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In search of random noiseIn order to make the best high resolution images of IRAS data it is necessary to incorporate any knowledge about the instrument into a model: the IRAS model. This is necessary since every remaining systematic effect will be amplified by any high resolution technique into spurious artifacts in the images. The search for random noise is in fact the never-ending quest for better quality results, and can only be obtained by better models. The Dutch high-resolution effort has resulted in HIRAS which drives the MEMSYS5 algorithm. It is specifically designed for IRAS image construction. A detailed description of HIRAS with many results is in preparation. In this paper we emphasize many of the instrumental effects incorporated in the IRAS model, including our improved 100 micron IRAS response functions.
Document ID
19950015336
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kester, DO
(Groningen Rijksuniv. Netherlands)
Bontekoe, Tj. Romke
(European Space Agency. European Space Research and Technology Center ESTEC, Noordwijk, Netherlands)
Date Acquired
September 6, 2013
Publication Date
April 1, 1994
Publication Information
Publication: JPL, Science with High Spatial Resolution Far-Infrared Data
Subject Category
Documentation And Information Science
Accession Number
95N21753
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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