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Infrared space observatory photometry of circumstellar dust in Vega-type systemsThe ISOPHOT (Infrared Space Observatory Photometry) instrument onboard the Infrared Space Observatory (ISO) was used to obtain 3.6-90 micron photometry of Vega-type systems. Photometric data were calibrated with the ISOPHOT fine calibration source 1 (FCS1). Linear regression was used to derive transformations to make comparisons to ground-based and IRAS photometry systems possible. These transformations were applied to the photometry of 14 main-sequence stars. Details of these results are reported on.
Document ID
19980219279
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Fajardo-Acosta, S. B. (Denver Univ. Denver, CO United States)
Stencel, R. E. (Denver Univ. Denver, CO United States)
Backman, D. E. (Franklin and Marshall Coll. Lancaster, PA United States)
Thakur, N. (Denver Univ. Denver, CO United States)
Date Acquired
August 18, 2013
Publication Date
April 1, 1998
Publication Information
Publication: Exozodiacal Dust Workshop
Subject Category
Astronomy
Funding Number(s)
CONTRACT_GRANT: NAG5-3411
CONTRACT_GRANT: NAGw-3680
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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