activity
20182022
most citedThe C-Band All-Sky Survey (C-BASS): Design and capabilities

59 citations · 139 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2022★ 18 cited

The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky

S. E. Harper, C. Dickinson, A. Barr +12

The C-Band All-Sky Survey (C-BASS) has observed the Galaxy at 4.76GHz with an angular resolution of full-width half-maximum, and detected Galactic synchrotron emission…

astro-ph.IM2021★ 3 cited

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-ph.GA2020★ 26 cited

Detection of Spectral Variations of Anomalous Microwave Emission with QUIJOTE and C-BASS

R. Cepeda-Arroita, S. Harper, C. Dickinson +32

Anomalous Microwave Emission (AME) is a significant component of Galactic diffuse emission in the frequency range -GHz and a new window into the properties of sub-nanomet…

astro-ph.CO2019★ 3 cited

The C-Band All-Sky Survey (C-BASS): Total intensity point-source detection over the northern sky

R. D. P. Grumitt, Angela C. Taylor, Luke Jew +14

We present a point-source detection algorithm that employs the second order Spherical Mexican Hat wavelet filter (SMHW2), and use it on C-BASS northern intensity data to produce a…

astro-ph.CO2019★ 6 cited

The C-Band All-Sky Survey (C-BASS): Simulated parametric fitting in single pixels in total intensity and polarization

Luke Jew, Angela C. Taylor, Michael E. Jones +14

The cosmic microwave background -mode signal is potentially weaker than the diffuse Galactic foregrounds over most of the sky at any frequency. A common method of separating the…

astro-ph.GA2018★ 17 cited

The C-Band All-Sky Survey (C-BASS): Constraining diffuse Galactic radio emission in the North Celestial Pole region

C. Dickinson, A. Barr, H. C. Chiang +17

The C-Band All-Sky Survey C-BASS is a high-sensitivity all-sky radio survey at an angular resolution of 45 arcmin and a frequency of 4.7 GHz. We present a total intensity 4.7 GHz m…

astro-ph.IM2018★ 7 cited

Probing Radio Intensity at high-Z from Marion: 2017 Instrument

L. Philip, Z. Abdurashidova, H. C. Chiang +11

We introduce Probing Radio Intensity at high-Z from Marion (PRIZM), a new experiment designed to measure the globally averaged sky brightness, including the expected redshifted 21…

astro-ph.IM2018★ 59 cited

The C-Band All-Sky Survey (C-BASS): Design and capabilities

Michael E. Jones, Angela C. Taylor, Moumita Aich +23

The C-Band All-Sky Survey (C-BASS) is an all-sky full-polarisation survey at a frequency of 5 GHz, designed to provide complementary data to the all-sky surveys of WMAP and Planck,…