Raman LIDARs for the atmospheric calibrationalong the line-of-sight of CTA

Autor: Ballester, Otger, Blanch, Oscar, Boix, Joan, Bregeon, Johan, Brun, Patrick, Çolak, §ıdıka Merve, Doro, Michele, Da Deppo, Vania, Font, Lluís, Gabella, Omar, García-Tenorio García-Balmaseda, Rafael, Gaug, Markus, Maggio, Camilla, Martínez, Manel Cruz, Martínez, Óscar, Adrover, Pere Munar, Ramos, Raúl, Rivoire, Stephane, Staniˇc, Samo, Villar, David, Vasileiadis, George, Wang, Longlong, Zavrtanik, Marko

Publikováno v: idUS: Depósito de Investigación de la Universidad de Sevilla
Universidad de Sevilla (US)
idUS. Depósito de Investigación de la Universidad de Sevilla
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The Cherenkov Telescope Array (CTA) is the next generation ground-based observatory forgamma-ray astronomy at very-high energies. Employing more than 100 Imaging AtmosphericCherenkov Telescopes in the northern and southern hemispheres, it was designe

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::5608208703bd639f67e3195686579bee