Travis Mong

"Learn from yesterday, live for today, hope for tomorrow.
The important thing is not to stop questioning."

Albert Einstein

November 4, 2022

Self-supervised clustering on image-subtracted data
with Deep-Embedded Self-Organizing Map

DESOM

Developing an effective automatic classifier to separate genuine sources from artifacts is essential for transient follow-ups in wide-field optical surveys. The identification of transient detections from the subtraction artifacts after the image differencing proccess is a key step in such classifiers, known as real-bogus classification problem. I applied a self-supervised machine learning model, the deep-embedded self-organizing map (DESOM) to this 'real-bogus' classification problem. DESOM combines an autoencoder and a self-organizing map to perform clustering in order to distinguish between real and bogus detections, based on their dimensionality-reduced representations. I used 32x32 normalized detection thumbnails as the input of DESOM. I demonstrated different model training approaches, and find that the best DESOM classifier shows a missed detection rate of 6.6% with a false positive rate of 1.5%⁠. DESOM offers a more nuanced way to fine-tune the decision boundary identifying likely real detections when used in combination with other types of classifiers, for example built on neural networks or decision trees.

September 7, 2021

Searching for Fermi GRB optical counterparts with the prototype Gravitational-wave Optical Transient Observer (GOTO)

GOTO GRB

I reviewed 53 Fermi-GRB events followed up by GOTO. This project includes data extraction from GOTO PostgreSQL database, data cleaning and visualization with Python, and temporal data analysis. I systematically narrowed down the number of the transient candidates from 60,085 to 29. My results show that GOTO can effectively search for GRB optical counterparts thanks to its large field of view of ~40 sq.degrees and its depth of ~20 mag. I also detailed several methods to improve our overall performance for future follow-up programmes of Fermi GRBs.