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91探花
Black Hole

Lensing of space time around a black hole. At 91探花 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

Estimate of the Cosmological Bispectrum from the MAXIMA-1 Cosmic Microwave Background Map

Physical Review Letters 88 (2002) 241302 4pp

Authors:

P Ferreira, M. Santos, S. Hanany, J. Magueijo

Making maps of the cosmic microwave background: The MAXIMA example

Physical Review D 65:2 (2002)

Authors:

R Stompor, A Balbi, JD Borrill, PG Ferreira, S Hanany, AH Jaffe, AT Lee, S Oh, B Rabii, PL Richards, GF Smoot, CD Winant, JHP Wu

Abstract:

This work describes cosmic microwave background (CMB) data analysis algorithms and their implementations, developed to produce a pixelized map of the sky and a corresponding pixel-pixel noise correlation matrix from time ordered data for a CMB mapping experiment. We discuss in turn algorithms for estimating noise properties from the time ordered data, techniques for manipulating the time ordered data, and a number of variants of the maximum likelihood map-making procedure. We pay particular attention to issues pertinent to real CMB data, and present ways of incorporating them within the framework of maximum likelihood map making. Making a map of the sky is shown to be not only an intermediate step rendering an image of the sky, but also an important diagnostic stage, when tests for and/or removal of systematic effects can efficiently be performed. The case under study is the MAXIMA-I data set. However, the methods discussed are expected to be applicable to the analysis of other current and forthcoming CMB experiments. 漏2001 The American Physical Society.

The MAXIMA and MAXIPOL experiments

EXPERIMENTAL COSMOLOGY AT MILLIMETRE WAVELENGTHS 616 (2002) 12-17

Authors:

PL Richards, M Abroe, P Ade, A Balbi, J Bock, J Borrill, A Boscaleri, P de Bernardis, J Collins, PG Ferreira, S Hanany, VV Hristov, AH Jaffe, B Johnson, AT Lee, T Matsumu, PD Mauskopf, CB Netterfield, E Pascale, B Rabii, GF Smoot, R Stompor, CD Winant, JHP Wu

Tests for Gaussianity of the MAXIMA-1 cosmic microwave background map

Physical Review Letters 87:25 (2001)

Authors:

JHP Wu, A Balbi, J Borrill, PG Ferreira, S Hanany, AH Jaffe, AT Lee, B Rabii, PL Richards, GF Smoot, R Stompor, CD Winant

Abstract:

A series of Gaussianity tests were performed on the MAXIMA-1 CMB map. To optimize both the resolution and the signal-to-noise ratio for these tests, a map with 5972 square pixels of 8' each was used. Using these high-quality data, the Gaussianity of CMB anisotropy on subdegree scales was probed for the first time. It was found that the MAXIMA-1 CMB map is consistent with Gaussianity on angular scales between 10 arcmin and 5 deg.

Have Acoustic Oscillations been Detected in the Current Cosmic Microwave Background Data?

(2001)

Authors:

M Douspis, PG Ferreira

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