Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Cosmology and Gravitation Theories, Radio Astronomy Observations and Technology, and Superconducting and THz Device Technology.
SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos
SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region
Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and <i>Planck</i>. III. Combined 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
Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-<i>y</i>maps from SPT and<i>Planck</i>
CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
CMB/kSZ and Compton-y Maps from 2500 deg<sup>2</sup> of SPT-SZ and Planck Survey Data
Neutrino Properties with Ground-based Millimeter-wavelength Line Intensity Mapping
Optimal Cosmic Microwave Background Lensing Reconstruction and Parameter Estimation with SPTpol Data
A demonstration of improved constraints on primordial gravitational waves with delensing
The SPTpol Extended Cluster Survey
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 deg<sup>2</sup> SPTPOL Lensing Power Spectrum
Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects
A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg<sup>2</sup> of SPTpol Temperature and Polarization Data
Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions
Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>Telescope</mml:mi><mml:mo>+</mml:mo><mml:mi>Planck</mml:mi></mml:mrow></mml:math>
Mass Calibration of Optically Selected DES Clusters Using a Measurement of CMB-cluster Lensing with SPTpol Data
Fractional polarization of extragalactic sources in the 500 deg2 SPTpol survey
Detection of CMB-Cluster Lensing using Polarization Data from SPTpol
A measurement of CMB cluster lensing with SPT and DES year 1 data
Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg<sup>2</sup> SPT-SZ and Planck Gravitational Lensing Map
A 2500 deg<sup>2</sup> CMB Lensing Map from Combined South Pole Telescope and Planck Data
A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite
COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY
SPT-GMOS: A GEMINI/GMOS-SOUTH SPECTROSCOPIC SURVEY OF GALAXY CLUSTERS IN THE SPT-SZ SURVEY
MILLIMETER TRANSIENT POINT SOURCES IN THE SPTpol 100 SQUARE DEGREE SURVEY
GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE 2500-SQUARE-DEGREE SPT-SZ SURVEY
MASS CALIBRATION AND COSMOLOGICAL ANALYSIS OF THE SPT-SZ GALAXY CLUSTER SAMPLE USING VELOCITY DISPERSION σ<sub><i>v</i></sub>AND X-RAY<i>Y</i><sub>X</sub>MEASUREMENTS