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astronomy
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Update README.md

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@@ -70,7 +70,7 @@ Both input and output data is multiplied with an alpha coefficient.
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  For the inputs, Fourier components, it is for normalization.
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  For the outputs, reconstructed solar flare images, it is to have a steady flux intensity range.
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- ![Overall Framework](images/framework)
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  #### Training Hyperparameters
@@ -116,7 +116,7 @@ Carbon emission is estimated using the [Machine Learning Impact calculator](http
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  - **Hours used:** 2.5 hours
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  - **Training Type:** Standard training
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- ![CO2eq](images/co2_eq)
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  ## Technical Specifications
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@@ -124,7 +124,7 @@ Carbon emission is estimated using the [Machine Learning Impact calculator](http
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  Overcomplete Autoencoder trained in a supervised manner to reconstruct solar flare images from the Fourier components.
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- ![Model Architecture](images/model_arch)
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  ### Compute Infrastructure
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  For the inputs, Fourier components, it is for normalization.
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  For the outputs, reconstructed solar flare images, it is to have a steady flux intensity range.
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+ ![Overall Framework](images/framework.png)
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  #### Training Hyperparameters
 
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  - **Hours used:** 2.5 hours
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  - **Training Type:** Standard training
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+ ![CO2eq](images/co2_eq.png)
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  ## Technical Specifications
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  Overcomplete Autoencoder trained in a supervised manner to reconstruct solar flare images from the Fourier components.
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+ ![Model Architecture](images/model_arch.png)
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  ### Compute Infrastructure
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