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 | methods: data analysis | cosmic background radiation | MODE POLARIZATION | STATISTICS | DAMPING TAIL | PROBE WMAP OBSERVATIONS | ATACAMA COSMOLOGY TELESCOPE | ANISOTROPY | MICROWAVE BACKGROUND POLARIZATION | COUNTS | methods: statistical | TEMPERATURE | ASTRONOMY & ASTROPHYSICS | SCALES | cosmology: observations | cosmological parameters | 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 | data analysis methods | cosmology observations | statistical methods

Cosmological parameters | Methods: data analysis | Cosmology: observations | Methods: statistical | Cosmic background radiation | methods: data analysis | cosmic background radiation | MODE POLARIZATION | STATISTICS | DAMPING TAIL | PROBE WMAP OBSERVATIONS | ATACAMA COSMOLOGY TELESCOPE | ANISOTROPY | MICROWAVE BACKGROUND POLARIZATION | COUNTS | methods: statistical | TEMPERATURE | ASTRONOMY & ASTROPHYSICS | SCALES | cosmology: observations | cosmological parameters | 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 | data analysis methods | cosmology observations | statistical methods

Journal Article

Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2014, Volume 571, pp. A24 - 58

The Planck nominal mission cosmic microwave background (CMB) maps yield unprecedented constraints on primordial non-Gaussianity (NG). Using three optimal...

Cosmology: theory | Inflation | Methods: data analysis | Cosmology: observations | Cosmic background radiation | Early Universe | NONLINEAR COUPLING PARAMETER | methods: data analysis | cosmic background radiation | PROBE WMAP OBSERVATIONS | NEEDLET BISPECTRUM | MINKOWSKI FUNCTIONALS | early Universe | inflation | POLARIZATION ANISOTROPIES | cosmology: theory | WAVELET ESTIMATOR | MICROWAVE BACKGROUND BISPECTRUM | POINT SOURCES | ASTRONOMY & ASTROPHYSICS | cosmology: observations | COMPONENT SEPARATION | 3-POINT CORRELATION-FUNCTION | Reconstruction | Separation | Computer simulation | Cosmic microwave background | Missions | Estimates | Three dimensional models | Estimators | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | ASTRONOMY AND ASTROPHYSICS

Cosmology: theory | Inflation | Methods: data analysis | Cosmology: observations | Cosmic background radiation | Early Universe | NONLINEAR COUPLING PARAMETER | methods: data analysis | cosmic background radiation | PROBE WMAP OBSERVATIONS | NEEDLET BISPECTRUM | MINKOWSKI FUNCTIONALS | early Universe | inflation | POLARIZATION ANISOTROPIES | cosmology: theory | WAVELET ESTIMATOR | MICROWAVE BACKGROUND BISPECTRUM | POINT SOURCES | ASTRONOMY & ASTROPHYSICS | cosmology: observations | COMPONENT SEPARATION | 3-POINT CORRELATION-FUNCTION | Reconstruction | Separation | Computer simulation | Cosmic microwave background | Missions | Estimates | Three dimensional models | Estimators | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | ASTRONOMY AND ASTROPHYSICS

Journal Article

Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2016, Volume 594, pp. 1 - 31

We study the implications of Planck data for models of dark energy (DE) and modified gravity (MG) beyond the standard cosmological constant scenario. We start...

Gravitation | Cosmology: theory | Dark energy | Cosmic background radiation | DISTANCE | REDSHIFT SPACE DISTORTIONS | cosmic background radiation | HUBBLE CONSTANT | GROWTH-RATE | MAIN GALAXY SAMPLE | MODEL | dark energy | cosmology: theory | POWER SPECTRUM | gravitation | COSMOLOGICAL PARAMETERS | ASTRONOMY & ASTROPHYSICS | BARYON ACOUSTIC-OSCILLATIONS | CONSTRAINTS | Parametrization | Equations of state | Perturbation methods | Data sets | Scalars | Principal components analysis | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | ASTRONOMY AND ASTROPHYSICS

Gravitation | Cosmology: theory | Dark energy | Cosmic background radiation | DISTANCE | REDSHIFT SPACE DISTORTIONS | cosmic background radiation | HUBBLE CONSTANT | GROWTH-RATE | MAIN GALAXY SAMPLE | MODEL | dark energy | cosmology: theory | POWER SPECTRUM | gravitation | COSMOLOGICAL PARAMETERS | ASTRONOMY & ASTROPHYSICS | BARYON ACOUSTIC-OSCILLATIONS | CONSTRAINTS | Parametrization | Equations of state | Perturbation methods | Data sets | Scalars | Principal components analysis | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | ASTRONOMY AND ASTROPHYSICS

Journal Article

Astronomy and Astrophysics, ISSN 0004-6361, 10/2016, Volume 594, p. A17

The Planck full mission cosmic microwave background (CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial...

