public:user_software:prefactor

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public:user_software:prefactor [2019-02-25 09:13] – [Software requirements] David Raffertypublic:user_software:prefactor [2019-02-25 09:15] – [To do list] David Rafferty
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 ==== Documentation ==== ==== Documentation ====
  
-Installation and setup is explained in the preliminary version of a cookbook chapter at: https://github.com/lofar-astron/prefactor/blob/pdf-doc/docs/cookbook_prefacet.pdf \\ +Installation and setup is explained at the GitHub page: https://github.com/lofar-astron/prefactor \\ 
 **Please read that first!** **Please read that first!**
  
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     * Calibrator and target data are typically processed separately.     * Calibrator and target data are typically processed separately.
     * The target data can be processed one time- or frequency- block at a time, e.g. when you have limited disk space. (The processed data is a lot smaller than the input data.)     * The target data can be processed one time- or frequency- block at a time, e.g. when you have limited disk space. (The processed data is a lot smaller than the input data.)
-  * Yes, updating the LOFAR software can be annoying. But it is worth ist! Trust me. 8-) 
-  * Get someone to write a better documentation for the genericpipeline. 
   * Don't forget to update the recipe_directories entry in the pipeline.cfg to include the pre-factor plugins, for example: <code> recipe_directories = [%(pythonpath)s/lofarpipe/recipes,/home/rvweeren/software/prefactor]  </code>   * Don't forget to update the recipe_directories entry in the pipeline.cfg to include the pre-factor plugins, for example: <code> recipe_directories = [%(pythonpath)s/lofarpipe/recipes,/home/rvweeren/software/prefactor]  </code>
  
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 https://github.com/lofar-astron/prefactor/issues https://github.com/lofar-astron/prefactor/issues
  
-== FACTOR == 
- 
- 
-  * Time correlation settings given by user. 
-  * Aplpy plots (Tammo has script on his github but change noise to 1mJy (current 5mJy)) 
-  * All WSclean (any aliasing issues?) 
-  * pybdsm boxes from restoring beam size. 
-  * outer uvrange option (maybe good for help create models for selfcalbration when working at full resolution) 
-  * Check that amplitudes are properly normalised 
-  * Second major iteration 
-  * High dynamic range option 
-  * optimize number of IO-intesive (NDPPP) processes 
  • Last modified: 2019-02-25 09:16
  • by David Rafferty