Galaxy halo masses and implications for galaxy evolution from weak lensing measurements (speaker: Rachel Mandelbaum, Carnegie Mellon University)

Date: 
Tuesday, March 15, 4:00pm
Location: 
Marlar Lounge (37-252)

Abstract:
In the past decade, weak gravitational lensing has become one of the best ways of measuring the masses of the extended dark matter halos in which galaxies reside.  Measurements of the dark matter halo masses for galaxies with a given luminosity or stellar mass (observable mass proxies) have revealed a great deal about the connection between halo masses and these more easily observable quantities.  After an overview of what such measurements have shown us before, I will describe some recent measurements in the Sloan Digital Sky Survey that illustrate a bimodality in dark matter halo mass at fixed galaxy stellar mass, with red galaxies (with older stellar populations) having dark matter halo masses a factor of 2-3 larger than blue galaxies (younger stellar populations).  I will discuss the implications of these results for models of galaxy formation and evolution, and also propose future measurements with upcoming datasets that will shed further light on the relevant galaxy formation and evolution processes.

Host: Michael McDonald

 

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Image: galaxies in the Hubble Ultra Deep field

Image source:  Hubble Space Telescope image gallery