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## Search Articles

Astronomy and astrophysics (Berlin), ISSN 0004-6361, 10/2016, Volume 594, p. A13

...), a matter density parameter Omega(m) = 0.308 +/- 0.012, and a tilted scalar spectral index with ns = 0.968...

Physical Sciences | Astronomy & Astrophysics | Science & Technology | Polarization | Parameters | Supernovae | Mathematical analysis | Neutrinos | Cosmology | Mathematical models | Standards | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | ASTRONOMY AND ASTROPHYSICS | cosmology: observations | cosmic background radiation | cosmological parameters | cosmology: thoery

Physical Sciences | Astronomy & Astrophysics | Science & Technology | Polarization | Parameters | Supernovae | Mathematical analysis | Neutrinos | Cosmology | Mathematical models | Standards | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | ASTRONOMY AND ASTROPHYSICS | cosmology: observations | cosmic background radiation | cosmological parameters | cosmology: thoery

Journal Article

Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2016, Volume 594, pp. 1 - 63

Journal Article

Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2016, Volume 594, p. A11

This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlation functions of the cosmic microwave background (CMB)...

Cosmological parameters | Methods: data analysis | Cosmology: observations | Methods: statistical | Cosmic background radiation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Polarization | Uncertainty | Cosmic microwave background | Multipoles | Emission | Cosmology | Robustness | Spectra | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | ASTRONOMY AND ASTROPHYSICS | cosmic background radiation | data analysis methods | cosmology observations | cosmological parameters | statistical methods

Cosmological parameters | Methods: data analysis | Cosmology: observations | Methods: statistical | Cosmic background radiation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Polarization | Uncertainty | Cosmic microwave background | Multipoles | Emission | Cosmology | Robustness | Spectra | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | ASTRONOMY AND ASTROPHYSICS | cosmic background radiation | data analysis methods | cosmology observations | cosmological parameters | statistical methods

Journal Article

Astronomy and astrophysics (Berlin), ISSN 1432-0746, 10/2014, Volume 571, pp. A16 - 66

... (l greater than or similar to 40) are extremely well described by the standard spatially-flat six-parameter ACDM cosmology with a power-law spectrum of adiabatic scalar perturbations...

Inflation | Cosmological parameters | Primordial nucleosynthesis | Cosmic background radiation | Early Universe | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Cosmic microwave background | Multipoles | Cosmology | Scalars | Mathematical models | Spectra | Standards | Astronomy | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | ASTRONOMY AND ASTROPHYSICS

Inflation | Cosmological parameters | Primordial nucleosynthesis | Cosmic background radiation | Early Universe | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Cosmic microwave background | Multipoles | Cosmology | Scalars | Mathematical models | Spectra | Standards | Astronomy | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | ASTRONOMY AND ASTROPHYSICS

Journal Article