Conveners
Foregrounds
- Carlo Baccigalupi (SISSA)
Foregrounds
- Carlo Baccigalupi (SISSA)
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25/05/2022, 09:00
In the recent years it has become clear how the contamination coming from Galactic and extra-Galactic emissions represents one of the main limiting factor for any new science achievable with Cosmic Microwave Background observations. Having a thorough understanding of the foreground properties is therefore fundamental in order to achieve a reliable reconstruction of the clean CMB signal and to...
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25/05/2022, 09:30
Beyond the significant legacy of the ESA's Planck mission, the cosmic microwave background (CMB) radiation carries much more information that remains to be exploited in the coming decades. Next-generation CMB experiments of unprecedented sensitivity are being planned to extract and interpret new cosmological observables out of future CMB data. Among these new, yet undetected, cosmological...
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25/05/2022, 10:00
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25/05/2022, 10:20
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25/05/2022, 11:00
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25/05/2022, 11:20
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25/05/2022, 11:40
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25/05/2022, 12:00
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25/05/2022, 12:20