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F. Couchot

Researcher at University of Paris-Sud

Publications -  182
Citations -  31551

F. Couchot is an academic researcher from University of Paris-Sud. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 95, co-authored 180 publications receiving 29846 citations.

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Planck 2015 results. XII. Full Focal Plane simulations

Peter A. R. Ade, +229 more
TL;DR: The 8th Full Focal Plane Simulation Set (FFP8) as mentioned in this paper was deployed in support of the Planck 2015 results and consists of 10 fiducial mission realizations reduced to 18144 maps, together with the most massive suite of Monte Carlo realizations of instrument noise and CMB ever generated.
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Planck 2013 results - VIII. HFI photometric calibration and mapmaking

Peter A. R. Ade, +284 more
TL;DR: In this paper, the authors describe the methods used to produce photometrically calibrated maps from the Planck High Frequency Instrument (HFI) cleaned, time-ordered information.
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Planck Early Results. X. Statistical analysis of Sunyaev-Zeldovich scaling relations for X-ray galaxy clusters

TL;DR: In this article, the relationship between the thermal Sunyaev-Zeldovich (SZ) signal and X-ray luminosity is investigated and the measured SZ signal is compared to values predicted from X-rays data.
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Planck early results. XXI. Properties of the interstellar medium in the Galactic plane

A. Abergel, +200 more
TL;DR: In this paper, the authors show that anomalous dust emission is present in the atomic, molecular and dark gas phases throughout the Galactocentricity of the Galactic disk, and the derived dust propeties associated with the dark gas phase are derived but do not allow us to reveal the nature of this phase.
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Planck 2015 results: XXI. The integrated Sachs-Wolfe effect

Peter A. R. Ade, +279 more
TL;DR: In this article, the integrated Sachs-Wolfe (ISW) effect from the Planck 2015 temperature and polarization data release is investigated from different perspectives, and the authors show that the ISW effect is detected only at ≈3σ, which is similar to the detection level achieved by combining the cross-correlation signal coming from all the galaxy catalogues mentioned above.