Origin and evolution of the brown dwarfs and giant planets
One of the main results obtained by the large optical and infrared sky surveys (DENIS, SDSS, 2MASS, UKIDSS, WISE) that started at the end of the last century...
PARSEC central de galaxias y tecnicas de alta resolucion espacial
PARSEC is an unique project in the astronomy community committed to the dual effort of maximum angular resolution -parsec-, maximum spectral coverage, and time...
Participation in the NISP instrument and preparation for EUCLID science
The main goal of this project is to ensure the scientific and technical participation of IAC and UPCT in the ESA space mission EUCLID (Cosmic Vision Program)...
Participation in the NISP instrument and preparation for the science of Euclid
The activity of the IAC in the NISP instrument will be focused on tasks related to testing the different models of the DAS (Driving and Acquisition Submodule)...
Participation in the NISP instrument and preparation for the scientific exploitation of Euclid
Esclarecer las propiedades de la materia y la energía oscura es uno de los problemas clave de la astrofísica actual. Este es el principal objetivo de la misión...
The Alpha Magnetic Spectrometer (AMS-02) is a general purpose high energy particle detector that was deployed to the International Space Station (ISS) on May 19...
AMS-02 (Alpha Magnetic Spectrometer) is a multi-purpose particle physics detector that was deployed in the International Space Station (ISS) on May 19, 2011...
The Alpha Magnetic Spectrometer (AMS) is a general purpose high energy particle detector that was deployed to the International Space Station (ISS) on May 19...
Participation of the Instituto de Astrofísica de Canarias in the development of HARMONI: Fase Delta-D1
The High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) is the first light instrument for the ELT, therefore...