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Absolute calibration of imaging atmospheric Cherenkov telescopes

2005/07/04 by N. Shepherd, Shepherd, N., J. H. Buckley +16
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #Atmospheric Ozone and Climate #Calibration and Measurement Techniques #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0507083

4 pages, 2 figure, Submitted to the 29th ICRC, Pune

arxiv created 2005/07/04 · openalex publication_date 2005/07/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

A calibrated laser pulse propagating through the atmosphere produces a flash of Rayleigh scattered light with an intensity that can be calculated very accurately when atmospheric conditions are good. This is used in a technique developed for the absolute calibration of ultra high energy cosmic ray fluorescence telescopes, and it can also be applied to imaging atmospheric Cherenkov telescopes (IACTs). In this paper we present the absolute calibration system being constructed and tested for the VERITAS project.

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