Time series photometry with a CCD camera

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Astronomical Photometry, Cameras, Charge Coupled Devices, Accuracy, Quantum Efficiency, Scintillation, Star Clusters, Time

Scientific paper

Time series observations of a field in the cluster NGC 4755 with a CCD camera are used to show that differential photometry between stars on the CCD frame is limited in accuracy mostly by photon statistics, over a 5 magnitude range. Scintillation noise appears to be almost entirely suppressed. The maximum accuracy possible is limited by the storage capacity of the CCD to about 0.001 mag.

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