A&A 414, 677-697 (2004)
DOI: 10.1051/0004-6361:20031579
On the analysis of band 3 of the ISO-SWS calibration sources
R. Van Malderen1, L. Decin1, D. Kester2, B. Vandenbussche1, C. Waelkens1, J. Cami3 and R. F. Shipman21 Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium
2 Space Research Organization Netherlands, PO Box 800, 9700 AV Groningen, The Netherlands
3 NASA Ames Research Center, Mail Stop 245-6, Moffett Field, CA 94035-1000, USA
(Received 2 January 2003 / Accepted 2 October 2003 )
Abstract
We analyse ISO-SWS 01 (
)
m (band 3) spectra of the 10 standard calibration stars
with the highest flux using synthetic spectra generated from
(MARCS) atmosphere models. The comparison between the observed
and synthetic spectra reveals the quality of (1) the atmospheric model
construction and subsequent synthetic spectra computation and of (2)
the (OLP 10.1) calibration and data reduction of the spectrometer at
these wavelengths.
Key words: stars: atmospheres -- stars: fundamental parameters -- instrumentation: spectrographs -- molecular data
Offprint request: R. Van Malderen, Roeland.VanMalderen@ster.kuleuven.ac.be
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© ESO 2004

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