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Gain calibrating nonuniform image-array data using only the image dataAn algorithm is developed for calibrating the spatial nonuniformity of image-array (CCD-type) detectors. Like other techniques this approach uses multiple, spatially displaced images. In circumstances where high-precision flat fields are not available by other means (i.e., sky flats) this technique is advantageous as it uses the data frames for gain calibration even when the array images extended, nonuniform, sources. Numerical experiments and direct observations with intrinsically uniform and quite nonuniform detectors show that this algorithm is useful when data frames are crowded with sources - circumstance where 'median filtering' flatfielding techniques often fail. The algorithm described is robust and efficiently uses information from multiple data frames to determine pixel gain variations, using visible and IR array observations of extended sources.
Document ID
19920030009
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kuhn, J. R.
(Michigan State Univ. East Lansing, MI, United States)
Lin, H.
(Michigan State Univ. East Lansing, MI, United States)
Loranz, D.
(Michigan State University East Lansing, United States)
Date Acquired
August 15, 2013
Publication Date
October 1, 1991
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 103
ISSN: 0004-6280
Subject Category
Astronomy
Accession Number
92A12633
Funding Number(s)
CONTRACT_GRANT: NAS5-30386
CONTRACT_GRANT: NSF ATM-89-01689
Distribution Limits
Public
Copyright
Other

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