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P. G. Ferreira

Identifiers

  • name variant P. G. Ferreira 0.60 · backfill

Papers (27)

  1. \textit{Euclid} preparation. Baryon acoustic oscillations extraction techniques: comparison and optimisation astro-ph.CO · 2026 · author #218
  2. Euclid preparation. XCVI. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and Forecasts astro-ph.CO · 2025 · author #255
  3. Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$ astro-ph.GA · 2025 · author #239
  4. A comparison of Einstein-Boltzmann solvers for testing General Relativity astro-ph.CO · 2017 · author #14
  5. Probing the accelerating Universe with radio weak lensing in the JVLA Sky Survey astro-ph.CO · 2013 · author #15
  6. First Season QUIET Observations: Measurements of CMB Polarization Power Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475 astro-ph.CO · 2010 · author #21
  7. Vector field models of modified gravity and the dark sector astro-ph.CO · 2010 · author #4
  8. Detecting the B-mode Polarisation of the CMB with Clover astro-ph · 2008 · author #12
  9. Searching for non Gaussian signals in the BOOMERanG 2003 CMB maps astro-ph · 2007 · author #14
  10. The cosmological behavior of Bekenstein's modified theory of gravity astro-ph · 2006 · author #2
  11. The Cosmology of a Universe with Spontaneously-Broken Lorentz Symmetry astro-ph · 2006 · author #1
  12. Implications of the Cosmic Background Imager Polarization Data astro-ph · 2005 · author #8
  13. Measuring the geometry of the Universe in the presence of isocurvature modes astro-ph · 2005 · author #3
  14. Large Scale Structure in Bekenstein's theory of relativistic Modified Newtonian Dynamics astro-ph · 2005 · author #3
  15. Constraints on isocurvature models from the WMAP first-year data astro-ph · 2004 · author #4
  16. The initial conditions of the universe: how much isocurvature is allowed? astro-ph · 2004 · author #3
  17. Determining Foreground Contamination in CMB Observations: Diffuse Galactic Emission in the MAXIMA-I Field astro-ph · 2003 · author #5
  18. Multiple Methods for Estimating the Bispectrum of the Cosmic Microwave Background with Application to the MAXIMA Data astro-ph · 2002 · author #5
  19. The Trispectrum of the 4 Year COBE-DMR data astro-ph · 2001 · author #4
  20. Estimate of the Cosmological Bispectrum from the MAXIMA-1 Cosmic Microwave Background Map astro-ph · 2001 · author #4
  21. Isotropy and Stability of the Brane hep-ph · 2001 · author #3
  22. Asymmetric Beams in Cosmic Microwave Background Anisotropy Experiments astro-ph · 2000 · author #4
  23. Constraints on Cosmological Parameters from MAXIMA-1 astro-ph · 2000 · author #7
  24. MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees astro-ph · 2000 · author #8
  25. Measurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American test flight of BOOMERANG astro-ph · 1999 · author #11
  26. A measurement of Omega from the North American test flight of BOOMERANG astro-ph · 1999 · author #10
  27. A Bayesian estimate of the skewness of the Cosmic Microwave Background astro-ph · 1999 · author #2

Mentions

  • 1012.3191 #21 · backfill · confidence 0.70 P. G. Ferreira
  • 1002.0849 #4 · backfill · confidence 0.70 P. G. Ferreira
  • 0805.3690 #12 · backfill · confidence 0.70 P. G. Ferreira
  • 0705.1615 #14 · backfill · confidence 0.70 P. G. Ferreira

Frequent Coauthors