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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 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

The science case for PILOT I: Summary and overview

Publications of the Astronomical Society of Australia 26:4 (2009) 379-396

Authors:

JS Lawrence, MCB Ashley, J Bailey, D Barrado Y Navascues, TR Beddings, J Bland-Hawthorn, I Bond, E Boulanger, R Bouwens, H Bruntt, A Bunker, D Burgarella, MG Burton, M Busso, D Coward, MR Cioni, G Durands, C Eiroa, N Epchtein, N Gehrels, R Gillingham, K Glazebrook, R Haynes, L Kiss, PO Lagage, T Le Bertre, C Mackay, JP Maillard, A McGrath, V Minier, A Mora, K Olsen, P Persi, K Pimbblet, R Quimby, W Saunders, B Schmidt, D Stello, JWV Storey, C Tinney, P Tremblin, JC Wheeler, P Yock

Abstract:

PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed 2.5-m optical/ infrared telescope to be located at Dome C on the Antarctic plateau. Conditions at Dome C are known to be exceptional for astronomy. The seeing (above ∼30 m height), coherence time, and isoplanatic angle are all twice as good as at typical mid-latitude sites, while the water-vapour column, and the atmosphere and telescope thermal emission are all an order of magnitude better. These conditions enable a unique scientific capability for PILOT, which is addressed in this series of papers. The current paper presents an overview of the optical and instrumentation suite for PILOT and its expected performance, a summary of the key science goals and observational approach for the facility, a discussion of the synergies between the science goals for PILOT and other telescopes, and a discussion of the future of Antarctic astronomy. Paper II and Paper III present details of the science projects divided, respectively, between the distant Universe (i.e. studies of first light, and the assembly and evolution of structure) and the nearby Universe (i.e. studies of Local Group galaxies, the Milky Way, and the Solar System). © Astronomical Society of Australia 2009.
More details from the publisher

GRB 080503: IMPLICATIONS OF A NAKED SHORT GAMMA-RAY BURST DOMINATED BY EXTENDED EMISSION

ASTROPHYSICAL JOURNAL 696:2 (2009) 1871-1885

Authors:

DA Perley, BD Metzger, J Granot, NR Butler, T Sakamoto, E Ramirez-Ruiz, AJ Levan, JS Bloom, AA Miller, A Bunker, H-W Chen, AV Filippenko, N Gehrels, K Glazebrook, PB Hall, KC Hurley, D Kocevski, W Li, S Lopez, J Norris, AL Piro, D Poznanski, JX Prochaska, E Quataert, N Tanvir
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Pushing FORS to the Limit—A New Population of Faint Extended Lyα Emitters at z∼3

Astrophysics and Space Science Proceedings Springer Nature (2009) 23-26

Authors:

Martin G Haehnelt, Michael Rauch, Andrew Bunker, George Becker, Francine Marleau, James Graham, Stefano Cristiani, Matt J Jarvis, Cedric Lacey, Simon Morris, Celine Peroux, Huub Röttgering, Tom Theuns
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GRB 080503: Implications of a Naked Short Gamma-Ray Burst Dominated by Extended Emission

(2008)

Authors:

DA Perley, BD Metzger, J Granot, NR Butler, T Sakamoto, E Ramirez-Ruiz, AJ Levan, JS Bloom, AA Miller, A Bunker, H-W Chen, AV Filippenko, N Gehrels, K Glazebrook, PB Hall, KC Hurley, D Kocevski, W Li, S Lopez, J Norris, AL Piro, D Poznanski, JX Prochaska, E Quataert, N Tanvir
More details from the publisher

Tracing metallicities in the Universe with the James Webb Space Telescope

Chapter in The Metal-Rich Universe, Cambridge University Press (CUP) (2008) 212-224

Authors:

R Maiolino, S Arribas, T Böker, A Bunker, S Charlot, G de Marchi, P Ferruit, M Franx, P Jakobsen, H Moseley, T Nagao, L Origlia, B Rauscher, M Regan, HW Rix, CJ Willott
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