The star 55 Cancri was one of the first known exoplanet hosts and each of the planets in this system is remarkable. Planets b and c are in a near 1:3 resonance...
Hard X-ray-to-radio energy distributions in starburst galaxies
We present in this contribution the predictions on the multiwavelength spectral energy distribution of our evolutionary population synthesis models including...
HARMONI - the Extremely Large Telescope first light integral field spectrograph: pre-optics: stray light analysis
HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 450nm to 2450nm with resolving...
HARMONI at ELT: athermal toroidal mirror mount for HARMONI pre-optics
HARMONI is the high angular resolution optical and near-IR integral field spectrograph for the Extremely Large telescope (ELT). It covers a large spectral range...
HARMONI at ELT: design and tests results of the instrument cryogenic fast shutter
HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470nm to 2450nm with resolving...
HARMONI at ELT: designing a laser guide star wavefront sensors for the ELT
HARMONI is the first light visible and near-IR integral field spectrograph for the ELT covering a large spectral range from 450nm to 2450nm with resolving...
The High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) is planned as a first light instrument for the Extremely...
HARMONI at ELT: HIPOTEC electronics and control system
HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470nm to 2450nm with resolving...
HARMONI at ELT: mechanisms of the pre-optics at CDR
HARMONI is the first light visible and near-IR integral field spectrograph for the Extremely Large Telescope (ELT). This instrument covers a large spectral...