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Signal-to-noise ratios in IUE low-dispersion spectra. II - Photometrically corrected imagesPhotometrically corrected images from the IUE's two intensified vidicon cameras are used to explore the character of detector noise, and a protocol for the derivation of realistic noise models is proposed on the basis of available collections of UV-Flood calibration images. The incomplete removal of the pixel-to-pixel sensitivity pattern can lead to a factor-of-2 enhancement in apparent noise; even with good suppression of pixel granularity, the remaining random noise can exhibit saturation behavior which causes S/N to cease improving with increasing exposure. When all relevant effects are considered, underlying, 'pristine' noise models show virtually no dependence on spatial position.
Document ID
19930057075
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ayres, Thomas R.
(Colorado Univ. Boulder, United States)
Date Acquired
August 16, 2013
Publication Date
May 1, 1993
Publication Information
Publication: Astronomical Society of the Pacific, Publications
Volume: 105
Issue: 687
ISSN: 0004-6280
Subject Category
Astronomy
Accession Number
93A41072
Funding Number(s)
CONTRACT_GRANT: NAG5-1215
Distribution Limits
Public
Copyright
Other

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