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20012025
most citedThe Arcminute Microkelvin Imager

246 citations · 2k across the 53 of their papers we have counts for

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Showing astro-ph.IMShow all

9 papers · 1 filter

astro-ph.IM2020★ 33 cited

Characterising the Performance of High-Speed Data Converters for RFSoC-based Radio Astronomy Receivers

Chao Liu, Michael E. Jones, Angela C. Taylor

RF system-on-chip (RFSoC) devices provide the potential for implementing a complete radio astronomy receiver on a single board, but performance of the integrated analogue-to-digita…

astro-ph.IM2020★ 13 cited

MID-Radio Telescope, Single Pixel Feed Packages for the Square Kilometre Array: An Overview

Alice Pellegrini, Jonas Flygare, Isak P. Theron +10

The Square Kilometre Array (SKA) project is an international effort to build the world s largest radio telescope, enabling science with unprecedented detail and survey speed. The p…

astro-ph.IM2019★ 3 cited

Gain Stabilization for Radio Intensity Mapping using a Continuous-Wave Reference Signal

Alexander W. Pollak, Christian M. Holler, Michael E. Jones +1

Stabilizing the gain of a radio astronomy receiver is of great importance for sensitive radio intensity mapping. In this paper we discuss a stabilization method using a continuous-…

astro-ph.IM2018★ 1 cited

The C-Band All-Sky Survey (C-BASS): Digital backend for the northern survey

M. A. Stevenson, T. J. Pearson, Michael E. Jones +6

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

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,…

astro-ph.IM2014★ 3 cited

Astronomical Receiver Modelling Using Scattering Matrices

O. G. King, Michael E. Jones, C. Copley +6

Proper modelling of astronomical receivers is vital: it describes the systematic errors in the raw data, guides the receiver design process, and assists data calibration. In this p…