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--- information_for_astronomers:user_guide:semi-automatic_reduction_of_spectroscopic_measurements_-_a_cookbook [2019/09/03 16:59]
akraus created
+++ information_for_astronomers:user_guide:semi-automatic_reduction_of_spectroscopic_measurements_-_a_cookbook [2020/06/11 11:10] (current)
akraus
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 ====== Semi-automatic reduction of spectroscopic observations ======
-**Under develpoment**
+**Under development**
 This is meant as a cookbook describing the procedures for analyzing the
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-Compile a list of appropriate scans for the continuum pipeline. In case of just one used frequency it might be sufficient to give the first and the last frequency to the pipeline. It might, however, be useful to have a file with the scans of interest.
+Compile a list of appropriate scans for the continuum pipeline. In case of just one used frequency it might be sufficient to give the first and the last scan to the pipeline.
+It might, however, be useful to have a file with the scans of interest.
 Run the continuum pipeline with
@@ Line 33: / Line 34: @@
 The output file can be freely chosen, the selection of input files should be appropriate to accelerate the calculations. It is recommend that the
 output of the pipeline is stored for further references - just in case.
+In the file xxxxxx_cal.100m (in this example 20190618_cal.100m) you find all spectra
+observed (i.e. all subscans) calibrated in Jy (or in K T_MB).
 What is left to do is:

Effelsberg 100m Teleskop