Fingerprints of structure formation in the microwave background ...
Non-linear structures in the universe leave characteristic imprints in the cosmic microwave background. These include Compton scattering (Sunyaev-Zeldovich effects) and gravitational lensing. The South Pole Telescope now has a catalog of massive galaxy clusters that were discovered this way, along w...
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Perimeter Institute
2010
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Online Access: | https://dx.doi.org/10.48660/10040090 https://pirsa.org/10040090 |
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ftdatacite:10.48660/10040090 2024-03-31T07:55:23+00:00 Fingerprints of structure formation in the microwave background ... 2010 video/mp4 https://dx.doi.org/10.48660/10040090 https://pirsa.org/10040090 en eng Perimeter Institute Cosmology Audiovisual Video Recording article MediaObject 2010 ftdatacite https://doi.org/10.48660/10040090 2024-03-04T13:30:01Z Non-linear structures in the universe leave characteristic imprints in the cosmic microwave background. These include Compton scattering (Sunyaev-Zeldovich effects) and gravitational lensing. The South Pole Telescope now has a catalog of massive galaxy clusters that were discovered this way, along with a measure of the background fluctuations generated by smaller clusters, that can be used to chart the growth of structure in the universe. ... Article in Journal/Newspaper South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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Open Polar |
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DataCite Metadata Store (German National Library of Science and Technology) |
op_collection_id |
ftdatacite |
language |
English |
topic |
Cosmology |
spellingShingle |
Cosmology Fingerprints of structure formation in the microwave background ... |
topic_facet |
Cosmology |
description |
Non-linear structures in the universe leave characteristic imprints in the cosmic microwave background. These include Compton scattering (Sunyaev-Zeldovich effects) and gravitational lensing. The South Pole Telescope now has a catalog of massive galaxy clusters that were discovered this way, along with a measure of the background fluctuations generated by smaller clusters, that can be used to chart the growth of structure in the universe. ... |
format |
Article in Journal/Newspaper |
title |
Fingerprints of structure formation in the microwave background ... |
title_short |
Fingerprints of structure formation in the microwave background ... |
title_full |
Fingerprints of structure formation in the microwave background ... |
title_fullStr |
Fingerprints of structure formation in the microwave background ... |
title_full_unstemmed |
Fingerprints of structure formation in the microwave background ... |
title_sort |
fingerprints of structure formation in the microwave background ... |
publisher |
Perimeter Institute |
publishDate |
2010 |
url |
https://dx.doi.org/10.48660/10040090 https://pirsa.org/10040090 |
geographic |
South Pole |
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South Pole |
genre |
South pole |
genre_facet |
South pole |
op_doi |
https://doi.org/10.48660/10040090 |
_version_ |
1795037204276314112 |