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Roger Davies (astrophysicist)

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Roger Davies
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Roger Davies presenting at the National Astronomy Meeting 2012
7th President of the European Astronomical Society
Incumbent
Assumed office
30 June 2017
Thesis The Dynamics of Elliptical Galaxies  (1978)
Doctoral advisor C.D. Mackay
Doctoral students

Roger Llewelyn Davies (born 13 January 1954) is a British astronomer and cosmologist, one of the so-called Seven Samurai collaboration who discovered an apparent concentration of mass in the Universe called the Great Attractor. [1] He is the emeritus Philip Wetton Professor of Astrophysics in the Department of Physics, Oxford University [2] and Student of Christ Church. His research interests centre on cosmology and how galaxies form and evolve. He has a longstanding interest in astronomical instruments and telescopes and promoted the scientific case for the UK's involvement in the 8m Gemini telescopes project that constructed telescopes in Hawaii and Chile. He has pioneered the use of a new class of astronomical spectrograph to measure the masses and ages of galaxies, as well as search for black holes in their nuclei. He was the founding director of the Hintze Centre for Astrophysical Surveys.

Contents

Early life and education

Davies was born in Scunthorpe, Lincolnshire, and grew up there, attending John Leggott Grammar School. A school project fired his interest in astronomy, augmented by his parents’ purchase of a small telescope. As a teenager Davies also attended evening classes run by the Workers' Educational Association, leading him to become a supporter of astronomy outreach work.

Career and research

Davies took his first degree in physics at University College London and his PhD at the Institute of Astronomy and Churchill College, Cambridge. Posts at Lick Observatory, California, then Cambridge and Kitt Peak National Observatory, Arizona, followed. While at Kitt Peak he became part of the Seven Samurai collaboration which surveyed the distances and velocities of 400 nearby elliptical galaxies, discovering the Great Attractor, at that time thought to be pulling the Milky Way and other galaxies in the direction of the constellations of Hydra and Centaurus.

Returning to the UK, Davies was based in Oxford leading the team that developed a proposal for UK participation in an 8-m telescope project which ultimately led to the establishment of the Gemini Observatory, twin 8m telescopes in Hawaii and Chile. He became Head of Astronomy at Durham University in 1994 where he developed his interest in integral field spectroscopy and played a leading role in building instruments for Gemini (GMOS) [3] and the William Herschel Telescope (SAURON). [4] [5] He used these to map the motions and composition of the gas and stars in galaxies leading to new insights into galaxy evolution and the supermassive black holes they host.

Davies returned to Oxford in 2002 as Philip Wetton Professor of Astrophysics (a post he holds in conjunction with a fellowship at Christ Church, Oxford) where he pursues research in cosmology and the evolution of galaxies. He was head of the physics department from 2005 to 2010 and head of astrophysics from 2011 to 2014. From 2014 - 2022 he was the founding director of the Oxford Hintze Centre for Astrophysical Surveys.

He was President of the Royal Astronomical Society between 2010 and 2012. [6]

References

  1. ↑ Lynden-Bell, D.; Faber, S. M.; Burstein, David; Davies, Roger L.; Dressler, Alan; Terlevich, R. J.; Wegner, Gary (March 1988). "Spectroscopy and photometry of elliptical galaxies. V - Galaxy streaming toward the new supergalactic center". The Astrophysical Journal. 326: 19. doi:10.1086/166066.
  2. ↑ "Roger Davies". www2.physics.ox.ac.uk. Retrieved 6 March 2020.
  3. ↑ Allington-Smith, J.; Murray, G.; Content, R.; Dodsworth, G.; Davies, R.; Miller, B. W.; Turner, J.; Jorgensen, I.; Hook, I.; Crampton, D.; Murowinski, R. (January 2002). "The GMOS Integral Field Unit: First Integral Field Spectroscopy with an 8m Telescope (Invited Talk)". ASPC. 282. San Francisco, Calif.: Astronomical Society of the Pacific: 415. arXiv: astro-ph/0202330 . Bibcode:2002ASPC..282..415A. ISBN   1-58381-125-7. ISSN   1050-3390. OCLC   51953629. The GMOS Integral Field Unit
  4. ↑ Miller, B. W. ((; Bureau)), M.; Verolme, E.; de Zeeuw, P. T.; Bacon, R.; Copin, Y.; Emsellem, E.; Davies, R. L.; Peletier, R. F.; Allington-Smith, J. R.; Carollo, C. M. (2000). "SAURON: Integral-field Spectroscopy of Galaxies (Poster)". ASPC. 195: 158. arXiv: astro-ph/9906091 . Bibcode:2000ASPC..195..158M. ISSN   1050-3390.
  5. ↑ Copin, Y.; Bacon, R.; Emsellem, E. ((; Bureau)), M.; Miller, B. W.; Verolme, E.; de Zeeuw, P. T.; Davies, R.; Peletier, R. F.; Carollo, M. C.; Monnet, G. (2000). "SAURON: First Results from Wide-field 3D-Spectroscopy of Galaxies". ASPC. 197: 249. Bibcode:2000ASPC..197..249C. ISSN   1050-3390.
  6. ↑ "List of presidents and dates of office". A brief history of the RAS. Royal Astronomical Society. Retrieved 3 February 2015.
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