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\textbf{B-101} Identify Tidal Disruption Events (TDEs) and extreme AGN by constructing long-term light curves from difference images using forced photometry. Combine host galaxy properties (e.g., mass, Start Formation Rate, etc) with TDE candidates to build a comprehensive classification. | ||
\textbf{B-201} Detect and characterize microlensing events by analyzing DIA images. Model light curves and assess crowding effects to estimate baseline magnitudes and object properties. | ||
\textbf{B-202} Classify periodic variable stars using a neural network. Improve classification algorithms with DR1 data and develop labeled datasets for future analyses. | ||
\textbf{B-201} Identify Tidal Disruption Events (TDEs) and extreme AGN by constructing long-term light curves from difference images using forced photometry. | ||
Combine host galaxy properties (e.g., mass, Start Formation Rate, etc) with TDE candidates to build a comprehensive classification. | ||
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\textbf{B-202} Detect and characterize microlensing events by analyzing DIA images. | ||
Model light curves and assess crowding effects to estimate baseline magnitudes and object properties. | ||
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||
\textbf{B-203} Classify periodic variable stars using a neural network. | ||
Improve classification algorithms with DR1 data and develop labeled datasets for future analyses. |