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researcher

N. Aghanim

369 papers hereh-index 8652.1k citations555 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author12
  • middle author125
  • last author30

Across the 167 of 369 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO218
  • astro-ph.GA83
  • astro-ph35
  • astro-ph.IM24
  • astro-ph.SR3
  • astro-ph.EP2
same name
  • N. Aghanim — 25 papers
  • N. Aghanim — 22 papers, h 3
  • N. Aghanim — 5 papers, h 7
  • N. Aghanim — 2 papers, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 45.9k across the 359 of their papers we have counts for

collaborators
Showing 2002Show all

4 papers · 1 filter

astro-ph2002★ 37 cited

Cosmological Magnetogenesis driven by Radiation Pressure

Mathieu Langer, Jean-Loup Puget, Nabila Aghanim

The origin of large scale cosmological magnetic fields remains a mystery, despite the continuous efforts devoted to that problem. We present a new model of magnetic field generatio…

astro-ph2002★ 15 cited

Extraction of cluster parameters with future Sunyaev-Zel'dovich observations

Nabila Aghanim, Steen H. Hansen, Sergio Pastor +1

The Sunyaev-Zel'dovich (SZ) effect of galaxy clusters is characterized by three parameters: Compton parameter, electron temperature and cluster peculiar velocity. In the present st…

astro-ph2002★ 107 cited

XMM-Newton observation of the distant (z=0.6) galaxy cluster RX J1120.1+4318

M. Arnaud, S. Majerowicz, D. Lumb +12

We report on a 20 ksec XMM observation of the distant cluster RXJ1120.1+4318, discovered at z=0.6 in the SHARC survey. The cluster has a regular spherical morphology, suggesting it…

astro-ph2002★ 11 cited

Cosmic Microwave Background anisotropies beyond the third peak

N. Aghanim, P. G. Castro, A. Melchiorri +1

Forthcoming CMB experiments will allow us to accurately investigate the power spectrum at very small scales (ℓ>1000). We predict the level of the primary anisotropies, given…

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