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KICP People
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![]() Surhud More KICP Fellow Ph.D., Astronomy/Astrophysics, Max Planck Institute for Astronomy, 2009 Research
Research Interests: Structures in the Universe; Theory
I am a postdoctoral fellow at the Kavli Institute for Cosmological Physics at the University of Chicago and part of the Computational Astrophysics Group of Andrey Kravtsov. Prior to that, I was in the Theory group of the Galaxies and Cosmology section at the Max Planck Institute for Astronomy. I worked with Dr. Frank van den Bosch and my phd thesis focussed on understanding the Galaxy-Dark Matter Connection. Halo Mass-Luminosity Relation of Central Galaxies in SDSS According to our current understanding, galaxies are believed to reside in extended dark matter haloes. The properties of a dark matter halo, in particular its mass, shapes the properties of the galaxy that forms at its center. I am interested in the scaling relations between galaxy properties and halo mass. I have investigated the halo mass-luminosity relationship of galaxies. The kinematics of satellite galaxies can be used to infer the mass of the halo of a galaxy. I have developed methods to reliably obtain the mean and the scatter of the halo mass-luminosity relation of galaxies and applied it to the Sloan Digital Sky Survey. Cosmic Transparency The Universe is remarkably transparent. Photons from distant cosmic objects travel to us, uninhibited, despite encountering considerable columns of dark matter, hydrogen plasma, hydrogen gas and dust. In a research project, in collaboration with David Hogg and Jo Bovy, we recently obtained a quantitative measure of the transparency of the Universe by testing the Etherington relation using current SNeIa and Baryon acoustic feature measurements. Ongoing Scientific Projects: Talks, Lectures, & Workshops
KICP Publications
2012 | 2011 | 2010
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