Speaker
Elisa Russier
(Lawrence Berkeley National Laboratory)
Description
Polarized dust emission is one of the major foreground contaminants in CMB data. With increasing sensitivity and resolution in new CMB experiments, we need dust models in polarization that reflect the data both at large and small angular scales. In this talk, I will present new polarized dust maps using Planck PR4 data which improve on the existing GNILC PR3 maps.
| Would you be interested in presenting a poster if the conference is oversubcribed? | No |
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Primary author
Elisa Russier
(Lawrence Berkeley National Laboratory)
Co-authors
Dr
Jacques Delabrouille
(Centre Pierre Binétruy)
Dr
Shamik Ghosh
(Lawrence Berkeley National Laboratory)
