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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.

Lance Miller

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Cosmology
  • Euclid
Lance.Miller@physics.ox.ac.uk
  • About
  • Publications

The gaseous environments of double radio galaxies

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 215:4 (1985) 799-814

Authors:

L Miller, MS Longair, G Fabbiano, G Trinchieri, M Elvis
More details from the publisher

The morphologies and magnetic field structures of six 3CR double radio galaxies

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 215:4 (1985) 773-797
More details from the publisher

Non-stellar radiation in radio galaxies at 3.5 µm

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 214:2 (1985) 109-118

Authors:

SJ Lilly, MS Longair, L Miller
More details from the publisher

An X-ray survey of a complete sample of 3CR radio galaxies

The Astrophysical Journal American Astronomical Society 277 (1984) 115

Authors:

G Fabbiano, G Trinchieri, M Elvis, L Miller, M Longair
More details from the publisher

2dF QSO Redshift Survey

Conference: Clustering at High Redshift

Authors:

T Shanks, BJ Boyle, SM Croom, N Loaring, L Miller, RJ Smith

Abstract:

With approximately 6000 QSO redshifts,the 2dF QSO redshift survey is already the biggest complete QSO survey. The aim for the survey is to have 25000 QSO redshifts, providing an order of magnitude increase in QSO clustering statistics. We first describe the observational parameters of the 2dF QSO survey. We then describe several highlights of the survey so far, including new estimates of the QSO luminosity function and its evolution. We also review the current status of QSO clustering analyses from the 2dF data. Finally, we discuss how the complete QSO survey will be able to constrain the value of Omega_o by measuring the evolution of QSO clustering, place limits on the cosmological constant via a direct geometrical test and determine the form of the fluctuation power-spectrum out to the approximately 1000 Mpc scales only previously probed by COBE.
Details from ArXiV
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