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insulators and Weyl semimetals. The former favours quantum states of matter (e.g. excitonic superfluidity, quantum magnetism, superconductivity), while the latter makes their optical and transport properties
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, spectroscopy, astrometry) using massive optical telescopes on Earth and in space (e.g., Hubble, Gaia, JWST, Kepler, TESS). My group develops cutting-edge models to extract the most from noisy data and to better
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My primary areas of research activity are two fold: first, studing thermonuclear (X-ray) bursts from accreting neutron stars; and second, searches for optical counterparts of gravitational-wave
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incorporate other data as well, from gamma-ray burst satellites to optical surveys of flaring supermassive black holes. "Probing the population properties of merging binary black holes with gravitational waves
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Zealand and Italy. "Structuring x-ray light to investigate the macro and microscale" "Dark-field x-ray imaging without optics" "Adding time to the X-ray Fokker-Planck Equation" (with Prof David Paganin