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DTSTART;TZID=America/Los_Angeles:20181116T120000
DTEND;TZID=America/Los_Angeles:20181116T130000
DTSTAMP:20260526T161929
CREATED:20180917T155219Z
LAST-MODIFIED:20181107T194052Z
UID:434-1542369600-1542373200@inpa.lbl.gov
SUMMARY:Andrej Dvornik (UNLV) - KiDS and biases
DESCRIPTION:The current ongoing large imaging surveys are an excellent tool for studying the origin and evolution of the Universe and the galaxy – dark matter connection\, using the weak gravitational lensing as the main probe. Using the predicting power of the halo model formalism\, the weak gravitational lensing (together with other large scale probes) can be used to constrain the origin of the scale dependence of the galaxy bias – the relation between the galaxies and the dark matter distribution\, as well as studying the dependence of the formation time of galaxies on their halo masses – so called assembly bias. In this talk I will present the KiDS survey and way it can be used to shine a light on the different aspects of galaxy-halo connection.
URL:https://inpa.lbl.gov/event/andrej-dvornik-unlv/
LOCATION:50A-5132- Sessler\, 50A-5132 Sessler Conference Room\, CA
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