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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.

Jo Dunkley

Visitor

Sub department

  • Astrophysics
jo.dunkley@physics.ox.ac.uk
Denys Wilkinson Building, room 532E
  • About
  • Publications

FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: LIKELIHOODS AND PARAMETERS FROM THE WMAP DATA

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 180:2 (2009) 306-329

Authors:

J Dunkley, E Komatsu, MR Nolta, DN Spergel, D Larson, G Hinshaw, L Page, CL Bennett, B Gold, N Jarosik, JL Weiland, M Halpern, RS Hill, A Kogut, M Limon, SS Meyer, GS Tucker, E Wollack, EL Wright
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FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: ANGULAR POWER SPECTRA

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 180:2 (2009) 296-305

Authors:

MR Nolta, J Dunkley, RS Hill, G Hinshaw, E Komatsu, D Larson, L Page, DN Spergel, CL Bennett, B Gold, N Jarosik, N Odegard, JL Weiland, E Wollack, M Halpern, A Kogut, M Limon, SS Meyer, GS Tucker, EL Wright
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FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: DATA PROCESSING, SKY MAPS, AND BASIC RESULTS

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 180:2 (2009) 225-245

Authors:

G Hinshaw, JL Weiland, RS Hill, N Odegard, D Larson, CL Bennett, J Dunkley, B Gold, MR Greason, N Jarosik, E Komatsu, MR Nolta, L Page, DN Spergel, E Wollack, M Halpern, A Kogut, M Limon, SS Meyer, GS Tucker, EL Wright
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Prospects for polarized foreground removal

CMB POLARIZATION WORKSHOP: THEORY AND FOREGROUNDS 1141 (2009) 222-+

Authors:

J Dunkley, A Amblard, C Baccigalupi, M Betoule, D Chuss, A Cooray, J Delabrouille, C Dickinson, G Dobler, J Dotson, HK Eriksen, D Finkbeiner, D Fixsen, P Fosalba, A Fraisse, C Hirata, A Kogut, J Kristiansen, C Lawrence, AM Magalhaes, MA Miville-Deschenes, S Meyer, A Miller, SK Naess, L Page, HV Peiris, N Phillips, E Pierpaoli, G Rocha, JE Vaillancourt, L Verde
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CMBPol Mission Concept Study: A Mission to Map our Origins

ArXiv 0811.3911 (2008)

Authors:

Daniel Baumann, Asantha Cooray, Scott Dodelson, Joanna Dunkley, Aurélien A Fraisse, Mark G Jackson, Al Kogut, Lawrence M Krauss, Kendrick M Smith, Matias Zaldarriaga

Abstract:

Quantum mechanical metric fluctuations during an early inflationary phase of the universe leave a characteristic imprint in the polarization of the cosmic microwave background (CMB). The amplitude of this signal depends on the energy scale at which inflation occurred. Detailed observations by a dedicated satellite mission (CMBPol) therefore provide information about energy scales as high as $10^{15}$ GeV, twelve orders of magnitude greater than the highest energies accessible to particle accelerators, and probe the earliest moments in the history of the universe. This summary provides an overview of a set of studies exploring the scientific payoff of CMBPol in diverse areas of modern cosmology, such as the physics of inflation, gravitational lensing and cosmic reionization, as well as foreground science and removal .
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