Multi-wavelength Studies of Galaxy Clusters and Their Use as Cosmological Probes
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If you have a question about this talk, please contact Dr Jonathan Gair.
The availability of extensive optical measurements of member galaxies, strong and weak gravitational lensing measurements, and resolved X-ray images, afford detailed determination of the galaxy, gas, and dark matter spatial profiles. I will describe the results from combined analyses of high quality multi-wavelength data by implementing a new, largely model-independent approach. I will then show that the contribution of clusters to the the X-ray background can be used to set meaningful constraints on alternative non-Gaussian cosmological models.
This talk is part of the Institute of Astronomy Seminars series.
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