Raman LIDARs and atmospheric calibration for the Cherenkov Telescope Array
G. Vasileiadis, O. Blanch, J. Bregeon, P. Brun, O. Calpe, M. Colak, M., Doro, L. Font, M. Gaug, S. Griffiths, C. Maggio, M. Martinez, O. Martinez, P., Ristori, S. Rivoire (for the CTA Consortium)

TL;DR
This paper discusses the development and design of Raman LIDARs for the Cherenkov Telescope Array to improve atmospheric calibration and reduce systematic uncertainties in gamma-ray observations.
Contribution
It introduces novel Raman LIDAR designs with large mirrors and multiple channels tailored for CTA, enhancing atmospheric measurement accuracy.
Findings
Raman LIDARs can reduce atmospheric systematic uncertainties to <5%.
Designed LIDARs achieve faster acquisition times with large mirrors.
The paper details the current status and technological advancements of these LIDARs.
Abstract
The Cherenkov Telescope Array (CTA) is the next generation of Imaging Atmospheric Cherenkov Telescopes. It will reach a sensitivity and energy resolution never obtained until now by any other high energy gamma-ray experiment. Understanding the systematic uncertainties in general will be a crucial issue for the performance of CTA. It is well known that atmospheric conditions contribute particularly in this aspect.Within the CTA consortium several groups are currently building Raman LIDARs to be installed on the two sites. Raman LIDARs are devices composed of a powerful laser that shoots into the atmosphere, a collector that gathers the backscattered light from molecules and aerosols, a photo-sensor, an optical module that spectrally selects wavelengths of interest, and a read--out system.Unlike currently used elastic LIDARs, they can help reduce the systematic uncertainties of the…
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Taxonomy
TopicsRadiation Detection and Scintillator Technologies · Astrophysics and Cosmic Phenomena · Advanced Optical Sensing Technologies
