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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.

Dr Peter Hatfield

Visitor

Research theme

  • Astronomy and astrophysics
  • Lasers and high energy density science

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
  • Hintze Centre for Astrophysical Surveys
peter.hatfield@physics.ox.ac.uk
peterhatfield.wordpress.com
  • About
  • Publications

Transforming education with the Timepix detector - Ten years of CERN@school

Radiation Measurements Elsevier BV (2019) 106090

Authors:

B Parker, L Thomas, E Rushton, P Hatfield
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IRIS opens pupils' eyes to real space research

Astronomy & Geophysics Oxford University Press (OUP) 60:1 (2019) 1.22-1.24

Authors:

Peter Hatfield, W Furnell, A Shenoy, E Fox, B Parker, L Thomas, EAC Rushton
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The LUCID-Timepix spacecraft payload and the CERN@school educational programme

JOURNAL OF INSTRUMENTATION 13 (2018)

Authors:

P Hatfield, W Furnell, A Shenoy, E Fox, R Parker, L Thomas
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Extragalactic optical and near-infrared foregrounds to 21-cm epoch of reionisation experiments

Proceedings of the International Astronomical Union Cambridge University Press 12:S333 (2018) 183-190

Authors:

Matthew J Jarvis, Rebecca AA Bowler, PW Hatfield

Abstract:

Foreground contamination is one of the most important limiting factors in detecting the neutral hydrogen in the epoch of reionisation. These foregrounds can be roughly split into galactic and extragalactic foregrounds. In these proceedings we highlight information that can be gleaned from multi-wavelength extragalactic surveys in order to overcome this issue. We discuss how clustering information from the lower-redshift, foreground galaxies, can be used as additional information in accounting for the noise associated with the foregrounds. We then go on to highlight the expected contribution of future optical and near-infrared surveys for detecting the galaxies responsible for ionising the Universe. We suggest that these galaxies can also be used to reduce the systematics in the 21-cm epoch of reionisation signal through cross-correlations if enough common area is surveyed.
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Environmental quenching and galactic conformity in the galaxy cross-correlation signal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 472:3 (2017) 3570-3588

Authors:

PW Hatfield, MJ Jarvis
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