The first ISO workshop on analytical spectroscopy with SWS, LWS, PHT-S and CAM-CVF

(Oct 6-8, 1997, Madrid, Spain)

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A. Salama tex2html_wrap_inline448 , H. Feuchtgruber tex2html_wrap_inline450 , A. Heras tex2html_wrap_inline448 , F. Lahuis tex2html_wrap_inline454 ,
K. J. Leech tex2html_wrap_inline448 , R. Lorente tex2html_wrap_inline448 , P. Morris tex2html_wrap_inline460 , B. Vandenbussche tex2html_wrap_inline462 & E. Wieprecht tex2html_wrap_inline450
With contributions from the SWS Instrument Support Teams tex2html_wrap_inline466

tex2html_wrap_inline448 ISO Science Operations Centre, Astrophysics Division, ESA SSD, Villafranca, 28080 Madrid, Spain
tex2html_wrap_inline470 Max-Planck-Institut für extraterrestrische Physik, Giessenbachstr. 1, D-85748 Garching, Germany
tex2html_wrap_inline472 SRON, P.O. Box 800, 9700 AV Groningen, The Netherlands
tex2html_wrap_inline474 SRON, CA 3584 Utrecht, The Netherlands
tex2html_wrap_inline476 Instituut voor Sterrenkunde, University of Leuven, Celestijnenlaan 200B, B-3001 Heverlee, Belgium


An overview of the current status of the SWS instrument and its calibration is given. Guidance is given to observers concerning data reduction, what instrumental artifacts may contaminate their data and where further information may be obtained from.

Key words: ISO; SWS

Postscript version (gzip-ped)

A. Salama et al.