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information_for_astronomers:user_guide:semi-automatic_reduction_of_spectroscopic_measurements_-_a_cookbook
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information_for_astronomers:user_guide:semi-automatic_reduction_of_spectroscopic_measurements_-_a_cookbook [2019/10/29 15:21] akraus |
information_for_astronomers:user_guide:semi-automatic_reduction_of_spectroscopic_measurements_-_a_cookbook [2020/06/11 11:10] akraus |
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| ====== Semi-automatic reduction of spectroscopic observations ====== | ====== Semi-automatic reduction of spectroscopic observations ====== | ||
| - | **Under develpoment** | + | **Under development** |
| This is meant as a cookbook describing the procedures for analyzing the | This is meant as a cookbook describing the procedures for analyzing the | ||
| Line 34: | 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 | 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. | 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: | What is left to do is: | ||
information_for_astronomers/user_guide/semi-automatic_reduction_of_spectroscopic_measurements_-_a_cookbook.txt ยท Last modified: 2020/06/11 11:10 by akraus
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