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Simon Berg (University of Oslo)09/09/2026, 11:00
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Simon Silverstein (University of Oslo)09/09/2026, 11:00
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Valentina Genesini09/09/2026, 11:00
The imprint of the Epoch of Reionization is encoded in the large-scale E-mode polarization of the CMB, which provides a direct constraint on the Thomson optical depth, $\tau$. Despite the high quality of the Planck and WMAP datasets, a fully consistent framework that jointly exploits all available large-scale polarization information has so far been lacking.
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To address this, we have developed... -
Synne Jørgensen (University of Oslo)09/09/2026, 11:00
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Diana Victoria Lopez Navarro (Bonn University)09/09/2026, 11:00
The scattering of the CMB photons off of free electrons contained within the intracluster medium (ICM) of galaxy clusters gives rise to the Sunyaev-Zel’dovich (SZ) effect. Typically, this effect can be separated into two components: the thermal and the kinematic SZ effect. The latter arises from contributions from bulk and internal motion of the gas, including rotational motion. Recent studies...
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Kaustuv Basu (Bonn University)09/09/2026, 11:00
We present the latest updates from the CCAT scientific collaboration, which is finishing the construction of its state-of-the-art Fred Young Submillimeter Telescope (FYST), at an altitude of 5600 m in the Atacama plateau in Chile. The telescope construction is nearly complete and the installation of the first-light cameras are in progress. We specifically highlight the status and the science...
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