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Nabila Aghanim

Researcher at Université Paris-Saclay

Publications -  450
Citations -  110271

Nabila Aghanim is an academic researcher from Université Paris-Saclay. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 137, co-authored 416 publications receiving 100914 citations. Previous affiliations of Nabila Aghanim include University of Paris-Sud & University of Paris.

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Planck Early Results: The High Frequency Instrument data processing

TL;DR: In this paper, the authors describe the processing of the 334 billion raw data samples from the High Frequency Instrument (hereafter HFI) which they performed to produce six temperature maps from the first 295 days of Planck-HFI survey data.
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Planck intermediate results (Corrigendum) - V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect

Peter A. R. Ade, +272 more
TL;DR: Author(s): Ade, PAR; Aghanim, N; Arnaud, M; Ashdown, M ; Atrio-Barandela, F; Aumont, J; Baccigalupi, C; Balbi, A; Banday, AJ; Barreiro, RB; Bartlett, JG; Battaner, E; Benabed, K; Bernard, J-P; Bersanelli, M.
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Planck intermediate results. XV. A study of anomalous microwave emission in Galactic clouds

Peter A. R. Ade, +181 more
TL;DR: In this paper, the authors used WMAP and Planck maps, combined with ancillary radio and IR data, to construct a sample of 98 candidate AME sources, assembling SEDs for each source using aperture photometry on 1deg-smoothed maps from 0.408 GHz up to 3000 GHz.
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The cross-correlation of the CMB polarisation and the 21-cm line fluctuations from cosmic reionisation

TL;DR: In this article, the cross-correlation between the CMB polarisation (E-modes) and the 21 cm line fluctuations can be used to gain further understanding of the reionisation history, within the framework of inhomogeneous reionization.
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Large Scale Magnetogenesis Through Radiation Pressure

TL;DR: In this article, a new model for the generation of magnetic fields on large scales occurring at the end of cosmological reionisation is presented, where the inhomogeneous radiation provided by luminous sources and the fluctuations in the matter density field are the major ingredients of the model.