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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.

Papers
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Planck intermediate results: XV: A study of anomalous microwave emission in Galactic clouds

Peter A. R. Ade, +183 more
- 01 May 2014 - 
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 1 ◦ -smoothed maps from 0.408 GHz up to 3000 GHz.
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Planck 2015 results. VI. LFI mapmaking

Peter A. R. Ade, +199 more
- 05 Feb 2015 - 
TL;DR: In this paper, a map-making procedure for Planck LFI (low frequency instrument) data is described, where the main products are sky maps of $I,Q, and $U$ Stokes components.
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Planck 2015 results - VI. LFI mapmaking

Peter A. R. Ade, +258 more
- 01 Oct 2016 - 
TL;DR: This paper describes the mapmaking procedure applied to Planck Low Frequency Instrument (LFI) data, based on a destriping technique, which is enhanced with a noise prior, and presents polarization maps at LFI frequencies for the first time.
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Planck early results. XXVI. Detection with Planck and confirmation by XMM-Newton of PLCK G266.6–27.3, an exceptionally X-ray luminous and massive galaxy cluster at z ~ 1

Nabila Aghanim, +234 more
- 01 Dec 2011 - 
TL;DR: The first results on PLCK G266.3, a galaxy cluster candidate detected at a signal-to-noise ratio of 5 in the Planck All Sky survey, were presented in this article.
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The X-ray surface brightness profiles of hot galaxy clusters up to $\vec z$ ~ 0.8: Evidence for self-similarity and constraints on $\Omega_\mathsf{0}$

M. Arnaud, +2 more
- 01 Jul 2002 - 
TL;DR: In this paper, the authors used the surface brightness profiles of a sample of 25 distant $(0.3 3.5~\rm keV) clusters, observed with ROSAT, with published temperatures from ASCA.