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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. V. LFI calibration

Peter A. R. Ade, +270 more
TL;DR: In this article, the authors present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the planck 2015 data release, covering four years of uninterrupted operations.
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A Mosaic of the Coma Cluster of Galaxies with XMM-Newton

TL;DR: The Coma cluster of galaxies was observed with XMM-Newton in 12 partially overlapping pointings as mentioned in this paper, and the resulting X-ray map in different energy bands and discuss the large scale structure of this cluster.
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Planck intermediate results. XLIX. Parity-violation constraints from polarization data

Nabila Aghanim, +149 more
TL;DR: In this paper, the authors present new constraints on an isotropic rotation, parametrized by the angle π, derived from Planck 2015 CMB polarization data, and employ two complementary approaches, in harmonic space and in map space, the latter based on a peak stacking technique.
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Planck 2015 results. V. LFI calibration

Peter A. R. Ade, +207 more
TL;DR: In this paper, the authors present a description of the pipeline used to calibrate the Planck Low Frequency Instrument (LFI) timelines into thermodynamic temperatures for the planck 2015 data release, covering four years of uninterrupted operations.
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Planck intermediate results XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIRE

Nabila Aghanim, +212 more
TL;DR: In this article, the authors used the Planck all-sky submillimetre and millimetre maps to search for rare sources distinguished by extreme brightness, a few hundred millijanskies, and their potential for being situated at high redshift.