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
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.

Professor Pedro Ferreira

Professor of Astrophysics

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
pedro.ferreira@physics.ox.ac.uk
Telephone: 01865 (2)73366
Denys Wilkinson Building, room 757
Personal Webpage
  • About
  • Publications

Determining Foreground Contamination in Cosmic Microwave Background Observations: Diffuse Galactic Emission in the MAXIMA-I Field

The Astrophysical Journal American Astronomical Society 615:1 (2004) 55-62

Authors:

AH Jaffe, A Balbi, JR Bond, J Borrill, PG Ferreira, D Finkbeiner, S Hanany, AT Lee, B Rabii, PL Richards, GF Smoot, R Stompor, CD Winant, JHP Wu
More details from the publisher

Initial conditions of the Universe: How Much Isocurvature is Allowed?

Physical Review Letters 93 (2004) 081301 4pp

Authors:

P Ferreira, M. Bucher, K. Moodley, J. Dunkley
More details from the publisher
Details from ArXiV

Constraints on isocurvature models from the WMAP first-year data

(2004)

Authors:

K Moodley, M Bucher, J Dunkley, PG Ferreira, C Skordis
More details from the publisher

Simulation of non-Gaussian CMB maps

(2004)

Authors:

Graca Rocha, MP Hobson, Sarah Smith, Pedro Ferreira, Anthony Challinor
More details from the publisher

Simulation of non-Gaussian CMB maps

ArXiv astro-ph/0406136 (2004)

Authors:

Graca Rocha, MP Hobson, Sarah Smith, Pedro Ferreira, Anthony Challinor

Abstract:

A simple method is presented for the rapid simulation of statistically-isotropic non-Gaussian maps of CMB temperature fluctuations with a given power spectrum and analytically-calculable bispectrum and higher-order polyspectra. The $n$th-order correlators of the pixel values may also be calculated analytically. The cumulants of the simulated map may be used to obtain an expression for the probability density function of the pixel temperatures. The statistical properties of the simulated map are determined by the univariate non-Gaussian distribution from which pixel values are drawn independently in the first stage of the simulation process. We illustrate the method using a non-Gaussian distribution derived from the wavefunctions of the harmonic oscillator. The basic simulation method is easily extended to produce non-Gaussian maps with a given power spectrum and diagonal bispectrum.
Details from ArXiV
More details from the publisher
More details

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 82
  • Page 83
  • Page 84
  • Page 85
  • Current page 86
  • Page 87
  • Page 88
  • Page 89
  • Page 90
  • …
  • 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
  • Current students
  • Staff intranet