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start [2015/04/28 03:52]
kim 		start [2025/07/03 00:18] (current)
onken Updates for v2
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 [[start|{{wiki:pywifes_logo.png}}]] [[start|{{wiki:pywifes_logo.png}}]]
 ====== Introduction ====== ====== Introduction ======
-This is the homepage of **pywifes**, a Python-based pipeline for reducing data from the Wide Field Spectrograph (WiFeS).+This is the original homepage of **pywifes**, a Python-based pipeline for reducing data from the Wide Field Spectrograph (WiFeS).
  
-An overview of the instrument itself can be found on its [[http://rsaa.anu.edu.au/observers/observing-rsaa/wifes-information-observers|RSAA webpage]] +**For up-to-date documentation on version 2 of PyWiFeS, please see [[https://pywifes-pipeline.readthedocs.io/en/latest/| our ReadTheDocs page]]** 
-and further details about instrument configurations and observing can be found on the + 
-[[http://www.mso.anu.edu.au/ssowiki/index.php/2.3m_WiFeS|WiFeS Wiki]].+An overview of the instrument itself can be found on its [[https://rsaa.anu.edu.au/observatories/instruments/wide-field-spectrograph-wifes|RSAA webpage]].
  
 If you use WiFeS data in your paper, be sure to cite the Dopita instrument papers: If you use WiFeS data in your paper, be sure to cite the Dopita instrument papers:
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   * [[http://adsabs.harvard.edu/abs/2010Ap%26SS.327..245D| Dopita et al. (2010), ApSS, 327, 245]]   * [[http://adsabs.harvard.edu/abs/2010Ap%26SS.327..245D| Dopita et al. (2010), ApSS, 327, 245]]
  
-We now have a published paper on PyWiFeS, which you can reference to save yourself a 2-page data reduction description in your papers.  The paper is here:+We have a published paper on PyWiFeS **(version 1)**, which you can reference to save yourself a 2-page data reduction description in your papers.  The paper is here:
   * [[http://adsabs.harvard.edu/abs/2014Ap%26SS.349..617C| Childress, Vogt, Nielsen, & Sharp (2014), ApSS, 349, 617]]   * [[http://adsabs.harvard.edu/abs/2014Ap%26SS.349..617C| Childress, Vogt, Nielsen, & Sharp (2014), ApSS, 349, 617]]
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