Extremely Large Teles...
We present dust-attenuated and dust emission fluxes for sufficiently resolved galaxies in the EAGLE ...
International audienceOne of the prominent science goal of the ELTs will be to study the physics and...
International audienceOne of the prominent science goal of the ELTs will be to study the physics and...
International audienceOne of the prominent science goal of the ELTs will be to study the physics and...
International audienceOne of the prominent science goal of the ELTs will be to study the physics and...
One of the prominent science goal of the ELTs will be to study the physics and mass assembly of...
One of the prominent science goal of the ELTs will be to study the physics and mass assembly of...
10m-class telescopes such as the VLT and the Keck Telescope have allowed tremendous progress on the ...
EAGLE is an instrument under consideration for the European Extremely Large Telescope (E-ELT). EAGLE...
EAGLE is an instrument under consideration for the European Extremely Large Telescope (E-ELT). EAGLE...
We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE...
We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly...
Future galaxy surveys will map the galaxy distribution in the redshift interval 0.5 −15.4 and a flu...
We study present-day galaxy clustering in the EAGLE cosmological hydrodynamical simulation. EAGLE’s ...
EAGLE is a Phase A study of a multi-IFU, near-IR spectrometer for the European Extremely Large Teles...
We present dust-attenuated and dust emission fluxes for sufficiently resolved galaxies in the EAGLE ...