|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
WMAP polarization observations: seeing through the Galaxy
If you have a question about this talk, please contact Antony Lewis.
Current polarization measurements from WMAP provide information about the reionization epoch. However, WMAP observes significant levels of polarized radiation from our Galaxy. I will present a sampling method for estimating the polarized CMB maps, marginalizing over Galactic contributions. I will show the application of this method to the five year WMAP data, where we find that the large scale polarized CMB signal is consistent with the standard ‘template-cleaned’ result. The synchrotron emission is found to have mean index ~ -3.0 in regions of high signal to noise. The large scale polarized CMB is also used to search for a background of gravitational waves from inflation in the early universe, so I’ll discuss the application to future estimation of this primordial signal.
This talk is part of the Cosmology lunch series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsBiological and Statistical Physics discussion group (BSDG) Engineers Without Borders Panel Talks firstname.lastname@example.org
Other talksThe neglected Giant: Incontinence and ageing Replication restart and mechanisms of replication-associated genome rearrangement Recent results from the T2K experiment Working Title: Aspects of Globular Ethics and Energy Poetry’s Role in Leningrad Samizdat