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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 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
  • About
  • Publications

Streaming velocities as a dynamical estimator of 惟

ASTROPHYSICAL JOURNAL 515:1 (1999) L1-L4

Authors:

PG Ferreira, R Juszkiewicz, HA Feldman, M Davis, AH Jaffe

The 4 year COBE DMR data is non-Gaussian

3 K COSMOLOGY 476 (1999) 293-297

Authors:

PG Ferreira, KM G贸rski, J Magueijo

Where is COBE maps' non-Gaussianity?

COSMO-98: SECOND INTERNATIONAL WORKSHOP ON PARTICLE PHYSICS AND THE EARLY UNIVERSE 478 (1999) 176-179

Authors:

J Magueijo, PG Ferreira, KM G贸rski

Streaming velocities as a dynamical estimator of Omega

(1998)

Authors:

PG Ferreira, R Juszkiewicz, HA Feldman, M Davis, AH Jaffe

Evidence for non-Gaussianity in the CMB

ArXiv astro-ph/9810414 (1998)

Authors:

J Magueijo, P Ferreira, K Gorski

Abstract:

In a recent Letter we have shown how COBE-DMR maps may be used to disprove Gaussianity at a high confidence level. In this report we digress on a few issues closely related to this Letter. We present the general formalism for surveying non-Gaussianity employed. We present a few more tests for systematics. We wonder about the theoretical implications of our result.

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