papers

Publications (14)

astro-ph.CO2014

Neutrino Physics from the Cosmic Microwave Background and Large Scale Structure

K. N. Abazajian, K. Arnold, J. Austermann +74

This is a report on the status and prospects of the quantification of neutrino properties through the cosmological neutrino background for the Cosmic Frontier of the Division of Pa…

astro-ph.IM2013

Large-aperture wide-bandwidth antireflection-coated silicon lenses for millimeter wavelengths

R. Datta, C. D. Munson, M. D. Niemack +17

The increasing scale of cryogenic detector arrays for sub-millimeter and millimeter wavelength astrophysics has led to the need for large aperture, high index of refraction, low lo…

astro-ph2006

A Shell of Thermal X-ray Emission Associated with the Young Crab-like Remnant 3C58

E. V. Gotthelf, D. J. Helfand, L. Newburgh

Deep X-ray imaging spectroscopy of the bright pulsar wind nebula 3C58 confirms the existence of an embedded thermal X-ray shell surrounding the pulsar PSR J0205+6449. Radially reso…

physics.acc-ph2003

A Frictional Cooling Demonstration Experiment with Protons

R. Galea, A. Caldwell, L. Newburgh

Muon cooling is the main technological obstacle in the building of a muon collider. A muon cooling scheme based on Frictional Cooling holds promise in overcoming this obstacle. An…

astro-ph.CO2025

The Simons Observatory: forecasted constraints on primordial gravitational waves with the expanded array of Small Aperture Telescopes

The Simons Observatory Collaboration, I. Abril-Cabezas, S. Adachi +479

We present updated forecasts for the scientific performance of the degree-scale (0.5 deg FWHM at 93 GHz), deep-field survey to be conducted by the Simons Observatory (SO). By 2027,…

astro-ph.IM2016

The Atacama Cosmology Telescope: The polarization-sensitive ACTPol instrument

R. J. Thornton, P. A. R. Ade, S. Aiola +53

The Atacama Cosmology Telescope (ACT) is designed to make high angular resolution measurements of anisotropies in the Cosmic Microwave Background (CMB) at millimeter wavelengths. W…

astro-ph.IM2021

The CHIME Pulsar Project: System Overview

Pulsar Collaboration, M. Amiri, K. M. Bandura +42

We present the design, implementation and performance of a digital backend constructed for the Canadian Hydrogen Intensity Mapping Experiment (CHIME) that uses accelerated computin…

astro-ph.CO2017

Detection of the pairwise kinematic Sunyaev-Zel'dovich effect with BOSS DR11 and the Atacama Cosmology Telescope

F. De Bernardis, S. Aiola, E. M. Vavagiakis +55

We present a new measurement of the kinematic Sunyaev-Zeldovich effect using data from the Atacama Cosmology Telescope (ACT) and the Baryon Oscillation Spectroscopic Survey (BOSS).…

astro-ph.IM2016

Survey strategy optimization for the Atacama Cosmology Telescope

F. De Bernardis, J. R. Stevens, M. Hasselfield +34

In recent years there have been significant improvements in the sensitivity and the angular resolution of the instruments dedicated to the observation of the Cosmic Microwave Backg…

astro-ph.CO2019

Measurement of the Splashback Feature around SZ-selected Galaxy Clusters with DES, SPT and ACT

T. Shin, S. Adhikari, E. J. Baxter +107

We present a detection of the splashback feature around galaxy clusters selected using their Sunyaev-Zel'dovich (SZ) signal. Recent measurements of the splashback feature around op…

astro-ph.IM2015

Advanced ACTPol Cryogenic Detector Arrays and Readout

S. W. Henderson, R. Allison, J. Austermann +54

Advanced ACTPol is a polarization-sensitive upgrade for the 6 m aperture Atacama Cosmology Telescope (ACT), adding new frequencies and increasing sensitivity over the previous ACTP…

astro-ph.CO2023

Cosmology from Cross-Correlation of ACT-DR4 CMB Lensing and DES-Y3 Cosmic Shear

S. Shaikh, I. Harrison, A. van Engelen +105

Cross-correlation between weak lensing of the Cosmic Microwave Background (CMB) and weak lensing of galaxies offers a way to place robust constraints on cosmological and astrophysi…

astro-ph.CO2014

Inflation Physics from the Cosmic Microwave Background and Large Scale Structure

K. N. Abazajian, K. Arnold, J. Austermann +91

Fluctuations in the intensity and polarization of the cosmic microwave background (CMB) and the large-scale distribution of matter in the universe each contain clues about the natu…

astro-ph.IM2025

The Simons Observatory: Science Goals and Forecasts for the Enhanced Large Aperture Telescope

The Simons Observatory Collaboration, M. Abitbol, I. Abril-Cabezas +419

We describe updated scientific goals for the wide-field, millimeter-wave survey that will be produced by the Simons Observatory (SO). Significant upgrades to the 6-meter SO Large A…