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Advanced Photometric Analysis for Predicting Specific Star Formation Rates in Large Galaxies

Project Overview

Evaluated the effectiveness of Generative Adversarial Networks (GANs), Conditional GANs (CGANs), and Contrastive GANs (ContraGANs) for generating synthetic data to predict the B-V color index in astronomical datasets. Assessed models based on predictive accuracy, clustering quality, and statistical alignment. ContraGAN outperformed other models with the lowest MSE of 0.1294, highest R² of 0.7258, and superior clustering scores. Highlighted the benefits of contrastive learning and conditional generation for synthetic data applications in scientific and industrial fields.

Key Features

Data Source: Utilizes photometric data from over 27 million galaxies collected by SDSS-DR7.

Algorithms Implemented

Linear Regression

Long Short-Term Memory (LSTM) Networks

Support Vector Regression (SVR)

Random Forest Regressor

Decision Tree Regressor

Gradient Boosting Regressor

Classical Deep Learning Models

Performance Metrics: Evaluates model performance using Mean Absolute Error (MAE) and other relevant metrics. Comparative Analysis: Provides a comprehensive comparison of the performance of different algorithms in estimating SFRs from photometric data.

Contributing

Contributions are welcome! Please submit a pull request or open an issue if you have any suggestions or improvements.

Contact

For any questions or inquiries, please reach out to [satvikraghav007@gmail.com].

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This repo is about predicting specific Star Formation rates using various algorithms

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