papers

Publications (35)

astro-ph.CO2026

The Tianlai-WIYN North Celestial Cap Redshift Survey

Reza Ansari, Gabriela A. Marques, John P. Marriner +13

We present the results of a small, low redshift spectroscopic survey of galaxies within 3 degrees of the North Celestial Pole (NCP) selected using V-band photometry obtained from t…

astro-ph.IM2020

Reflections and Standing Waves on the Tianlai Cylinder Array

Jixia Li, Fengquan Wu, Shijie Sun +8

In 21~cm intensity mapping, the spectral smoothness of the foreground is exploited to separate it from the much weaker 21~cm signal. However, the non-smooth frequency response of t…

astro-ph.CO2009

Observing the Evolution of the Universe

James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…

astro-ph.IM2022

The Hydrogen Intensity and Real-time Analysis eXperiment: 256-Element Array Status and Overview

Devin Crichton, Moumita Aich, Adam Amara +97

The Hydrogen Intensity and Real-time Analysis eXperiment (HIRAX) is a radio interferometer array currently in development, with an initial 256-element array to be deployed at the S…

astro-ph1997

Large Angular Scale Polarization of the Cosmic Microwave Background and the Feasibility of its Detection

Brian Keating, Peter Timbie, Alexander Polnarev +1

In addition to its spectrum and temperature anisotropy, the 2.7K Cosmic Microwave Background is also expected to exhibit a low level of polarization. The spatial power spectrum of…

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.IM2024

The FRB-searching pipeline of the Tianlai Cylinder Pathfinder Array

Zijie Yu, Furen Deng, Shijie Sun +14

This paper presents the design, calibration, and survey strategy of the Fast Radio Burst (FRB) digital backend and its real-time data processing pipeline employed in the Tianlai Cy…

astro-ph.CO2022

Snowmass 2021 CMB-S4 White Paper

Kevork Abazajian, Arwa Abdulghafour, Graeme E. Addison +353

This Snowmass 2021 White Paper describes the Cosmic Microwave Background Stage 4 project CMB-S4, which is designed to cross critical thresholds in our understanding of the origin a…

astro-ph.CO2013

Maximum likelihood analysis of systematic errors in interferometric observations of the cosmic microwave background

Le Zhang, Ata Karakci, Paul M. Sutter +5

We investigate the impact of instrumental systematic errors in interferometric measurements of the cosmic microwave background (CMB) temperature and polarization power spectra. We…

astro-ph.IM2020

The Tianlai Cylinder Pathfinder Array: System Functions and Basic Performance Analysis

Jixia Li, Shifan Zuo, Fengquan Wu +35

The Tianlai Cylinder Pathfinder is a radio interferometer array designed to test techniques for 21 cm intensity mapping in the post-reionization Universe, with the ultimate aim of…

astro-ph.CO2019

Messengers from the Early Universe: Cosmic Neutrinos and Other Light Relics

Daniel Green, Mustafa A. Amin, Joel Meyers +136

The hot dense environment of the early universe is known to have produced large numbers of baryons, photons, and neutrinos. These extreme conditions may have also produced other lo…

astro-ph2003

The Large-Scale Polarization of the Microwave Foreground

Angelica de Oliveira-Costa, Max Tegmark, Christopher O'Dell +4

Most of the useful information about inflationary gravitational waves and reionization is on large angular scales where Galactic foreground contamination is the worst, so a key cha…

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.IM2026

21 cm Power Spectrum Analysis of North Celestial Pole Observations with the Tianlai Dish Pathfinder Array

Guangzhi He, Shifan Zuo, Jixia Li +11

The Tianlai Dish Pathfinder Array (TDPA) is a radio interferometer designed to test techniques for 21 cm intensity mapping in the post-reionization universe as a means of measuring…

astro-ph.CO2019

Primordial Non-Gaussianity

P. Daniel Meerburg, Daniel Green, Muntazir Abidi +175

Our current understanding of the Universe is established through the pristine measurements of structure in the cosmic microwave background (CMB) and the distribution and shapes of…

astro-ph.IM2019

QUBIC: Exploring the primordial Universe with the Q\&U Bolometric Interferometer

Aniello Mennella, Peter Ade, Giorgio Amico +127

In this paper we describe QUBIC, an experiment that will observe the polarized microwave sky with a novel approach, which combines the sensitivity of state-of-the art bolometric de…

astro-ph2004

The large-scale polarization of the microwave background and foreground

Angelica de Oliveira-Costa, Max Tegmark, Chris O'Dell +4

The DASI discovery of CMB polarization has opened a new chapter in cosmology. Most of the useful information about inflationary gravitational waves and reionization is on large ang…

astro-ph.CO2013

Systematic Effects in Interferometric Observations of the CMB Polarization

Ata Karakci, Le Zhang, P. M. Sutter +5

The detection of the primordial -mode spectrum of the polarized cosmic microwave background (CMB) signal may provide a probe of inflation. However, observation of such a faint s…

astro-ph2003

COMPASS: An Instrument for Measuring the Polarization of the CMB on Intermediate Angular Scales

