Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
Menu
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.

Prof Michael Jones

Professor of Experimental Cosmology

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Cosmology
  • Experimental radio cosmology
  • C-BASS
  • The Square Kilometre Array (SKA)
Mike.Jones@physics.ox.ac.uk
Telephone: 01865 (2)73441
Denys Wilkinson Building, room 758
  • About
  • Publications

Astronomical receiver modelling using scattering matrices

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 446:2 (2015) 1252-1267

Authors:

OG King, Michael E Jones, C Copley, RJ Davis, JP Leahy, J Leech, SJC Muchovej, TJ Pearson, Angela C Taylor
More details from the publisher
More details
Details from ArXiV

Astronomical receiver modelling using scattering matrices

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 446:2 (2015) 1252-1267

Authors:

OG King, ME Jones, C Copley, RJ Davis, JP Leahy, J Leech, SJC Muchovej, TJ Pearson, AC Taylor

Effect of gain and phase errors on SKA1-Low imaging quality from 50-600 MHz

SKA Organisation (2014) 153

Authors:

D Sinclair, F Dulwich, B Mort, ME Jones, K Grainge, E de Lera Acedo
Details from ArXiV

The C-Band All-Sky Survey (C-BASS): design and implementation of the northern receiver

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 438:3 (2014) 2426-2439

Authors:

OG King, Michael E Jones, EJ Blackhurst, C Copley, RJ Davis, C Dickinson, CM Holler, MO Irfan, JJ John, JP Leahy, J Leech, SJC Muchovej, TJ Pearson, MA Stevenson, Angela C Taylor
More details from the publisher
More details
Details from ArXiV

SKA synergy with microwave background studies

Chapter in , 9-13-June-2014 (2014)

Authors:

C Burigana, P Alexander, C Baccigalupi, D Barbosa, A Blanchard, AD Rosa, G De Zotti, F Finelli, A Gruppuso, M Jones, S Matarrese, A Melchiorri, D Molinari, M Negrello, D Paoletti, F Perrotta, R Scaramella, T Trombetti

Abstract:

The extremely high sensitivity and resolution of the Square Kilometre Array (SKA) will be useful for addressing a wide set of themes relevant for cosmology, in synergy with current and future cosmic microwave background (CMB) projects. Many of these themes also have a link with future optical-IR and X-ray observations. We discuss the scientific perspectives for these goals, the instrumental requirements and the observational and data analysis approaches, and identify several topics that are important for cosmology and astrophysics at different cosmic epochs.

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 2
  • Page 3
  • Page 4
  • Page 5
  • Current page 6
  • Page 7
  • Page 8
  • Page 9
  • Page 10
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics
  • Current students
  • Staff intranet