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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 intermediate results. XXI. Comparison of polarized thermal emission from Galactic dust at 353GHz with optical interstellar polarization

P. A. R. Ade, +153 more
TL;DR: In this article, the authors used ancillary catalogues of interstellar polarization and extinction of starlight to obtain the degree of polarization, pV, and optical depth in the V band to the star, V.
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Planck intermediate results - XV. A study of anomalous microwave emission in Galactic clouds (Corrigendum)

Peter A. R. Ade, +234 more
TL;DR: For example, the Engineering and Technology Facilities Council (ETFCC) as mentioned in this paper proposed a new architecture for the first phase of the LEACH project, which is called LEACH.
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Star formation rates and stellar masses from machine learning

TL;DR: In this article, the authors proposed a method based on the machine learning algorithm Random Forest to estimate the star formation rate (SFR) and the stellar mass (Mstar) of galaxies at redshifts in the range 0.1
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Gas distribution from clusters to filaments in IllustrisTNG

TL;DR: In this paper , the radial and azimuthal distribution of gas is investigated in galaxy clusters and how it can be related to cluster-mass assembly history and its evolutionary state.
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Relative distribution of dark matter, gas and stars around cosmic filaments in the IllustrisTNG simulation

TL;DR: In this article, the authors present a comprehensive study of the distribution of matter around different populations of filaments, using the IllustrisTNG simulation at z = 0.68 and find that baryons exactly follow the underlying DM distribution up to r~7 Mpc to the filament spines.