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Planck 2018 results: VII. Isotropy and statistics of the CMB
- Source :
- Astronomy & Astrophysics, 641, 1-61, Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2020, 641, pp.A7. ⟨10.1051/0004-6361/201935201⟩, Astron.Astrophys., Astron.Astrophys., 2020, 641, pp.A7, Astronomy & Astrophysics. Vol 641, Augt 2021. A7, UCrea Repositorio Abierto de la Universidad de Cantabria, Universidad de Cantabria (UC), WOS:000571763700007, RUO: Repositorio Institucional de la Universidad de Oviedo, Universidad de Oviedo (UNIOVI), Digital.CSIC. Repositorio Institucional del CSIC, instname, Astronomy & Astrophysics, 641, pp. 1-61, RUO. Repositorio Institucional de la Universidad de Oviedo, Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 641, pp.A7. ⟨10.1051/0004-6361/201935201⟩
- Publication Year :
- 2020
-
Abstract
- Planck Collaboration: et al.<br />Analysis of the Planck 2018 data set indicates that the statistical properties of the cosmic microwave background (CMB) temperature anisotropies are in excellent agreement with previous studies using the 2013 and 2015 data releases. In particular, they are consistent with the Gaussian predictions of the ΛCDM cosmological model, yet also confirm the presence of several so-called “anomalies” on large angular scales. The novelty of the current study, however, lies in being a first attempt at a comprehensive analysis of the statistics of the polarization signal over all angular scales, using either maps of the Stokes parameters, Q and U, or the E-mode signal derived from these using a new methodology (which we describe in an appendix). Although remarkable progress has been made in reducing the systematic effects that contaminated the 2015 polarization maps on large angular scales, it is still the case that residual systematics (and our ability to simulate them) can limit some tests of non-Gaussianity and isotropy. However, a detailed set of null tests applied to the maps indicates that these issues do not dominate the analysis on intermediate and large angular scales (i.e., ℓ ≲ 400). In this regime, no unambiguous detections of cosmological non-Gaussianity, or of anomalies corresponding to those seen in temperature, are claimed. Notably, the stacking of CMB polarization signals centred on the positions of temperature hot and cold spots exhibits excellent agreement with the ΛCDM cosmological model, and also gives a clear indication of how Planck provides state-of-the-art measurements of CMB temperature and polarization on degree scales.<br />The Planck Collaboration acknowledges the support of: ESA; CNES, and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); ERC andPRACE (EU).
- Subjects :
- statistical [Methods]
cosmological model
POWER SPECTRUM
Astronomy
Gaussian
Cosmic microwave background
cosmic background radiation: polarization
Astrophysics
Residual
Cosmic background radiation
7. Clean energy
01 natural sciences
Cosmology: observation
Polarization
Statistics
Stokes parameters
MICROWAVE
Anisotropy
observations [Cosmology]
data analysis [Methods]
010303 astronomy & astrophysics
Methods: statistical
Physics
Cosmology: observations
Polarization (waves)
symbols
astro-ph.CO
Methods: data analysis
COLD SPOTS
Astrophysics - Cosmology and Nongalactic Astrophysics
temperature: anisotropy
data analysis method
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
satellite: Planck
FOS: Physical sciences
anomaly
Astrophysics::Cosmology and Extragalactic Astrophysics
Astronomy & Astrophysics
NO
symbols.namesake
statistical analysis
Settore FIS/05 - Astronomia e Astrofisica
0103 physical sciences
0201 Astronomical and Space Sciences
ESTIMATOR
Planck
DISCRETIZATION
010308 nuclear & particles physics
Computer Science::Information Retrieval
Isotropy
Astronomy and Astrophysics
ANOMALOUS NATURE
115 Astronomy, Space science
cosmic background radiation: temperature
INCOMPLETE-SKY
13. Climate action
Space and Planetary Science
Cosmic background radiation, Cosmology: observations, Methods: data analysis, Methods: statistical, Polarization
NON-GAUSSIANITY
PROBE WMAP OBSERVATIONS
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Methods: data analysi
Subjects
Details
- ISSN :
- 14320746 and 00046361
- Database :
- OpenAIRE
- Journal :
- Astronomy & Astrophysics, 641, 1-61, Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, 2020, 641, pp.A7. ⟨10.1051/0004-6361/201935201⟩, Astron.Astrophys., Astron.Astrophys., 2020, 641, pp.A7, Astronomy & Astrophysics. Vol 641, Augt 2021. A7, UCrea Repositorio Abierto de la Universidad de Cantabria, Universidad de Cantabria (UC), WOS:000571763700007, RUO: Repositorio Institucional de la Universidad de Oviedo, Universidad de Oviedo (UNIOVI), Digital.CSIC. Repositorio Institucional del CSIC, instname, Astronomy & Astrophysics, 641, pp. 1-61, RUO. Repositorio Institucional de la Universidad de Oviedo, Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 641, pp.A7. ⟨10.1051/0004-6361/201935201⟩
- Accession number :
- edsair.doi.dedup.....3beeeed061a69c62a915061d77b5dd61