Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
Menu
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

OASIS high-resolution integral field spectroscopy of the SAURON ellipticals and lenticulars

ASTRON NACHR 325:2 (2004) 100-103

Authors:

R McDermid, E Emsellem, M Cappellari, H Kuntschner, R Bacon, M Bureau, Y Copin, RL Davies, J Falcon-Barroso, P Ferruit, D Krajnovic, RF Peletier, K Shapiro, F Wernli, PT de Zeeuw

Abstract:

We present a summary of high-spatial resolution follow-up observations of the elliptical (E) and lenticular (SO) galaxies in the SAURON survey using the OASIS integral field spectrograph. The OASIS observations explore the central 8" x 10" regions of these galaxies using a spatial sampling four times higher than SAURON, often revealing previously undiscovered features. Around 75% (31/48) of the SAURON E/SOs with central velocity dispersion greater than or similar to 120 kin s(-1) were observed with OASIS, covering well the original SAURON representative sample. We present here an overview of this follow-up survey, and some preliminary results on individual objects, including a previously unreported counter-rotating core in NGC4382; the decoupled stellar and gas velocity fields of NGC 2768; and the strong age gradient towards the centre of NGC 3489.
More details from the publisher
More details

The Gemini-North multi-object spectrograph: Performance in imaging, long-slit, and multi-object spectroscopic modes

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 116:819 (2004) 425-440

Authors:

IM Hook, I Jorgensen, JR Allington-Smith, RL Davies, N Metcalfe, RG Murowinski, D Crampton
More details from the publisher

A Million Element Integral Field Unit (MEIFU)

Scientific Drivers for ESO Future VLT/VLTI Instrumentation Springer (2003)

Authors:

S Morris, R Content, R Sharples, R Bower, Roger Davies, C Baugh

Abstract:

We describe an instrument concept that will provide simultaneous spectra for a million spatial samples on the sky. With the proposed field of view and spectral resolution, it will be able to measure redshifts and line strengths for around 2-4000 z~3-7 galaxies in a 16 night campaign. The main science driver is to obtain a complete census of the star formation properties of galaxies with 2.5
More details from the publisher
Details from ORA
Details from ArXiV

Recent Results from the NOAO Fundamental Plane Survey

AIP Conference Proceedings AIP Publishing 666:1 (2003) 315-318

Authors:

JE Nelan, GA Wegner, RJ Smith, MJ Hudson, JJ Malecki, JR Lucey, SAW Moore, SJ Quinney, D Schade, NB Suntzeff, RL Davies
More details from the publisher

The Stellar Content of the Bulge of M31**Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA under contract NAS 5-26555.

The Astronomical Journal American Astronomical Society 125:5 (2003) 2473-2493

Authors:

Andrew W Stephens, Jay A Frogel, DL DePoy, Wendy Freedman, Carme Gallart, Pascale Jablonka, Alvio Renzini, R Michael Rich, Roger Davies
More details from the publisher

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 49
  • Page 50
  • Page 51
  • Page 52
  • Current page 53
  • Page 54
  • Page 55
  • Page 56
  • Page 57
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics
  • Current students
  • Staff intranet