W. L. K. Wu

SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G main field

SPT-3G D1: Constraints on inflationary gravitational waves with two years of SPT-3G data

Measurement of the CMB temperature power spectrum and constraints on cosmology from the SPT-3G 2018 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:mi>T</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:mrow></mml:math>, <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mi>E</mml:mi></mml:mrow></mml:math>, and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mm

Measurement of gravitational lensing of the cosmic microwave background using SPT-3G 2018 data

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mi>l</mml:mi><mml:mi>a</mml:mi><mml:mi>n</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:math>. II. Cross-correlation measurements and cosmological constraints

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and<i>Planck</i>. I. Construction of CMB lensing maps and modeling choices

BICEP/Keck. XVI. Characterizing Dust Polarization through Correlations with Neutral Hydrogen

Bicep/Keck XV: The Bicep3 Cosmic Microwave Background Polarimeter and the First Three-year Data Set

BICEP/<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>K</mml:mi><mml:mi>e</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:math> XIV: Improved constraints on axionlike polarization oscillations in the cosmic microwave background

Searching for axionlike time-dependent cosmic birefringence with data from SPT-3G

Optimal Cosmic Microwave Background Lensing Reconstruction and Parameter Estimation with SPTpol Data

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>BICEP</mml:mi><mml:mo>/</mml:mo><mml:mi>K</mml:mi><mml:mi>e</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi><mml:mtext> </mml:mtext></mml:mrow></mml:math> XII: Constraints on axionlike polarization oscillations in the cosmic microwave background

Measurements of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>B</mml:mi></mml:math>-mode polarization of the cosmic microwave background from 500 square degrees of SPTpol data

Constraints on Cosmological Parameters from the 500 deg² SPTPOL Lensing Power Spectrum

Galaxy Clusters Selected via the Sunyaev–Zel’dovich Effect in the SPTpol 100-square-degree Survey

Searching for anisotropic cosmic birefringence with polarization data from SPTpol

Hubble constant difference between CMB lensing and BAO measurements

A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg² of SPTpol Temperature and Polarization Data

Dark Energy Survey Year 1 results: Methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions

Fractional polarization of extragalactic sources in the 500 deg2 SPTpol survey

BICEP2/Keck Array XI: Beam Characterization and Temperature-to-Polarization Leakage in the BK15 Data Set

Constraints on Primordial Gravitational Waves Using <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mi>l</mml:mi><mml:mi>a</mml:mi><mml:mi>n</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:math>, WMAP, and New BICEP2/<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>K</mml:mi><mml:mi>e</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:math> Observations through the 2015 Se

Dark Energy Survey Year 1 Results: A Precise H0 Estimate from DES Y1, BAO, and D/H Data

Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg² SPT-SZ and Planck Gravitational Lensing Map

CMB Polarization B-mode Delensing with SPTpol and Herschel

BICEP2 / <i>Keck Array</i> IX: New bounds on anisotropies of CMB polarization rotation and implications for axionlike particles and primordial magnetic fields

Improved Constraints on Cosmology and Foregrounds from BICEP2 and Keck Array Cosmic Microwave Background Data with Inclusion of 95 GHz Band

Optimization of Transition Edge Sensor Arrays for Cosmic Microwave Background Observations With the South Pole Telescope

BICEP3 performance overview and planned Keck Array upgrade

Neutrino physics from the cosmic microwave background and large scale structure

SBIR Phase I: High-Rate Production of Nano-Architectured Hybrid Oxide Materials for Lithium Battery Cathodes

SBIR Phase I: A Throughput Enhancer

A New Sequence Method for Low Cost Multiple Access Communications

New Coding Methods for Lower Cost Satellite Communication