Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision 		Previous revision
start [2012/11/08 22:49]
mjc fleshing out first filled version 		start [2025/07/03 00:18] (current)
onken Updates for v2
Line 1: Line 1:
 [[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: 
 +  * [[http://adsabs.harvard.edu/abs/2007Ap%26SS.310..255D| Dopita et al. (2007), ApSS, 310, 255]] 
 +  * [[http://adsabs.harvard.edu/abs/2010Ap%26SS.327..245D| Dopita et al. (2010), ApSS, 327, 245]] 
 + 
 +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]]
Back to top