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        <description>This was the beginning of an effort to document the options available for each step of the pipeline. For an up-to-date and complete implementation of this kind of documentation, please see the  ReadTheDocs site.

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Raising Issues

To get support for PyWiFeS problems from version 2 onwards, please raise an issue in  the GitHub repository.

Mailing List

There is a pywifes mailing list, although this has had little use in recent years.  To be added to this list, please contact Jon Nielsen (</description>
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 In version 2 of PyWiFeS, the association of the pipeline steps with their particular file suffixes from the table below has been retained. But note that the final datacubes are renamed from p11.fits to cube.fits. In addition, regarding footnote C, standard stars are now identified by header keyword IMAGETYP='STANDARD' with a user option to also grab any IMAGETYP='OBJECT' exposures with sky positions close to the tabulated standard stars.</description>
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 With version 2 of PyWiFeS, baseline calibrations are not provided, but should be available from the WiFeS data archive under the automated 2.3m telescope operations. However, the general principles below still hold. In addition, note that dark frames are not recommended because the dark current in the detectors (as of 2025 and going back to at least 2013) are below 1 ADU/hour.</description>
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From version 0.7.0 of PyWiFeS, we have migrated the code to a GitHub repository:
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The processes in version 2 of PyWiFeS largely build upon the excellent work of the previous PyWiFeS developers. Thus, we retain the original documentation here, but note that several aspects have undergone significant revision in the current version, described in Onken et al. (in prep). Documentation for the new processes may also be found in</description>
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 The usage of PyWiFeS has been modified for version 2. Please disregard these instructions and follow those on  our ReadTheDocs site.

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        <title>optical_fit_wifes.png - removed</title>
        <link>https://www.mso.anu.edu.au/pywifes/doku.php?image=optical_fit_wifes.png&amp;ns=&amp;rev=1378358375&amp;tab_details=history&amp;mediado=diff&amp;do=media</link>
        <description></description>
    </item>
</rdf:RDF>
