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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
Personal Webpage
  • About
  • Publications

Simultaneous Estimation of Noise and Signal in Cosmic Microwave Background Experiments

ArXiv astro-ph/9909250 (1999)

Authors:

Pedro G Ferreira, Andrew H Jaffe

Abstract:

To correctly analyse data sets from current microwave detection technology, one is forced to estimate the sky signal and experimental noise simultaneously. Given a time-ordered data set we propose a formalism and method for estimating the signal and associated errors without prior knowledge of the noise power spectrum. We derive the method using a Bayesian formalism and relate it to the standard methods; in particular we show how this leads to a change in the estimate of the noise covariance matrix of the sky signal. We study the convergence and accuracy of the method on two mock observational strategies and discuss its application to a currently-favoured calibration procedure.
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Simultaneous Estimation of Noise and Signal in Cosmic Microwave Background Experiments

(1999)

Authors:

Pedro G Ferreira, Andrew H Jaffe
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Measuring Omega with Galaxy Streaming Velocities

(1999)

Authors:

PG Ferreira, M Davis, HA Feldman, AH Jaffe, R Juszkiewicz
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The 4 Year COBE DMR data is non-Gaussian

(1999)

Authors:

PG Ferreira, KM Gorski, J Magueijo
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The 4 Year COBE DMR data is non-Gaussian

ArXiv astro-ph/9904073 (1999)

Authors:

PG Ferreira, KM Gorski, J Magueijo

Abstract:

I review our recent claim that there is evidence of non-Gaussianity in the 4 Year COBE DMR data. I describe the statistic we apply, the result we obtain and make a detailed list of the systematics we have analysed. I finish with a qualitative understanding of what it might be and its implications.
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