
https://github.com/csabiu/KAML-2025/blob/main/KAML_images.ipynb
Suk Kim (CNU)
Key Challenges Identified:
• Data Imbalance: The current dataset is unbalanced across morphological types, especially for complex structures, making It harder to find similar images for underrepresented types.
• Latent Feature Bias: The latent features are sometimes biased towards global characteristics like color and overall shape, rather than detalled structures such as spiral arms or bars, leading to misclassifications. The model can also struggle to reconstruct delicate, faint structures.
Planned Solutions:
• Data Augmentation: Use Variational Autoencoders (VAEs) to generate diverse images, enriching the dataset for sparse morphological types and enhancing diversity.
• Improved Training Data: Incorporate residual images from galaxy-profile fitting Into the training data. This is intended to highlight and emphasize the detailed structural features crucial for accurate classification, helping to mitigate the bias towards color and shape.
• Feature Analysis: Further examine the correlation between latent features and photometric parameters to better understand and refine their relative significance in similarity calculations.
To effectively integrate machine learning into astronomy, the following initiatives are essential:
(1) Systematic Database Development
Purpose-Built Databases: