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G

G. Polenta

Researcher at Agenzia Spaziale Italiana

Publications -  379
Citations -  104689

G. Polenta is an academic researcher from Agenzia Spaziale Italiana. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 136, co-authored 337 publications receiving 92816 citations. Previous affiliations of G. Polenta include INAF.

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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.
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Euclid preparation: VII. Forecast validation for Euclid cosmological probes

Alain Blanchard, +152 more
TL;DR: In this article, the authors present validated numerical codes and methods for Euclid cosmological forecasts for galaxy clustering, weak lensing, and their combination, which can be used to validate their own codes if required.
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Planck 2015 results - XII. Full focal plane simulations

Peter A. R. Ade, +294 more
TL;DR: Generated at a cost of some 25 million CPU-hours spread across multiple high-performance-computing (HPC) platforms, FFP8 is used to validate and verify analysis algorithms and their implementations, and to remove biases from and quantify uncertainties in the results of analyses of the real data.
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Planck early results. XVII. Origin of the submillimetre excess dust emission in the Magellanic Clouds

Peter A. R. Ade, +234 more
TL;DR: In this paper, the authors investigated the source of the millimetre excess in the spectral energy distribution of the Large Magellanic Cloud (LMC) and Small Magellan Cloud (SMC) using the Planck data.
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Planck 2013 results. VIII. HFI photometric calibration and mapmaking

Peter A. R. Ade, +224 more
TL;DR: In this article, the authors describe the processing applied to the HFI cleaned time-ordered data to produce photometrically calibrated maps, based on the photometric calibration parameters and detail the scheme used to a posteriori set the zero level of the maps.