G. Efstathiou
University of California, Santa Barbara
4 papers in the Anchorcite directory, published between 1985 and 2020, cited 34,871 times in total.
ORCID profileResearch topics
- Galaxies: Formation, Evolution, Phenomena · 4 papers
- Cosmology and Gravitation Theories · 4 papers
- Dark Matter and Cosmic Phenomena · 2 papers
- Radio Astronomy Observations and Technology · 1 paper
- Scientific Research and Discoveries · 1 paper
Frequent co-authors
- N. Aghanim · 3 papers
- M. Ashdown · 3 papers
- J. Aumont · 3 papers
- Carlo Baccigalupi · 3 papers
- R. Belén Barreiro · 3 papers
- Marco Bersanelli · 3 papers
- P. Bielewicz · 3 papers
- J. J. Bock · 3 papers
Papers
- Planck 2018 resultsAstronomy and Astrophysics · 2020 · 14,290 citations
We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the temperature and polarization maps and the lensing reconstruction. Compared to the 2015 results, improved measurements of large-scale polarization…
- Planck 2015 resultsAstronomy and Astrophysics · 2016 · 10,612 citations
This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation.Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with…
- Planck 2013 results. XVI. Cosmological parametersAstronomy and Astrophysics · 2014 · 6,567 citations
This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra.We find that the Planck spectra at high multipoles (ℓ > ∼ 40) are extremely well described by the…
- The evolution of large-scale structure in a universe dominated by cold dark matterThe Astrophysical Journal · 1985 · 3,402 citations
The results of numerical simulations of nonlinear gravitational clustering in universes dominated by weakly interacting, 'cold' dark matter are presented. The numerical methods used and the way in which initial conditions were generated are described, and the simulations performed are…
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