Orateur
Description
I report on preliminary results from a collaborative project between the Supernova Remnants and Cosmic Ray Group, the Observatory of Complex Systems Group, and the Quantum Theory Group at the University of Palermo.
By adopting different dendrogram-based techniques, we developed a tool to quantitatively measure the similarities among different narrow-band images of a supernova remnant and of different supernova remnants. We tested our tool on Chandra observations of Cassiopeia A, Tycho's SNR, Kepler's SNR, W49B, and G292.0+01.8. We identified clusters of different chemical elements in Type Ia and core-collapse remnants and obtained interesting clues on the origin of W49B.
I also present the methodology we developed to adopt Quantum Extreme Learning Machines for the retrieval of the best-fit parameters of optically-thin X-ray spectra. I will show preliminary results obtained by using a real quantum computer as a reservoir for the training of the deep learning algorithm.