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Open AccessKinetic Inductance Traveling Wave Amplifier Designs for Practical Microwave Readout Applications
A Kinetic Inductance Traveling Wave Amplifier (KIT) utilizes the nonlinear kinetic inductance of superconducting films, particularly niobium titanium nitride (NbTiN), for parametric amplification. These amplif...
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Article
Sensitivity Modeling for LiteBIRD
LiteBIRD is a future satellite mission designed to observe the polarization of the cosmic microwave background radiation in order to probe the inflationary universe. LiteBIRD is set to observe the sky using three...
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CCAT-Prime: Characterization of the First 280 GHz MKID Array for Prime-Cam
The Prime-Cam receiver on the Fred Young Submillimeter Telescope for the CCAT-prime project aims to address important astrophysical and cosmological questions with sensitive broadband, polarimetric, and spectr...
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Article
Magnetic Field Sensitivity of Microwave SQUID Multiplexers
We present magnetic field sensitivity measurements of microwave SQUID multiplexers designed for bolometric applications. These devices are often used in environments with changing external magnetic fields, due...
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Open AccessUpdated Design of the CMB Polarization Experiment Satellite LiteBIRD
Recent developments of transition-edge sensors (TESs), based on extensive experience in ground-based experiments, have been making the sensor techniques mature enough for their application on future satellite ...
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Sensitivity of the Prime-Cam Instrument on the CCAT-Prime Telescope
CCAT-prime is a new 6 m crossed Dragone telescope designed to characterize the cosmic microwave background (CMB) polarization and foregrounds, measure the Sunyaev–Zel’dovich effects of galaxy clusters, map the...
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Development of Space-Optimized TES Bolometer Arrays for LiteBIRD
LiteBIRD is a cosmic microwave background polarization experiment with the goal of measuring the tensor-to-scalar ratio with a total uncertainty of \(\delta r <0.001\)δr<0.001. It will survey the full sky from sp...
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Characterization of the Mid-Frequency Arrays for Advanced ACTPol
The Advanced ACTPol upgrade on the Atacama Cosmology Telescope aims to improve the measurement of the cosmic microwave background anisotropies and polarization, using four new dichroic detector arrays fabricat...
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Design and Deployment of a Multichroic Polarimeter Array on the Atacama Cosmology Telescope
We present the design and the preliminary on-sky performance with respect to beams and passbands of a multichroic polarimeter array covering the 90 and 146 GHz cosmic microwave background bands and its enablin...
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Advanced ACTPol Cryogenic Detector Arrays and Readout
Advanced ACTPol is a polarization-sensitive upgrade for the 6 m aperture Atacama Cosmology Telescope, adding new frequencies and increasing sensitivity over the previous ACTPol receiver. In 2016, Advanced ACTP...
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The First Multichroic Polarimeter Array on the Atacama Cosmology Telescope: Characterization and Performance
The Atacama Cosmology Telescope Polarimeter (ACTPol) is a polarization sensitive receiver for the 6-m Atacama Cosmology Telescope (ACT) and measures the small angular scale polarization anisotropies in the cos...
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Advanced ACTPol Multichroic Polarimeter Array Fabrication Process for 150 mm Wafers
Advanced ACTPol (AdvACT) is a third-generation cosmic microwave background receiver to be deployed in 2016 on the Atacama Cosmology Telescope (ACT). Spanning five frequency bands from 25 to 280 GHz and having ...
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High-Density Superconducting Cables for Advanced ACTPol
Advanced ACTPol (AdvACT) is an upcoming Atacama Cosmology Telescope (ACT) receiver upgrade, scheduled to deploy in 2016, that will allow measurement of the cosmic microwave background polarization and temperat...
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Horn Coupled Multichroic Polarimeters for the Atacama Cosmology Telescope Polarization Experiment
Multichroic polarization sensitive detectors enable increased sensitivity and spectral coverage for observations of the cosmic microwave background. An array optimized for dual frequency detectors can provide ...
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Open AccessPW02-018 - Impact of PSTPIP1 mutaions on clinical phenotype
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Optical and Thermal Properties of ANL/KICP Polarization Sensitive Bolometers for SPTpol
We present recent optical and thermal characterizations of polarization sensitive mm-wave bolometers fabricated at Argonne National Lab. The devices are designed to measure the polarization of the Cosmic Micro...
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An Overview of the SPTpol Experiment
In 2012 the South Pole Telescope (SPT) will begin a 625 deg2 survey to measure the polarization anisotropy of the cosmic microwave background (CMB). Observations of the CMB B-mode angular power spectrum will be u...
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Open AccessA novel mutatioin in the PSTPIP1 gene is associated with an autoinflammatory disease distinct from classical PAPA syndrome