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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.

Professor Roger Davies

Emeritus Wetton Professor

Research theme

  • Astronomy and astrophysics
  • Instrumentation

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Cosmology
  • Galaxy formation and evolution
  • Hintze Centre for Astrophysical Surveys
  • Rubin-LSST
  • Extremely Large Telescope
Roger.Davies@physics.ox.ac.uk
  • About
  • Publications

SPECTROSCOPY AND PHOTOMETRY OF ELLIPTIC GALAXIES .2. THE SPECTROSCOPIC PARAMETERS

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 64:4 (1987) 581-600

Authors:

RL DAVIES, D BURSTEIN, A DRESSLER, SM FABER, D LYNDENBELL, RJ TERLEVICH, G WEGNER
More details from the publisher

THE STELLAR KINEMATICS OF ELLIPTIC GALAXIES

IAU SYMPOSIA (1987) 63-77
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IMPLEMENTATION OF A SYSTEM FOR MONITORING IMAGE SIZE AND MOTION.

627:pt 2 (1986) 813-828

Authors:

WG Robinson, VD Russell, RL Davies

Abstract:

A system to measure image size and motion has been designed, constructed and put into operation at the 4-meter Mayall telescope at Kitt Peak National Observatory (KPNO). The present system configuration consists of three elements. A 128 multiplied by 128 pixel CID camera is mounted at the south port of the Cassegrain instrument rotator. The CID camera is fed, under software control, by a movable mirror in the instrument rotator. Focusing is achieved by determining the point of zero-image motion when the f/8 beam is cut by a rotating Newall mask. Focal plane images are digitized and stored on digital disk for later determination of image size and motion as a function of time. The second element is a two-dimensional position sensor which records image motion induced along an air path located between the primary and secondary mirrors of the telescope. The third element monitors temperature of the telescope and air throughout the telescope structure. The system is described and preliminary results are presented.

NGC-4261 - A PROLATE ELLIPTIC GALAXY

ASTROPHYSICAL JOURNAL 303:2 (1986) L45-&

Authors:

RL DAVIES, M BIRKINSHAW
More details from the publisher

THE DYNAMICS OF THE ACTIVE GALAXY NGC-1052

ASTROPHYSICAL JOURNAL 302:1 (1986) 234-&

Authors:

RL DAVIES, GD ILLINGWORTH
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