Area of research
Astronomy and Astrophysics · Nuclear and High Energy Physics
Research interest
Research interests include Radio Astronomy Observations and Technology, Superconducting and THz Device Technology, Cosmology and Gravitation Theories, and Dark Matter and Cosmic Phenomena.
BICEP/<i>Keck</i> XVIII: Measurement of BICEP3 polarization angles and consequences for constraining cosmic birefringence and inflation
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
Neutrino Properties with Ground-based Millimeter-wavelength Line Intensity Mapping
SPT-SLIM: A Line Intensity Mapping Pathfinder for the South Pole Telescope
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
A demonstration of improved constraints on primordial gravitational waves with delensing
<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
Microwave spectro-polarimetry of matter and radiation across space and time
Receiver development for BICEP Array, a next-generation CMB polarimeter at the South Pole
Full-Array Noise Performance of Deployment-Grade SuperSpec mm-Wave On-Chip Spectrometers
Microwave Spectro-Polarimetry of Matter and Radiation across Space and\n Time
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
Constraining the expansion history and early dark energy with line intensity mapping
The design and characterization of a 300 channel, optimized full-band millimeter filterbank for science with SuperSpec
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
BICEP3 performance overview and planned Keck Array upgrade
Detection of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>B</mml:mi></mml:math>-Mode Polarization at Degree Angular Scales by BICEP2
BICEP2. II. EXPERIMENT AND THREE-YEAR DATA SET
BICEP3: a 95GHz refracting telescope for degree-scale CMB polarization