papers

Publications (7)

astro-ph.IM2019

Packed Ultra-wideband Mapping Array (PUMA): A Radio Telescope for Cosmology and Transients

Kevin Bandura, Emanuele Castorina, Liam Connor +23

PUMA is a proposal for an ultra-wideband, low-resolution and transit interferometric radio telescope operating at . Its design is driven by six science goal…

astro-ph.IM2019

CMB-S4 Science Case, Reference Design, and Project Plan

Kevork Abazajian, Graeme Addison, Peter Adshead +222

We present the science case, reference design, and project plan for the Stage-4 ground-based cosmic microwave background experiment CMB-S4.

astro-ph.IM2019

Deprojecting beam systematics for next-generation CMB B-mode searches

Christopher Sheehy

Measurements of the cosmic microwave background polarization are vulnerable to systematic contamination from beam imperfections. Because the unpolarized CMB T is orders of magnitud…

astro-ph.CO2019

Inflation and Early Dark Energy with a Stage II Hydrogen Intensity Mapping Experiment

Cosmic Visions 21 cm Collaboration, Réza Ansari, Evan J. Arena +29

This white paper envisions a revolutionary post-DESI, post-LSST dark energy program based on intensity mapping of the redshifted 21cm emission line from neutral hydrogen at radio f…

astro-ph.IM2020

The Baryon Mapping Experiment (BMX), a 21cm intensity mapping pathfinder

Paul O'Connor, Anže Slosar, Maile Harris +10

The Baryon Mapping eXperiment (BMX) is an interferometric array designed as a pathfinder for a future post-reionization 21 cm intensity mapping survey. It consists of four 4-meter…

astro-ph.IM2019

CMB-S4 Decadal Survey APC White Paper

Kevork Abazajian, Graeme Addison, Peter Adshead +222

We provide an overview of the science case, instrument configuration and project plan for the next-generation ground-based cosmic microwave background experiment CMB-S4, for consid…

astro-ph.CO2017

No evidence for dust B-mode decorrelation in Planck data

Christopher Sheehy, Anže Slosar

Constraints on inflationary -modes using Cosmic Microwave Background polarization data commonly rely on either template cleaning or cross-spectra between maps at different frequ…