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calibration_files [2012/11/09 03:39]
mjc created
calibration_files [2025/07/03 00:38] (current)
onken Update for v2
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 ====== Calibration Files ====== ====== Calibration Files ======
-This page is a repository of baseline calibration files to be used in circumstances where observers were unable to obtain those data during their run.+** 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. ** 
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 +This page will ultimately be a repository of baseline calibration files to be used in circumstances where observers were unable to obtain those data during their run.  The file formats changed in v0.5.0 so previous calibration files were removed.  An update email will be sent when these files are available again.  (MC: 2015-Apr-28)
  
 The calibration files needed to fully process the data are: The calibration files needed to fully process the data are:
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   * Telluric correction (red side)   * Telluric correction (red side)
  
-To fix this, you need merely go to the repository below and choose the appropriate files for your given setup.  Be sure to point your reduction script to these new files. 
  
-=== Baseline Calibration Files === 
-Here will be the files...