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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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Magnetic fields from reionisation

TL;DR: In this paper, it was shown that soft X-ray photons could contribute to a significant premagnetisation of the intergalactic medium at a redshift of $z=15.
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Planck intermediate results: XXXVI. Optical identification and redshifts of Planck SZ sources with telescopes at the Canary Islands observatories

Peter A. R. Ade, +233 more
TL;DR: The results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with telescopes at the Canary Islands observatories as part of the general optical follow-up programme undertaken by the Planck Collaboration are discussed in this article.
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Planck intermediate results. XXIII. Galactic plane emission components derived from Planck with ancillary data

Peter A. R. Ade, +190 more
TL;DR: In this article, the spectral energy distributions (SEDs) at positions along the Galactic plane using the wide frequency coverage of Planck (28.4-857GHz) in combination with low-frequency radio data at 0.408-2.3GHz plus WMAP data at 23-94GHz, along with far-infrared (FIR) data from DIRBE and IRAS.
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Optimising large galaxy surveys for ISW detection

TL;DR: In this article, the authors investigate the potential of next-generation surveys of the cosmic microwave background and large-scale structure, to constrain the nature of dark energy, by means of the cross-correlation of the Integrated Sachs-Wolfe effect with the galaxy distribution.
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Planck intermediate results: XLIII. Spectral energy distribution of dust in clusters of galaxies

R. Adam, +249 more
TL;DR: In this article, the spectral energy distribution (SED) of the infrared spectrum of thermal dust emission in clusters of galaxies was obtained by using a stacking approach for a sample of several hundred objects from the Planck cluster sample; this procedure averaged out fluctuations from the IR sky, allowing to reach a significant detection of the faint cluster contribution.