Absolute Calibration of a Large-diameter Light Source
classification
🌌 astro-ph.IM
physics.ins-det
keywords
lightabsolutecalibrationsourceapertureaugercalibrateddetectors
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A method of absolute calibration for large aperture optical systems is presented, using the example of the Pierre Auger Observatory fluorescence detectors. A 2.5 m diameter light source illuminated by an ultra--violet light emitting diode is calibrated with an overall uncertainty of 2.1 % at a wavelength of 365 nm.
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