Philip C. Farese, Giorgio Dall'Oglio, Josh Gundersen +9

COMPASS is an on-axis 2.6 meter telescope coupled to a correlation polarimeter. The entire instrument was built specifically for CMB polarization studies. Careful attention was giv…

astro-ph.CO2020

CMB-S4: Forecasting Constraints on Primordial Gravitational Waves

S4 Collaboration, Kevork Abazajian, Graeme E. Addison +233

CMB-S4---the next-generation ground-based cosmic microwave background (CMB) experiment---is set to significantly advance the sensitivity of CMB measurements and enhance our underst…

astro-ph2006

Task Force on Cosmic Microwave Background Research

James Bock, Sarah Church, Mark Devlin +11

One of the most spectacular scientific breakthroughs in past decades was using measurements of the fluctuations in the cosmic microwave background (CMB) to test precisely our under…

astro-ph.IM2021

Overview and status of EXCLAIM, the experiment for cryogenic large-aperture intensity mapping

Giuseppe Cataldo, Peter Ade, Christopher Anderson +41

The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) is a balloon-borne far-infrared telescope that will survey star formation history over cosmological time sca…

astro-ph.CO2023

Needlet Karhunen-Loève (NKL): A Method For Cleaning Foregrounds From 21cm Intensity Maps

John Podczerwinski, Peter Timbie

This paper introduces a technique called NKL, which cleans both polarized and unpolarized foregrounds from HI intensity maps by applying a Karhunen-Loève transform on the needlet…

astro-ph.GA2024

Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations

Calvin Osinga, Benedikt Diemer, Francisco Villaescusa-Navarro +2

Intensity mapping experiments are beginning to measure the spatial distribution of neutral atomic hydrogen (HI) to constrain cosmological parameters and the large-scale distributio…

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.CO2013

Bayesian Inference of Polarized CMB Power Spectra from Interferometric Data

Ata Karakci, P. M. Sutter, Le Zhang +5

Detection of B-mode polarization of the cosmic microwave background (CMB) radiation is one of the frontiers of observational cosmology. Because they are an order of magnitude faint…

astro-ph.IM2025

Measurement of the Primary Beam of the Tianlai Cylindrical Antenna Using an Unmanned Aerial Vehicle

Jixia Li, Nanben Suo, Shenzhe Xu +9

The Tianlai Cylinder Pathfinder Array consists of three adjacent cylindrical reflectors fixed on the ground, each 40 meters long and 15 meters wide, with the cylinder axis oriented…

astro-ph.IM2024

Optical Design of the EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM)

Thomas Essinger-Hileman, Danny Chmaytelli, Trevor Oxholm +23

This work describes the design and implementation of optics for EXCLAIM, the EXperiment for Cryogenic Large-Aperture Intensity Mapping. EXCLAIM is a balloon-borne telescope that wi…

astro-ph.IM2021

AlgoSCR: An algorithm for Solar Contamination Removal from radio interferometric data

Anh Phan, Santanu Das, Albert Stebbins +10

Hydrogen intensity mapping is a new field in astronomy that promises to make three-dimensional maps of the matter distribution of the Universe using the redshifted $21\,\textrm{cm}…

astro-ph.IM2019

Research and Development for HI Intensity Mapping

Zeeshan Ahmed, David Alonso, Mustafa A. Amin +51

Development of the hardware, data analysis, and simulation techniques for large compact radio arrays dedicated to mapping the 21 cm line of neutral hydrogen gas has proven to be mo…

astro-ph.IM2023

The Effects of the Local Environment on a Compact Radio Interferometer I: Cross-coupling in the Tianlai Dish Pathfinder Array

Juhun Kwak, John Podczerwinski, Peter Timbie +10

The visibilities measured by radio astronomical interferometers include non-astronomical correlated signals that arise from the local environment of the array. These correlated sig…

astro-ph.IM2022

The Electromagnetic Characteristics of the Tianlai Cylindrical Pathfinder Array

Shijie Sun, Jixia Li, Fengquan Wu +8

A great challenge for 21 cm intensity mapping experiments is the strong foreground radiation which is orders of magnitude brighter than the 21cm signal. Removal of the foreground t…

astro-ph.CO2023

FAST drift scan survey for HI intensity mapping: I. preliminary data analysis

Yichao Li, Yougang Wang, Furen Deng +15

This work presents the initial results of the drift-scan observation for the neutral hydrogen (HI) intensity mapping survey with the Five-hundred-meter Aperture Spherical radio Tel…

astro-ph.IM2017

CMB-S4 Technology Book, First Edition

Maximilian H. Abitbol, Zeeshan Ahmed, Darcy Barron +58

CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible from the…

astro-ph.IM2013

Probabilistic image reconstruction for radio interferometers

P. M. Sutter, Benjamin D. Wandelt, Jason D. McEwen +6

We present a novel, general-purpose method for deconvolving and denoising images from gridded radio interferometric visibilities using Bayesian inference based on a Gaussian proces…