activity
20072023
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 3.3k across the 54 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

38 papers · 1 filter

astro-ph.CO2023★ 67 cited

A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data

Z. Pan, F. Bianchini, W. L. K. Wu +133

We present a measurement of gravitational lensing over 1500 deg of the Southern sky using SPT-3G temperature data at 95 and 150 GHz taken in 2018. The lensing amplitude relativ…

astro-ph.CO2023★ 19 cited

Constraints on axion-like polarization oscillations in the cosmic microwave background with POLARBEAR

The POLARBEAR Collaboration, Shunsuke Adachi, Tylor Adkins +29

Very light pseudoscalar fields, often referred to as axions, are compelling dark matter candidates and can potentially be detected through their coupling to the electromagnetic fie…

astro-ph.CO2022★ 20 cited

A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES

E. Schiappucci, F. Bianchini, M. Aguena +139

We infer the mean optical depth of a sample of optically-selected galaxy clusters from the Dark Energy Survey (DES) via the pairwise kinematic Sunyaev-Zel'dovich (kSZ) effect. The…

astro-ph.CO2022★ 37 cited

Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1

Shamik Ghosh, Yang Liu, Le Zhang +17

AliCPT is the first Chinese cosmic microwave background (CMB) experiment which will make the most precise measurements of the CMB polarization in the northern hemisphere. The key s…

astro-ph.CO2022

Forecasts on CMB lensing observations with AliCPT-1

Jinyi Liu, Zeyang Sun, Jiakang Han +18

AliCPT-1 is the first Chinese CMB experiment aiming for high precision measurement of Cosmic Microwave Background B-mode polarization. The telescope, currently under deployment in…

astro-ph.CO2022★ 6 cited

Testing synchrotron models and frequency resolution in BINGO 21 cm simulated maps using GNILC

Eduardo J. de Mericia, Larissa Santos, Carlos Alexandre Wuensche +16

To recover the 21 cm hydrogen line, it is essential to separate the cosmological signal from the much stronger foreground contributions at radio frequencies. The BINGO radio telesc…