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researcher

M. Arnaud

209 papers hereh-index 9039k citations418 works total

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

author position
  • sole author2
  • first author4
  • middle author90
  • last author9

Across the 105 of 209 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO129
  • astro-ph34
  • astro-ph.GA33
  • astro-ph.IM10
  • astro-ph.HE3
same name
  • M. Arnaud — 30 papers, h 12
  • M. Arnaud — 14 papers
  • M. Arnaud — 12 papers, h 5
  • M. Arnaud — 6 papers, h 2
  • M. Arnaud — 5 papers, h 3
  • M. Arnaud — 5 papers

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
19952024
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations · 45.8k across the 208 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.CO2018★ 1 cited

NIKA2 Performance and Cosmology Program with Galaxy Clusters

L. Perotto, R. Adam, P. Ade +38

NIKA2 is a dual-band millimetric camera of thousands of Kinetic Inductance Detectors (KID) installed at the IRAM 30-meter telescope in the Spanish Sierra Nevada. The instrument com…

astro-ph.GA2018★ 60 cited

The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching

Remco F. J. van der Burg, Sean McGee, Herve Aussel +4

We study the abundance of star-forming and quiescent galaxies in a sample of 21 massive clusters at 0.5<z<0.7, detected with the Planck satellite. We measure the cluster galaxy ste…

astro-ph.CO2018★ 39 cited

Resolving the hydrostatic mass profiles of galaxy clusters at z~1 with XMM-Newton and Chandra

Iacopo Bartalucci, Monique Arnaud, Gabriel W. Pratt +1

We present a detailed study of the integrated total hydrostatic mass profiles of the five most massive (M500SZ​>5×1014 M⊙​) galaxy clusters sele…

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