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A CCD antiblooming technique for use in photometryA new antiblooming technique was used to collect images for a BL Lac monitoring project. The antiblooming was accomplished by clocking two of the collection phases (in a three-phase chip) back and forth during the integration of an image. Calibrations were done using VRI standard stars to insure that the technique did not affect normal photon collection and photometric data. New sources of noise were identified which must be subtracted from the processed imaging. In contrast, the technique reduced dark current noise, which is of benefit with a thermoelectric-cooled camera. The technique eliminated blooming across the stars of interest, while preserving photon-collection efficiency. It also reduced the total noise of the exposures.
Document ID
19950041570
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Neely, A. William
(NF/Observatory Ltd. San Lorenzo, NM, United States)
Janesick, James R.
(Jet Propulsion Laboratory, California Inst. of Tech., Pasadena, CA United States)
Date Acquired
August 16, 2013
Publication Date
November 1, 1993
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 105
Issue: 693
ISSN: 0004-6280
Subject Category
Astronomy
Accession Number
95A73169
Distribution Limits
Public
Copyright
Other

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