Cosmology: theory | Inflation | Methods: data analysis | Cosmology: observations | Cosmic background radiation | Early Universe | methods: data analysis | cosmic background radiation | LARGE-SCALE STRUCTURE | PROBE WMAP OBSERVATIONS | MINKOWSKI FUNCTIONALS | early Universe | inflation | POLARIZATION ANISOTROPIES | cosmology: theory | TEMPERATURE | POINT SOURCES | ASTRONOMY & ASTROPHYSICS | INFRARED BACKGROUND ANISOTROPIES | CMB | cosmology: observations | FAST ESTIMATOR | 3-POINT CORRELATION-FUNCTION | Polarization | Adiabatic flow | Amplitudes | Cosmic microwave background | Estimating | Gaussian | Estimators | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | ASTRONOMY AND ASTROPHYSICS | cosmology | theory

Cosmology: theory | Inflation | Methods: data analysis | Cosmology: observations | Cosmic background radiation | Early Universe | methods: data analysis | cosmic background radiation | LARGE-SCALE STRUCTURE | PROBE WMAP OBSERVATIONS | MINKOWSKI FUNCTIONALS | early Universe | inflation | POLARIZATION ANISOTROPIES | cosmology: theory | TEMPERATURE | POINT SOURCES | ASTRONOMY & ASTROPHYSICS | INFRARED BACKGROUND ANISOTROPIES | CMB | cosmology: observations | FAST ESTIMATOR | 3-POINT CORRELATION-FUNCTION | Polarization | Adiabatic flow | Amplitudes | Cosmic microwave background | Estimating | Gaussian | Estimators | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | ASTRONOMY AND ASTROPHYSICS | cosmology | theory

Journal Article

Astronomy and Astrophysics, ISSN 0004-6361, 02/2016, Volume 586, p. A133

The polarized thermal emission from diffuse Galactic dust is the main foreground present in measurements of the polarization of the cosmic microwave background...

cosmology: observations | polarization | cosmic background radiation | ISM: structure | ISM: magnetic fields | SYNCHROTRON | 353 GHZ | MODEL | RADIATION | MICROWAVE BACKGROUND POLARIZATION | PRE-LAUNCH STATUS | SUBMILLIMETER | ASTRONOMY & ASTROPHYSICS | HIGH-FREQUENCY | STATISTICAL PROPERTIES | MOLECULAR GAS | Sky | Polarization | Dust | Cosmic dust | Power spectra | Cosmic microwave background | Emission | Assessments | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | Astrophysics | ASTRONOMY AND ASTROPHYSICS | ISM magnetic fields | ISM structure | cosmology observations

cosmology: observations | polarization | cosmic background radiation | ISM: structure | ISM: magnetic fields | SYNCHROTRON | 353 GHZ | MODEL | RADIATION | MICROWAVE BACKGROUND POLARIZATION | PRE-LAUNCH STATUS | SUBMILLIMETER | ASTRONOMY & ASTROPHYSICS | HIGH-FREQUENCY | STATISTICAL PROPERTIES | MOLECULAR GAS | Sky | Polarization | Dust | Cosmic dust | Power spectra | Cosmic microwave background | Emission | Assessments | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | Astrophysics | ASTRONOMY AND ASTROPHYSICS | ISM magnetic fields | ISM structure | cosmology observations

Journal Article

Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2014, Volume 571, pp. A23 - 48

The two fundamental assumptions of the standard cosmological model - that the initial fluctuations are statistically isotropic and Gaussian - are rigorously...

Cosmology: miscellaneous | Cosmology: observations | Cosmic background radiation | cosmic background radiation | MICROWAVE-ANISOTROPY-PROBE | cosmology: miscellaneous | BIANCHI-VIIH | MINKOWSKI FUNCTIONALS | BACKGROUND TEMPERATURE | COLD SPOT | DEPENDENT NON-GAUSSIANITIES | WMAP OBSERVATIONS | HEMISPHERICAL POWER ASYMMETRY | PRIMORDIAL NON-GAUSSIANITY | ASTRONOMY & ASTROPHYSICS | cosmology: observations | POINT CORRELATION-FUNCTIONS | Isotropy | Construction | Computer simulation | Anisotropy | Cosmic microwave background | Astronomical models | Planck satellite | Statistics | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | ASTRONOMY AND ASTROPHYSICS

Cosmology: miscellaneous | Cosmology: observations | Cosmic background radiation | cosmic background radiation | MICROWAVE-ANISOTROPY-PROBE | cosmology: miscellaneous | BIANCHI-VIIH | MINKOWSKI FUNCTIONALS | BACKGROUND TEMPERATURE | COLD SPOT | DEPENDENT NON-GAUSSIANITIES | WMAP OBSERVATIONS | HEMISPHERICAL POWER ASYMMETRY | PRIMORDIAL NON-GAUSSIANITY | ASTRONOMY & ASTROPHYSICS | cosmology: observations | POINT CORRELATION-FUNCTIONS | Isotropy | Construction | Computer simulation | Anisotropy | Cosmic microwave background | Astronomical models | Planck satellite | Statistics | Physics - Cosmology and Nongalactic Astrophysics | Sciences of the Universe | Astrophysics | Cosmology and Extra-Galactic Astrophysics | Physics | ASTRONOMY AND ASTROPHYSICS

Journal Article

The Lancet (British edition), ISSN 0140-6736, 2011, Volume 378, Issue 9793, pp. 771 - 784

Summary Background As trials of 5 years of tamoxifen in early breast cancer mature, the relevance of hormone receptor measurements (and other patient...

