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Time Series Photometry with a CCD CameraTime 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.
Document ID
19850009597
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Walker, A. R. (South African Astronomical Observatory Sutherland., United States)
Date Acquired
August 12, 2013
Publication Date
November 1, 1984
Publication Information
Publication: NASA. Ames Research Center Proc. of the Workshop on Improvements to Photometry
Subject Category
Astronomy
Accession Number
85N17906
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19850009583Collected WorksProceedings of the Workshop on Improvements to Photometry19850009583Collected WorksProceedings of the Workshop on Improvements to Photometry
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