Paper
25 January 2010 Electron-multiplying CCD astronomical photometry
Alejandro Ferrero, Riccardo Felletti, Lorraine Hanlon, Joaquin Campos, Alicia Pons
Author Affiliations +
Proceedings Volume 7536, Sensors, Cameras, and Systems for Industrial/Scientific Applications XI; 75360Q (2010) https://doi.org/10.1117/12.840225
Event: IS&T/SPIE Electronic Imaging, 2010, San Jose, California, United States
Abstract
Electron Multiplying CCD is a CCD technology sensor reduces read-out noise to less than one electron. We study the way the usage of this technology affects to the astronomical photometry and to the improvement of the temporal resolution of the measurements. We show the effect of this technology on individual celestial sources and in the limiting magnitude. We propose a criterion to choose the optimal EM gain for a specific integration time. We explain a straightforward procedure to characterize the actual EM gain and the readout noise expressed in photo-electrons for every software-displayed gain, and we applied this procedure to the Andor Ixon DU-888E-C00-BV EMCCD.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alejandro Ferrero, Riccardo Felletti, Lorraine Hanlon, Joaquin Campos, and Alicia Pons "Electron-multiplying CCD astronomical photometry", Proc. SPIE 7536, Sensors, Cameras, and Systems for Industrial/Scientific Applications XI, 75360Q (25 January 2010); https://doi.org/10.1117/12.840225
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KEYWORDS
Signal to noise ratio

Electron multiplying charge coupled devices

Charge-coupled devices

Photons

Temporal resolution

Astronomy

Telescopes

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