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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Angela Taylor

Professor of Experimental Astrophysics

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology
  • Instrumentation

Sub department

  • Astrophysics

Research groups

  • Experimental radio cosmology
  • C-BASS
  • The Square Kilometre Array (SKA)
Angela.Taylor@physics.ox.ac.uk
Telephone: 01865 (2)73297
Denys Wilkinson Building, room 753
  • About
  • Publications

The cosmic microwave background power spectrum out to ℓ= 1400 measured by the Very Small Array

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 341:4 (2003) l23-l28

Authors:

Keith Grainge, Pedro Carreira, Kieran Cleary, Rod D Davies, Richard J Davis, Clive Dickinson, Ricardo Genova-Santos, Carlos M Gutiérrez, Yaser A Hafez, Michael P Hobson, Michael E Jones, Rüdiger Kneissl, Katy Lancaster, Anthony Lasenby, JP Leahy, Klaus Maisinger, Guy G Pooley, Rafael Rebolo, José Alberto Rubiño-Martin, Pedro J Sosa Molina, Carolina Ödman, Ben Rusholme, Richard DE Saunders, Richard Savage, Paul F Scott, Anže Slosar, Angela C Taylor, David Titterington, Elizabeth Waldram, Robert A Watson, Althea Wilkinson
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The Very Small Array

AIP Conference Proceedings AIP Publishing 616:1 (2002) 72-78
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The very small array

EXPERIMENTAL COSMOLOGY AT MILLIMETRE WAVELENGTHS 616 (2002) 72-78
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The radio source counts at 15 GHz and their implications for cm-wave CMB imaging

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 327:1 (2001) l1-l4

Authors:

Angela C Taylor, Keith Grainge, Michael E Jones, GG Pooley, Richard DE Saunders, EM Waldram
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Characterising the Performance of High-Speed Data Converters for RFSoC-based Radio Astronomy Receivers

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP)

Authors:

Chao Liu, Michael E Jones, Angela C Taylor

Abstract:

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-digital converters is critical. We have evaluated the performance of the data converters in the Xilinx ZU28DR RFSoC, which are 12-bit, 8-fold interleaved converters with a maximum sample speed of 4.096 Giga-sample per second (GSPS). We measured the spurious-free dynamic range (SFDR), signal-to-noise and distortion (SINAD), effective number of bits (ENOB), intermodulation distortion (IMD) and cross-talk between adjacent channels over the bandwidth of 2.048 GHz. We both captured data for off-line analysis with floating-point arithmetic, and implemented a real-time integer arithmetic spectrometer on the RFSoC. The performance of the ADCs is sufficient for radio astronomy applications and close to the vendor specifications in most of the scenarios. We have carried out spectral integrations of up to 100 s and stability tests over tens of hours and find thermal noise-limited performance over these timescales.
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