Orateur
Michele Doro
(University of Padova and INFN)
Description
CTA is an advanced facility for ground-based gamma-ray astronomy in the GeV-TeV regime, currently in the Preparatory Phase. For a correct reconstruction of gamma-ray energies and fluxes, a precise monitoring of the atmospheric transmission is needed. With this aim, the IFAE and UAB institutes are building a specific Raman lidar.
For the optical module, we have foreseen to read-out from the lidar return 2 elastic (355 and 532 nm) and two Raman (387, 607) lines. In this contribution, we will discuss the design of the optical module, the light beam transportation, the solution for the custom made dichroic mirrors, interference filters.
Auteur principal
Michele Doro
(University of Padova and INFN)
Co-auteurs
Dr
Blanch Oscar
(Institut de Fisica d'Altes Energies)
Dr
Da Deppo Vania
(CNR-Institute for Photonics and Nanotechnologies UOS Padova LUXOR, Via Trasea 7, 35131 Padova, Italy)
Prof.
Font Lluis
(Universitat Autonoma de Barcelona)
Mlle
Lopez Oramas Alicia
(Institut de Fisica d'Altes Energies)
Prof.
Manel Martinez
(IFAE Barcelona)
Dr
Markus Gaug
(Universitat Autònoma de Barcelona)
