Calvin Tsai
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View article: Laminate polyethylene window development for large aperture millimeter receivers
Laminate polyethylene window development for large aperture millimeter receivers Open
New experiments that target the B-mode polarization signals in the Cosmic Microwave Background require more sensitivity, more detectors, and thus larger-aperture millimeter-wavelength telescopes, than previous experiments. These larger ape…
View article: Improved Polarization Calibration of the BICEP3 CMB Polarimeter at the South Pole
Improved Polarization Calibration of the BICEP3 CMB Polarimeter at the South Pole Open
The BICEP3 Polarimeter is a small aperture, refracting telescope, dedicated to the observation of the Cosmic Microwave Background (CMB) at 95GHz. It is designed to target degree angular scale polarization patterns, in particular the very-m…
View article: Improved polarization calibration of the BICEP3 CMB polarimeter at the South Pole
Improved polarization calibration of the BICEP3 CMB polarimeter at the South Pole Open
The BICEP3 Polarimeter is a small aperture, refracting telescope, dedicated to the observation of the Cosmic Microwave Background (CMB) at 95GHz. It is designed to target degree angular scale polarization patterns, in particular the very-m…
View article: Thermal testing for cryogenic CMB instrument optical design
Thermal testing for cryogenic CMB instrument optical design Open
Observations of the Cosmic Microwave Background rely on cryogenic instrumentation with cold detectors, readout, and optics providing the low noise performance and instrumental stability required to make more sensitive measurements. It is t…
View article: 2022 upgrade and improved low frequency camera sensitivity for CMB observation at the South Pole
2022 upgrade and improved low frequency camera sensitivity for CMB observation at the South Pole Open
Constraining the Galactic foregrounds with multi-frequency Cosmic Microwave Background (CMB) observations is an essential step towards ultimately reaching the sensitivity to measure primordial gravitational waves (PGWs), the sign of inflat…
View article: A Measurement of the CMB E-mode Angular Power Spectrum at Subdegree Scales from 670 Square Degrees of POLARBEAR Data
A Measurement of the CMB E-mode Angular Power Spectrum at Subdegree Scales from 670 Square Degrees of POLARBEAR Data Open
We report a measurement of the E -mode polarization power spectrum of the cosmic microwave background (CMB) using 150 GHz data taken from 2014 July to 2016 December with the P olarbear experiment. We reach an effective polarization map noi…
View article: A Measurement of the Degree-scale CMB B-mode Angular Power Spectrum with Polarbear
A Measurement of the Degree-scale CMB B-mode Angular Power Spectrum with Polarbear Open
We present a measurement of the B -mode polarization power spectrum of the cosmic microwave background (CMB) using data taken from 2014 July to 2016 December with the Polarbear experiment. The CMB power spectra are measured using observati…
View article: Deployment of Polarbear-2A
Deployment of Polarbear-2A Open
View article: Cross-correlation of CMB polarization lensing with High-z submillimeter Herschel-ATLAS galaxies
Cross-correlation of CMB polarization lensing with High-z submillimeter Herschel-ATLAS galaxies Open
We report a 4.8σ measurement of the cross-correlation signal between the cosmic microwave background (CMB) lensing convergence reconstructed from measurements of the CMB polarization made by the Polarbear experiment and the infrared-select…
View article: Evidence for the cross-correlation between cosmic icrowave background polarization lensing from Polarbear and cosmic shear from Subaru Hyper Suprime-Cam
Evidence for the cross-correlation between cosmic icrowave background polarization lensing from Polarbear and cosmic shear from Subaru Hyper Suprime-Cam Open
We present the first measurement of cross-correlation between the lensing potential, reconstructed from cosmic microwave background (CMB) polarization data, and the cosmic shear field from galaxy shapes. This measurement is made using data…
View article: Measurements of Tropospheric Ice Clouds with a Ground-based CMB Polarization Experiment, POLARBEAR
Measurements of Tropospheric Ice Clouds with a Ground-based CMB Polarization Experiment, POLARBEAR Open
The polarization of the atmosphere has been a long-standing concern for ground-based experiments targeting cosmic microwave background (CMB) polarization. Ice crystals in upper tropospheric clouds scatter thermal radiation from the ground …
View article: The POLARBEAR-2 and Simons Array Focal Plane Fabrication Status
The POLARBEAR-2 and Simons Array Focal Plane Fabrication Status Open
View article: Design and characterization of the POLARBEAR-2b and POLARBEAR-2c cosmic microwave background cryogenic receivers
Design and characterization of the POLARBEAR-2b and POLARBEAR-2c cosmic microwave background cryogenic receivers Open
The POLARBEAR-2/Simons Array Cosmic Microwave Background (CMB) polarization experiment is an upgrade and expansion of the existing POLARBEAR-1 (PB-1) experiment, located in the Atacama desert in Chile. Along with the CMB temperature and $E…
View article: Design and characterization of the POLARBEAR-2b and POLARBEAR-2c cosmic\n microwave background cryogenic receivers
Design and characterization of the POLARBEAR-2b and POLARBEAR-2c cosmic\n microwave background cryogenic receivers Open
The POLARBEAR-2/Simons Array Cosmic Microwave Background (CMB) polarization\nexperiment is an upgrade and expansion of the existing POLARBEAR-1 (PB-1)\nexperiment, located in the Atacama desert in Chile. Along with the CMB\ntemperature and…