Oriol Abril scite author profile

The Cherenkov Telescope Array (CTA) is the next generation of Imaging Atmospheric Cherenkov Telescopes. It will reach a sensitivity and an energy resolution with no precedent in very high energy gamma-ray astronomy. In order to achieve this goal, the systematic uncertainties derived from the atmospheric conditions shall be reduced to a minimum. Different instruments may help to understand and account for the precise state of the atmosphere at a given time. The Barcelona IFAE/UAB (acronyms for

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Oriol Abril

Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)

CTA contributions to the 33rd International Cosmic Ray Conference (ICRC2013)

The IFAE/UAB and LUPM Raman LIDARs for Cherenkov Telescope Array Observatory

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