Data Reduction & Analysis Recipes for LWS

New LWS data reduction & analysis recipes are now available. They are structured as worked examples for all AOT types. Recipes for different source strenghts are present when there are steps in the data reduction which are critical for sources in a specific flux range. We plan to regularly update these recipes with hints & tips on practical ``user cases'' as needed, based on inputs from the users community.

LWS01 - Wavelength range Grating scans

Faint source (http://www.ipac.caltech.edu/iso/lws/lia/lws/01_faint.html )
Medium brightness source (http://www.ipac.caltech.edu/iso/lws/lia/lws01_medium.html)
Bright source (http://www.ipac.caltech.edu/iso/lia/lws/01_strong.html)

LWS02 - Grating Line scans

Faint source (and all others...) (http://www.ipac.caltech.edu/iso/lws/lia/lws02_faint.html)

LWS04 - Fabry-Perot Line scans (http://www.ipac.caltech.edu/iso/lws/lia/fpproc.html)

For any questions about these recipes, or any help you may need in the reduction of your LWS data, please contact us at iso@ipac.caltech.edu if you are in the U.S., or helpdesk@iso.vilspa.esa.es if you are in Europe.

If your question concerns the use of the ISO Spectral Analysis Package (ISAP), please contact isap@ipac.caltech.edu.

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Last Updated: 15 September 1999