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The recalibration of the IUE scientific instrumentThe IUE instrument was recalibrated because of long time-scale changes in the scientific instrument, a better understanding of the performance of the instrument, improved sets of calibration data, and improved analysis techniques. Calibrations completed or planned include intensity transfer functions (ITF), low-dispersion absolute calibrations, high-dispersion ripple corrections and absolute calibrations, improved geometric mapping of the ITFs to spectral images, studies to improve the signal-to-noise, enhanced absolute calibrations employing corrections for time, temperature, and aperture dependence, and photometric and geometric calibrations for the FES.
Document ID
19890007232
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Imhoff, Catherine L.
(Computer Sciences Corp. Lanham, MD., United States)
Oliversen, Nancy A.
(Computer Sciences Corp. Lanham, MD., United States)
Nichols-Bohlin, Joy
(Computer Sciences Corp. Lanham, MD., United States)
Casatella, Angelo
(IUE Observatory Lanham, MD., United States)
Lloyd, Christopher
(European Space Agency. ESA Tracking Station Madrid, Spain)
Date Acquired
September 5, 2013
Publication Date
June 1, 1988
Publication Information
Publication: ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2
Subject Category
Astronomy
Accession Number
89N16603
Distribution Limits
Public
Copyright
Other
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