A method involving the use of a primary standard source of synchrotron radiation for precision calibration of the sensitivity of telescopes equipped with a CCD array and high angular resolution is considered. The method is based on precision reproduction of the spectral energy characteristics, the Gaussian distribution of the spectral density of the irradiance over a radiating region, and the stability and reproducibility of the characteristics of synchrotron radiation in a single-electron regime.
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The present study was carried out with the support of the Ministry of Education and Science of Russia (Contract No. 14.592.21.0001, August 22, 2014).
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Translated from Izmeritel’naya Tekhnika, No. 5, pp. 33–36, May, 2015.
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Anevskii, S.I., Zolotarevskii, Y.M., Krutikov, V.N. et al. The Use of a Standard Source of Synchrotron Radiation for Calibration of the Sensitivity of a Telescope with CCD Array and High Angular Resolution. Meas Tech 58, 520–525 (2015). https://doi.org/10.1007/s11018-015-0747-6
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DOI: https://doi.org/10.1007/s11018-015-0747-6