From its origins, the Instrumentation Division has participated in the construction of instrumentation to detect and analyze light in the visible range of the spectrum. Cameras, spectrographs, polarization analyzers, optical fibers fed systems, among others, have been designed, built, integrated and verified in our facilities.
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Gran Telescopio Canarias (GTC): 10 años de Ciencia
A lo largo de los últimos 10 años, desde su inauguración, el Gran Telescopio Canarias (GTC), también conocido como Grantecan, ha contribuido en gran medida a...
Contract Ramón y Cajal to develop his research work in the specific research project "Feeding and hiding the monster: Triggering and obscuring the central...
HADES RV program with HARPS-N at the TNG. IX. A super-Earth around the M dwarf Gl 686
Aims: The HArps-n red Dwarf Exoplanet Survey (HADES) is providing a major contribution to the widening of the current statistics of low-mass planets, through...
HARMONI is one of the three ELT (European Extremely Large Telescope) first light scientific instruments. It is a visible and near-infrared (0.47 to 2.45 µm)...
HARMONI view of the host galaxies of active galactic nuclei around cosmic noon. Resolved stellar morpho-kinematics and the M<SUB>BH</SUB> − σ<SUB>⋆</SUB> relation
Context. The formation and evolution of galaxies appear linked to the growth of supermassive black holes, as evidenced by empirical scaling relations in nearby...
HARPS3 (High Accuracy Radial velocity Planet Searcher) is a new version of the succesful HARPS instrument. HARPS3 is an Echelle spectrograph with high...