Planck 2015 resultsCitation formats

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  • Planck Collaboration

Standard

Planck 2015 results : I. Overview of products and scientific results. / Planck Collaboration.

In: Astronomy & Astrophysics, Vol. 594, A1, 2015, p. 1-38.

Research output: Contribution to journalArticle

Harvard

Planck Collaboration 2015, 'Planck 2015 results: I. Overview of products and scientific results', Astronomy & Astrophysics, vol. 594, A1, pp. 1-38. https://doi.org/10.1051/0004-6361/201527101

APA

Planck Collaboration (2015). Planck 2015 results: I. Overview of products and scientific results. Astronomy & Astrophysics, 594, 1-38. [A1]. https://doi.org/10.1051/0004-6361/201527101

Vancouver

Author

Planck Collaboration. / Planck 2015 results : I. Overview of products and scientific results. In: Astronomy & Astrophysics. 2015 ; Vol. 594. pp. 1-38.

Bibtex

@article{d089188a1d124ad6bb01cc5878717313,
title = "Planck 2015 results: I. Overview of products and scientific results",
abstract = "The European Space Agency{\textquoteright}s Planck satellite, which is dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013. In February 2015, ESA and the Planck Collaboration released the second set of cosmology products based ondata from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the main characteristics of the data and the data products in the release, as well as the associated cosmological and astrophysical science results and papers. The data products include maps of the cosmic microwave background (CMB), the thermal Sunyaev-Zeldovich effect, diffuse foregrounds in temperature and polarization, catalogues of compact Galactic and extragalactic sources (including separate catalogues of Sunyaev-Zeldovich clusters and Galactic cold clumps), and extensive simulations of signals and noise used in assessing uncertainties and the performance of the analysis methods. The likelihood code used to assess cosmological models against the Planck data is described, along with a CMB lensing likelihood. Scientific results include cosmological parameters derived from CMB power spectra, gravitational lensing, and cluster counts, as well as constraints on inflation, non-Gaussianity, primordial magnetic fields, dark energy, and modified gravity, and new results on low-frequency Galactic foregrounds.",
keywords = "cosmology: observations, cosmic background radiation, space vehicles: instruments, nstrumentation: detectors, surveys",
author = "Clive Dickinson and {Planck Collaboration}",
year = "2015",
doi = "https://doi.org/10.1051/0004-6361/201527101",
language = "Undefined",
volume = "594",
pages = "1--38",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "EDP Sciences",

}

RIS

TY - JOUR

T1 - Planck 2015 results

T2 - I. Overview of products and scientific results

AU - Dickinson, Clive

AU - Planck Collaboration

PY - 2015

Y1 - 2015

N2 - The European Space Agency’s Planck satellite, which is dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013. In February 2015, ESA and the Planck Collaboration released the second set of cosmology products based ondata from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the main characteristics of the data and the data products in the release, as well as the associated cosmological and astrophysical science results and papers. The data products include maps of the cosmic microwave background (CMB), the thermal Sunyaev-Zeldovich effect, diffuse foregrounds in temperature and polarization, catalogues of compact Galactic and extragalactic sources (including separate catalogues of Sunyaev-Zeldovich clusters and Galactic cold clumps), and extensive simulations of signals and noise used in assessing uncertainties and the performance of the analysis methods. The likelihood code used to assess cosmological models against the Planck data is described, along with a CMB lensing likelihood. Scientific results include cosmological parameters derived from CMB power spectra, gravitational lensing, and cluster counts, as well as constraints on inflation, non-Gaussianity, primordial magnetic fields, dark energy, and modified gravity, and new results on low-frequency Galactic foregrounds.

AB - The European Space Agency’s Planck satellite, which is dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013. In February 2015, ESA and the Planck Collaboration released the second set of cosmology products based ondata from the entire Planck mission, including both temperature and polarization, along with a set of scientific and technical papers and a web-based explanatory supplement. This paper gives an overview of the main characteristics of the data and the data products in the release, as well as the associated cosmological and astrophysical science results and papers. The data products include maps of the cosmic microwave background (CMB), the thermal Sunyaev-Zeldovich effect, diffuse foregrounds in temperature and polarization, catalogues of compact Galactic and extragalactic sources (including separate catalogues of Sunyaev-Zeldovich clusters and Galactic cold clumps), and extensive simulations of signals and noise used in assessing uncertainties and the performance of the analysis methods. The likelihood code used to assess cosmological models against the Planck data is described, along with a CMB lensing likelihood. Scientific results include cosmological parameters derived from CMB power spectra, gravitational lensing, and cluster counts, as well as constraints on inflation, non-Gaussianity, primordial magnetic fields, dark energy, and modified gravity, and new results on low-frequency Galactic foregrounds.

KW - cosmology: observations

KW - cosmic background radiation

KW - space vehicles: instruments

KW - nstrumentation: detectors

KW - surveys

U2 - https://doi.org/10.1051/0004-6361/201527101

DO - https://doi.org/10.1051/0004-6361/201527101

M3 - Article

VL - 594

SP - 1

EP - 38

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

M1 - A1

ER -