AtmoHEAD 2013 workshop / Atmospheric Monitoring for High-Energy Astroparticle Detectors
K. Bernl\"ohr, G. Bellassai, O. Blanch, M. Bourgeat, P. Bruno, M., Buscemi, C. Cassardo, P.M. Chadwick, R. Chalme-Calvet, F. Chouza, M. Cilmo,, M. Coco, J. Colombi, M. Compin, M.K. Daniel, R. De Los Reyes, J. Ebr, R., D'Elia, C. Deil, A. Etchegoyen, M. Doro, S. Ferrarese

TL;DR
This paper summarizes a workshop focused on atmospheric monitoring techniques crucial for calibrating high-energy astroparticle detectors, emphasizing the importance of real-time atmospheric data for reducing systematic uncertainties in astrophysical measurements.
Contribution
It highlights the interdisciplinary efforts and recent advancements in atmospheric calibration methods for next-generation high-energy astroparticle observatories.
Findings
Atmospheric conditions significantly impact detector calibration.
Improved atmospheric monitoring reduces systematic uncertainties.
Next-generation facilities require advanced atmospheric calibration techniques.
Abstract
A 3-day international workshop on atmospheric monitoring and calibration for high-energy astroparticle detectors, with a view towards next-generation facilities. The atmosphere is an integral component of many high-energy astroparticle detectors. Imaging atmospheric Cherenkov telescopes and cosmic-ray extensive air shower detectors are the two instruments driving the rapidly evolving fields of very-high- and ultra-high-energy astrophysics. In these instruments, the atmosphere is used as a giant calorimeter where cosmic rays and gamma rays deposit their energy and initiate EASs; it is also the medium through which the resulting Cherenkov light propagates. Uncertainties in real-time atmospheric conditions and in the fixed atmospheric models typically dominate all other systematic errors. With the improved sensitivity of upgraded IACTs such as H.E.S.S.-II and MAGIC-II and future facilities…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research · Dark Matter and Cosmic Phenomena
