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Monique Arnaud

Researcher at Paris Diderot University

Publications -  263
Citations -  87950

Monique Arnaud is an academic researcher from Paris Diderot University. The author has contributed to research in topics: Galaxy cluster & Planck. The author has an hindex of 109, co-authored 257 publications receiving 83329 citations. Previous affiliations of Monique Arnaud include Université Paris-Saclay & University of Paris.

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Planck intermediate results. XXVI. Optical identification and redshifts of Planck clusters with the RTT150 telescope

Peter A. R. Ade, +195 more
TL;DR: In this article, the results of approximately three years of observations of Planck Sunyaev-Zeldovich (SZ) sources with the Russian-Turkish 1.5m telescope (RTT150) are presented.
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X-Ray morphological analysis of the Planck ESZ clusters

TL;DR: In this article, the authors determined eight morphological parameters for the Planck Early Sunyaev-Zeldovich (ESZ) objects observed with XMM-Newton and found that two parameters, concentration and centroid-shift, are the best to distinguish between relaxed and disturbed systems.
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Weak Gravitational Lensing and X-Ray Analysis of Abell 2163

TL;DR: In this article, the authors reported on the detection of dark matter in the cluster of galaxies Abell 2163 using the weak gravitational distortion of background galaxies and an analysis of the X-ray emission from the cluster.
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Planck intermediate results - XXXI. Microwave survey of Galactic supernova remnants

Monique Arnaud, +203 more
TL;DR: The all-sky Planck survey in 9 frequency bands was used to search for emission from all 274 known Galactic supernova remnants as mentioned in this paper, of which 16 were detected in at least two Planck frequencies.
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The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population

TL;DR: In this article, the authors review the state of the art in cluster mass estimation methods and the systematic uncertainties and biases inherent in each approach, and explore how current uncertainties propagate into the cosmological parameter analysis.