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@@ -10,12 +10,12 @@ Inspect the *AE_correction.ipynb* notebook for a guide on performing telluric co
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Use *Training.pynb* notebook for understanding the training process of $\texttt{TAU}$ by visualzing network training on a single aperture / order of the data. For training on the entire spectral range of the HARPS-N data use the *training.py* script. The network is trained on solar observations from the HARPS-N spectrograph but can be extended to other spectrographs.
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## Preprocessing data for training
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The procedure for preprocessing data prior to training the network can be seen seen in the *Preproc.ipynb*.
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*Preproc.ipynb* notebook demonstrates the procedure for preprocessing the raw data prior to training the network.
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## Included Data
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Data from HARPS-N used for training $\texttt{TAU}$ is not included in this repository, but can be downloaded from https://dace.unige.ch/dashboard/
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Raw data from HARPS-N is not included in this repository, but can be downloaded from https://dace.unige.ch/dashboard/
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A sample of 100 preprocessed observation is included in the preproc directory and can be used to test the network.
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A sample of 100 preprocessed observations is included in the preproc directory and can be used to test the training procedure of $\texttt{TAU}$.
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The extracted telluric spectrum from training $\texttt{TAU}$ on 838 observations is included in the tellurics directory. This extracted spectrum is used to perform correction with the *telluric_fit* function.
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