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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

Unravelling the origin of the counter-rotating core in IC 1459 with KMOS and MUSE

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 488:2 (2019) 1679-1694

Authors:

Laura J Prichard, Sam P Vaughan, Roger L Davies
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Galaxy formation and evolution science in the era of the Large Synoptic Survey Telescope

Nature Reviews Physics Springer Nature 1:7 (2019) 450-462

Authors:

Brant E Robertson, Manda Banerji, Sarah Brough, Roger L Davies, Henry C Ferguson, Ryan Hausen, Sugata Kaviraj, Jeffrey A Newman, Samuel J Schmidt, J Anthony Tyson, Risa H Wechsler
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The fifteenth data release of the Sloan Digital Sky Surveys: First release of MaNGA-derived quantities, data visualization tools, and Stellar Library

Astrophysical Journal Supplement Institute of Physics 240:23 (2019)

Authors:

DS Aguado, R Ahumada, A Almeida, Michele Cappellari, R Davies, Chris Lintott

Abstract:

Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years of operation (2014 July–2017 July). This is the third data release for SDSS-IV, and the 15th from SDSS (Data Release Fifteen; DR15). New data come from MaNGA—we release 4824 data cubes, as well as the first stellar spectra in the MaNGA Stellar Library (MaStar), the first set of survey-supported analysis products (e.g., stellar and gas kinematics, emission-line and other maps) from the MaNGA Data Analysis Pipeline, and a new data visualization and access tool we call "Marvin." The next data release, DR16, will include new data from both APOGEE-2 and eBOSS; those surveys release no new data here, but we document updates and corrections to their data processing pipelines. The release is cumulative; it also includes the most recent reductions and calibrations of all data taken by SDSS since first light. In this paper, we describe the location and format of the data and tools and cite technical references describing how it was obtained and processed. The SDSS website (www.sdss.org) has also been updated, providing links to data downloads, tutorials, and examples of data use. Although SDSS-IV will continue to collect astronomical data until 2020, and will be followed by SDSS-V (2020–2025), we end this paper by describing plans to ensure the sustainability of the SDSS data archive for many years beyond the collection of data.
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The stellar population and initial mass function of NGC 1399 with MUSE

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 479:2 (2018) 2443-2456

Authors:

Sam P Vaughan, Roger L Davies, Simon Zieleniewski, Ryan CW Houghton
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Radial measurements of IMF-sensitive absorption features in two massive ETGs

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 475:1 (2018) 1073-1092

Authors:

SP Vaughan, RL Davies, S Zieleniewski, RCW Houghton
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