TL;DR
This study investigates how layer-wise fine-tuning of deep neural networks affects the classification accuracy of astronomical bodies in the SDSS-IV dataset, revealing that optimal tuning varies by architecture.
Contribution
It provides a detailed analysis of layer-wise fine-tuning strategies across multiple architectures for astronomical classification, highlighting the importance of specific training ratios and tuning levels.
Findings
Different architectures respond uniquely to fine-tuning levels.
Optimal models require specific training ratios and layer tuning.
Mobile networks may underperform despite smaller size.
Abstract
The SDSS-IV dataset contains information about various astronomical bodies such as Galaxies, Stars, and Quasars captured by observatories. Inspired by our work on deep multimodal learning, which utilized transfer learning to classify the SDSS-IV dataset, we further extended our research in the fine tuning of these architectures to study the effect in the classification scenario. Architectures such as Resnet-50, DenseNet-121 VGG-16, Xception, EfficientNetB2, MobileNetV2 and NasnetMobile have been built using layer wise fine tuning at different levels. Our findings suggest that freezing all layers with Imagenet weights and adding a final trainable layer may not be the optimal solution. Further, baseline models and models that have higher number of trainable layers performed similarly in certain architectures. Model need to be fine tuned at different levels and a specific training ratio is…
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Taxonomy
MethodsDepthwise Convolution · Pointwise Convolution · Softmax · Batch Normalization · Average Pooling · Dense Connections · 1x1 Convolution · Residual Connection · Depthwise Separable Convolution · Global Average Pooling
