en:praktikum:sternspektren_baches

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en:praktikum:sternspektren_baches [2023/11/30 17:54] – Immer noch, vermuteter Tippfehler jmkubaten:praktikum:sternspektren_baches [2024/03/20 09:29] (current) – [Plotting the spectrum] rhainich
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       Flatdarks/       Flatdarks/
       ...       ...
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 +<color #ed1c24>**Note:**</color> **This folder structure is essential for some data reduction steps. It is therefore essential that the files are sorted accordingly!**
  
 There are different tools to view the FITS files (two dimensional CCD images or data tables). //ds9// is easy to handle and can be started from the terminal via: There are different tools to view the FITS files (two dimensional CCD images or data tables). //ds9// is easy to handle and can be started from the terminal via:
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 If you want to mirror the recordings you have to set ''flip_images'' to ''True''. If the images should also be binned, set ''bin_images'' to ''True''. The binning factor can be determined via the variable ''binning_value''. If you want to mirror the recordings you have to set ''flip_images'' to ''True''. If the images should also be binned, set ''bin_images'' to ''True''. The binning factor can be determined via the variable ''binning_value''.
  
 +**Important:** When the data reduction is finished, disable the virtual environment with
 +
 +   deactivate
  
 ===== Data analysis ===== ===== Data analysis =====
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 {{section>deng:praktikum:a12:python#English&noheader}} {{section>deng:praktikum:a12:python#English&noheader}}
 +
 +**Important:** Make sure that the virtual environment we used for data reduction is disabled before proceeding:
 +
 +   deactivate
  
 The spectrum should be plotted by means of the python script ''3_printmasterplot.py'', which can be found in the following directory ''~/scripts/n1_baches/''. This script can extract both the total spectrum created by //MIDAS// and the individual spectra of the various orders from the FITS files and then display them.  The spectrum should be plotted by means of the python script ''3_printmasterplot.py'', which can be found in the following directory ''~/scripts/n1_baches/''. This script can extract both the total spectrum created by //MIDAS// and the individual spectra of the various orders from the FITS files and then display them. 
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  • Last modified: 2023/11/30 17:54
  • by jmkubat