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J. Nevalainen

55 papers hereh-index 252.4k citations103 works total

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

author position
  • sole author1
  • first author10
  • middle author28
  • last author8

Across the 47 of 55 papers where every author was matched, so the position is known.

fields
  • astro-ph23
  • astro-ph.CO17
  • astro-ph.HE7
  • astro-ph.IM6
  • astro-ph.GA2
same name
  • J. Nevalainen — 4 papers, h 30
  • J. Nevalainen — 2 papers
  • J. Nevalainen — 2 papers, h 3
  • J. Nevalainen — 1 paper, h 5
  • J. Nevalainen — 1 paper, h 4
  • J. Nevalainen — 1 paper, 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
19972023
most citedThe Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

395 citations · 2k across the 54 of their papers we have counts for

collaborators
Showing 2005Show all

3 papers · 1 filter

astro-ph2005★ 20 cited

Thermal and non-thermal nature of the soft excess emission from Sersic 159-03 observed with XMM-Newton

M. Bonamente, R. Lieu, J. P. D. Mittaz +2

Several nearby clusters exhibit an excess of soft X-ray radiation which cannot be attributed to the hot virialized intra-cluster medium. There is no consensus to date on the origin…

astro-ph2005★ 82 cited

XMM-Newton EPIC background modeling for extended sources

J. Nevalainen, M. Markevitch, D. Lumb

We use XMM-Newton blank-sky and closed-cover background data to explore the background subtraction methods for large extended sources filling the EPIC field of view, such as nearby…

astro-ph2005

XMM−Newton Ω project: III. Gas mass fraction shape in high redshift clusters

Rachida Sadat, Alain Blanchard, Sebastien C. Vauclair +10

We study the gas mass fraction, f_gas, behavior in XMM−Newton Ω project. The typical f_gas shape of high redshift galaxy clusters follows the global shape inf…

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