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My PhD Thesis


Hello! Welcome to my thesis page. Here I share my PhD project within the EDUCADO program, where I study faint structures in CO spectral-line datacubes from ALMA. My goal is to detect and analyse subtle features in galaxies that are often hidden in traditional data analysis.



Project Summary


My project is all about uncovering faint, one-dimensional structures in high-resolution astronomical datacubes. I combine data cleaning and processing with a machine learning toolbox called 1‑DREAM (Canducci et al. 2022) and kinematic modelling using BBarolo (Enrico & Fraternali 2015c).

First, I transform a galaxy datacube (like NGC 4303) into a point cloud. This allows 1‑DREAM to detect filaments that are hard to spot otherwise. The data is carefully cleaned, normalised, and stretched to reveal faint structures while keeping the bright regions in check.

Interactive visualisation of the NGC 4303 point cloud.

Then, 1‑DREAM identifies filamentary structures in the point cloud.


Interactive visualisation of the NGC 2775 point cloud with filamentary structures detected by 1-DREAM overlaid.

This is followed by BBarolo modelling, which produces residual velocity cubes. Comparing the filaments with the residuals helps validate that the detected structures are real and physically meaningful.


Video visualisation of the NGC 4303 ALMA datacube
Video visualisation of the NGC 4303 ALMA datacube across all spectral channels, showing the BBarolo kinematic model and the resulting residuals.

Future Ideas