Recent and ongoing results from the South Pole Telescope

• Main Author: Manzotti, A.
• Other Authors: Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut Lagrange de Paris
• Format: Conference Object
• Language: English
• Published: HAL CCSD 2018
• Subjects: cosmic background radiation: polarization; polarization; gravitation: lens; cosmological model; dark matter; dark energy; inflation; B-mode; satellite: Planck; Sunyaev-Zel'dovich effect; [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]; South Pole; South pole
• Online Access: https://hal.science/hal-02946228

International audience The Cosmic Microwave Background (CMB) has played a central role in developingthe current standard cosmological model a compelling and elegant description ofthe Universe. However, we still seek a more conclusive test of inflation and aphysical understanding of Dark Matter and Dark energy. The CMB will be, onceagain, a promising dataset to tackle these challenges. I will show the resultsof the analysis of small-scale polarization data from the 10-meter South PoleTelescope (SPT). Then I will present our cosmological parameter constraints fromthe CMB lensing maps reconstructed using combined SPT-SZ and Planck data. I willconclude with an update on the status of the ongoing SPT-Pol B-mode and CMBlensing analysis.