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Orientatio ad sideera VI: a cultural astronomy approach
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GrantPARSEC central de galaxias y tecnicas de alta resolucion espacialPARSEC is an unique project in the astronomy community committed to the dual effort of maximum angular resolution -parsec-, maximum spectral coverage, and time...
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GrantParticipation in the NISP instrument and preparation for the science of EuclidThe 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)...
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GrantParticipation of IAC in the AMS experimentAMS-02 (Alpha Magnetic Spectrometer) is a multi-purpose particle physics detector that was deployed in the International Space Station (ISS) on May 19, 2011...
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GrantParticipation of IAC in the AMS experimentThe 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...
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GrantParticipation of the Instituto de Astrofísica de Canarias in the development of HARMONI: Fase Delta-D1The High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) is the first light instrument for the ELT, therefore...
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GrantPlanetary nebulae as the key to understanding binary stellarPer the classical, textbook definition, planetary nebulae are the glowing shells of gas and dust expelled by single, Sun-like stars at the end of their lives as...
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GrantPolarimetric inference of magnetic fieldsThe magnetic field is the main driver of the spectacular activity of the solar atmosphere, which covers the photosphere, chromosphere, transition region, and...
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GrantPolarimetric inference of magnetic fieldsThe magnetic field is the main driver of the spectacular activity of the solar atmosphere, which covers the photosphere, chromosphere, transition region, and...