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20172026
most citedVariegate galaxy cluster gas content: Mean fraction, scatter, selection effects and covariance with X-ray luminosity

31 citations · 37 across the 5 of their papers we have counts for

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5 papers · 1 filter

astro-ph.CO2026

Testing X-ray selection effects with four rich, yet X--ray--faint, galaxy clusters

S. Andreon, A. Moretti

A robust understanding of selection effects in galaxy cluster studies is crucial for both astrophysical and cosmological applications. Examining clusters identified through differe…

astro-ph.CO2025★ 2 cited

The uncommon intracluster medium features of the first massive clusters selected independently of their baryon content

S. Andreon, M. Radovich, A. Moretti +6

Our current knowledge of the thermodynamic properties of galaxy clusters comes primarily from detailed studies of clusters selected by their minority components: hot baryons. Most…

astro-ph.CO2024

Observed abundance of X-ray low surface brightness clusters in optical, X-ray, and SZ selected samples

S. Andreon, G. Trinchieri, A. Moretti

The comparison of the properties of galaxy cluster samples selected using observations in different wavebands may shed light on potential biases of the way in which the samples are…

astro-ph.CO2019★ 4 cited

Why are some galaxy clusters underluminous? The very low concentration of the CL2015 mass profile

S. Andreon, A. Moretti, G. Trinchieri +1

Our knowledge of the variety of galaxy clusters has been increasing in the last few years thanks to our progress in understanding the severity of selection effects on samples. To u…

astro-ph.CO2017★ 31 cited

Variegate galaxy cluster gas content: Mean fraction, scatter, selection effects and covariance with X-ray luminosity

S. Andreon, J. Wang, G. Trinchieri +2

We use a cluster sample selected independently of the intracluster medium content with reliable masses to measure the mean gas mass fraction and its scatter, the biases of the X-ra…