I work on the large-scale structure of the Universe and the properties of the massive objects contained within it, using both observation and theory. I am particularly known for making the first detections of the change in brightness of the microwave background radiation caused by inverse-Compton scattering in clusters of galaxies (the Sunyaev-Zel'dovich effect), and in demonstrating how this effect can be used to measure cosmological parameters.
I worked on NASA's Chandra satellite before launch, and use it and other space-based and ground-based telescopes from X-ray to optical to radio bands to study galaxies, especially those hosting massive ...
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