Video URL
https://pirsa.org/16040056Results from Planck 2015
APA
Frolov, A. (2016). Results from Planck 2015. Perimeter Institute for Theoretical Physics. https://pirsa.org/16040056
MLA
Frolov, Andrei. Results from Planck 2015. Perimeter Institute for Theoretical Physics, Apr. 26, 2016, https://pirsa.org/16040056
BibTex
@misc{ scivideos_PIRSA:16040056, doi = {10.48660/16040056}, url = {https://pirsa.org/16040056}, author = {Frolov, Andrei}, keywords = {Cosmology}, language = {en}, title = {Results from Planck 2015}, publisher = {Perimeter Institute for Theoretical Physics}, year = {2016}, month = {apr}, note = {PIRSA:16040056 see, \url{https://scivideos.org/index.php/pirsa/16040056}} }
Andrei Frolov Simon Fraser University (SFU)
Abstract
Planck's full-mission data, released in 2015, provides a high-resolution whole-sky polarization and temperature maps of the CMB and astrophysical components. I will talk about implications of Planck 2015 results for inflation, why cosmic dust is important, and what we are currently doing to study it. I will also highlight some tests of the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies we have done with observations made by the Planck satellite. I will show how simple map stacking can be used as a powerful statistical tool for studying polarized CMB and dust emission maps.