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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 2013 results. XVIII. The gravitational lensing-infrared background correlation

Peter A. R. Ade, +290 more
TL;DR: In this paper, the authors measured the SFR density with around 2 sigma significance for three redshift bins between z=1 and 7, thus opening a new window into the study of the formation of stars at early times.
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Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies

Peter A. R. Ade, +195 more
TL;DR: In this article, the scaling relation between Sunyaev-Zeldovich (SZ) signal and stellar mass for almost 260,000 locally brightest galaxies (LBGs) selected from the Sloan Digital Sky Survey (SDSS) was presented.
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Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates

Nabila Aghanim, +198 more
TL;DR: In this paper, the XMM-Newton follow-up for confirmation of Planck cluster candidates is presented, where a total of 21 candidates are confirmed as extended X-ray sources.
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Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates

Nabila Aghanim, +225 more
TL;DR: In this paper, the XMM-Newton follow-up for confirmation of Planck cluster candidates is presented, where a total of 21 candidates are confirmed as extended X-ray sources.
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Planck intermediate results. XVII. Emission of dust in the diffuse interstellar medium from the far-infrared to microwave frequencies

A. Abergel, +197 more
TL;DR: In this paper, the Parkes survey of the 21-cm line emission of neutral atomic hydrogen, over a contiguous area of 7500 deg$^2$ centred on the southern Galactic pole, was used to characterize the emission properties of dust in the diffuse interstellar medium.