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The CCD/Transit Instrument (CTI) data-analysis systemAn account is given of the Kitt Peak CCD/Transit Instrument's software for the automated archiving, analysis, and interrogation of each observation night's nearly 450 Mbytes of image data. The analysis phase is performed by a pair of linked algorithms, one of which operates on the absolute pixel-values and the other on the spatial derivative of the data, so that both isolated and merged images are reliably detected in a single pass. This is in due course followed by the automatic comparison of each new detection with a set of predefined templates in parameter space, in order to find such interesting objects as supernovae, quasars, and variable stars.
Document ID
19870049110
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cawson, M. G. M.
(Arizona Univ. Tucson, AZ, United States)
Mcgraw, J. T.
(Arizona Univ. Tucson, AZ, United States)
Keane, M. J.
(Steward Observatory Tucson, AZ, United States)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Subject Category
Astronomy
Accession Number
87A36384
Funding Number(s)
CONTRACT_GRANT: NSF AST-83-14787
CONTRACT_GRANT: NAGW-121
CONTRACT_GRANT: NAGW-804
Distribution Limits
Public
Copyright
Other

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