206 citations
- The University of MelbourneAU12 papers
- Fermi National Accelerator LaboratoryUS6 papers
- Argonne National LaboratoryUS4 papers
- Kavli Institute for Particle Astrophysics and CosmologyUS4 papers
- Menlo SchoolUS4 papers
- Netherlands Institute for Radio AstronomyNL4 papers
- SLAC National Accelerator LaboratoryUS4 papers
- Stanford UniversityUS4 papers
- University of California, BerkeleyUS4 papers
- Astrobiology CenterJP3 papers
- Electronics for Imaging (United States)US3 papers
- Harvard UniversityUS3 papers
Showing astro-ph.COShow all
3 papers · 1 filter
astro-ph.CO2025
Measurements of the Temperature and E-mode Polarization of the Cosmic Microwave Background from the Full 500-square-degree SPTpol Dataset
T. -L. Chou, P. A. R. Ade, A. J. Anderson +59
Using the full four-year SPTpol 500 deg dataset in both the 95 GHz and 150 GHz frequency bands, we present measurements of the temperature and -mode polarization of the cosm…
astro-ph.CO2024
Constraints on gravity from tSZE-selected SPT galaxy clusters and weak lensing mass calibration from DES and HST
S. M. L. Vogt, S. Bocquet, C. T. Davies +52
We present constraints on the gravity model using a sample of 1,005 galaxy clusters in the redshift range that have been selected through the thermal Sunyaev-Z…
astro-ph.CO2022
Forecasting ground-based sensitivity to the Rayleigh scattering of the CMB in the presence of astrophysical foregrounds
Karia R. Dibert, Adam J. Anderson, Amy N. Bender +9
The Rayleigh scattering of cosmic microwave background (CMB) photons off the neutral hydrogen produced during recombination effectively creates an additional scattering surface aft…