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91̽»¨
Black Hole

Lensing of space time around a black hole. At 91̽»¨ 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 Andrew Bunker

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Galaxy formation and evolution
Andy.Bunker@physics.ox.ac.uk
Telephone: 01865 (2)83126
Denys Wilkinson Building, room 702
  • About
  • Publications

A New Measurement of the Stellar Mass Density at z~5: Implications for the Sources of Cosmic Reionization

(2006)

Authors:

DP Stark, AJ Bunker, RS Ellis, LP Eyles, M Lacy

Galaxies atz≈ 6–i′-drop selection and the GLARE Project

Chapter in Planets to Cosmology, Cambridge University Press (CUP) (2006) 185-194

Authors:

Elizabeth R Stanway, Karl Glazebrook, Andrew J Bunker

Galaxies Under the Cosmic Microscope: Resolved Spectroscopy and New Constraints on the z=1 Tully-Fisher relation

(2006)

Authors:

M Swinbank, R Bower, GP Smith, Ian Smail, J-P Kneib, R Ellis, D Stark, A Bunker

A Spitzer-IRS search for the galaxies that re-ionized the Universe

Proceedings of the International Astronomical Union 2:14 (2006) 249

Authors:

M Lacy, AJ Bunker, JP Kneib, HI Teplitz

Abstract:

We describe an observation designed to find H emission from galaxies at z712 made using the InfraRed spectrograph (IRS) on the Spitzer Space Telescope. © 2007 International Astronomical Union.

Galaxies in the first billion years: Implications for re-ionization and the star formation history at z>6

Proceedings of the International Astronomical Union 2:14 (2006) 248

Authors:

AJ Bunker, ER Stanway, LP Eyles, RS Ellis, RG McMahon, M Lacy, DP Stark

Abstract:

We discuss the selection of star-forming galaxies at z6 through the Lyman-break technique. Spitzer imaging implies many of these contain older stellar populations (>200Myr) which produce detectable Balmer breaks. The ages and stellar masses (1010M) imply that the star formation rate density at earlier epochs may have been significantly higher than at z6, and might have played a key role in re-ionizing the universe. © 2007 International Astronomical Union.

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