Internal Medicine | MEDICINE, GENERAL & INTERNAL | POSTMENOPAUSAL | THERAPY | HIGH-RISK | DOXORUBICIN | RECURRENCE | PREMENOPAUSAL WOMEN | PROGESTERONE-RECEPTOR | ESTROGEN-RECEPTOR | CHEMOTHERAPY | IMMUNOHISTOCHEMISTRY | Receptors, Estrogen - metabolism | Neoplasm Recurrence, Local - prevention & control | Humans | Selective Estrogen Receptor Modulators - adverse effects | Breast Neoplasms - drug therapy | Breast Neoplasms - metabolism | Randomized Controlled Trials as Topic | Receptors, Progesterone - metabolism | Antineoplastic Agents, Hormonal - adverse effects | Selective Estrogen Receptor Modulators - therapeutic use | Breast Neoplasms - pathology | Neoplasms, Second Primary - chemically induced | Antineoplastic Agents, Hormonal - therapeutic use | Tamoxifen - therapeutic use | Breast Neoplasms - mortality | Female | Chemotherapy, Adjuvant | Tamoxifen - adverse effects | Patient outcomes | Breast cancer | Research | Diagnosis | Tamoxifen | Drug therapy | Health aspects | Chemotherapy | Compliance | Womens health | Mortality | Endocrine therapy | Data collection | Stratigraphy | Cancer therapies

Internal Medicine | MEDICINE, GENERAL & INTERNAL | POSTMENOPAUSAL | THERAPY | HIGH-RISK | DOXORUBICIN | RECURRENCE | PREMENOPAUSAL WOMEN | PROGESTERONE-RECEPTOR | ESTROGEN-RECEPTOR | CHEMOTHERAPY | IMMUNOHISTOCHEMISTRY | Receptors, Estrogen - metabolism | Neoplasm Recurrence, Local - prevention & control | Humans | Selective Estrogen Receptor Modulators - adverse effects | Breast Neoplasms - drug therapy | Breast Neoplasms - metabolism | Randomized Controlled Trials as Topic | Receptors, Progesterone - metabolism | Antineoplastic Agents, Hormonal - adverse effects | Selective Estrogen Receptor Modulators - therapeutic use | Breast Neoplasms - pathology | Neoplasms, Second Primary - chemically induced | Antineoplastic Agents, Hormonal - therapeutic use | Tamoxifen - therapeutic use | Breast Neoplasms - mortality | Female | Chemotherapy, Adjuvant | Tamoxifen - adverse effects | Patient outcomes | Breast cancer | Research | Diagnosis | Tamoxifen | Drug therapy | Health aspects | Chemotherapy | Compliance | Womens health | Mortality | Endocrine therapy | Data collection | Stratigraphy | Cancer therapies

Journal Article

Astronomy and Astrophysics, ISSN 0004-6361, 10/2016, Volume 594, p. A16

We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our...

Polarization | Methods: data analysis | Cosmology: observations | Methods: statistical | Cosmic background radiation | methods: data analysis | cosmic background radiation | MICROWAVE-ANISOTROPY-PROBE | MINKOWSKI FUNCTIONALS | POWER ASYMMETRY | COLD SPOT | WMAP OBSERVATIONS | methods: statistical | MAPS | ASTRONOMY & ASTROPHYSICS | BACKGROUND ANISOTROPY | cosmology: observations | polarization | FULL-SKY | NON-GAUSSIANITY | Isotropy | Maps | Anisotropy | Cosmic microwave background | Planck satellite | Missions | Statistics | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | ASTRONOMY AND ASTROPHYSICS | data analysis | cosmology observations | statistical methods

Polarization | Methods: data analysis | Cosmology: observations | Methods: statistical | Cosmic background radiation | methods: data analysis | cosmic background radiation | MICROWAVE-ANISOTROPY-PROBE | MINKOWSKI FUNCTIONALS | POWER ASYMMETRY | COLD SPOT | WMAP OBSERVATIONS | methods: statistical | MAPS | ASTRONOMY & ASTROPHYSICS | BACKGROUND ANISOTROPY | cosmology: observations | polarization | FULL-SKY | NON-GAUSSIANITY | Isotropy | Maps | Anisotropy | Cosmic microwave background | Planck satellite | Missions | Statistics | Physics - Cosmology and Nongalactic Astrophysics | Cosmology and Extra-Galactic Astrophysics | Sciences of the Universe | Astrophysics | ASTRONOMY AND ASTROPHYSICS | data analysis | cosmology observations | statistical methods

Journal Article

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

Journal Article