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- Test_1: | ||
- Normal (vanilla) transformer trained on GALACTIC data. At this point we did not have the confusion matrix plots. At this point, we had a Linear embedding for the data before entering into the transformer. | ||
- Test_1_Convs: | ||
- This was a try to train a simple convolutional model on the data, but we did not have the confusion matrices plots yet. We can retrain it whenever is necessary. | ||
- Test_2: | ||
- Same test as 'Test_1' but we added the confusion matrices. | ||
- Test_3: | ||
- Same test as 'Test_2' but we changed the Linear embedding to a Conv embedding. The performance was a little better, but there was not a difference such as the one we observe in the reference paper. | ||
- Test_3_with_errors: | ||
- Same test as 'Test_3' but we consider 2 inputs of 6 channels each one independently for the brightness and for the uncertainty respectively. | ||
- Test_ZEROES: | ||
- Sample test where we interpolated using zeroes instead of the Gaussian process. | ||
- Test_4_multiply_errors: | ||
- Test with a transformer using as input the brightness multiplied by the inverse of the square root of the uncertainty obtained from the Gaussian interpolation process, i.e., ( 1/sqrt(error) ) * brightness. Therefore, there will be only one input of 6 channels. | ||
- Test_4: | ||
- Same test as 'Test_3' but considering the same weight for all labels. | ||
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All these tests have been done for the GALACTIC data. Furthermore, we have considered, regarding the loss function, a weighting that goes in an inverse manner with the frequency of each class thereby giving more 'importance' to those classes with less representation within the dataset. | ||
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