Galaxy cluster mass bias from projected mass maps

The determination of the mass of galaxy clusters from observations is subject to systematic uncertainties. Beyond the errors due to instrumental and observational systematic effects, in this work we investigate the bias introduced by modelling assumptions. In particular, we consider the reconstructi...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2024-02, Vol.682
Hauptverfasser:	Muñoz-Echeverría, M, Macías-Pérez, J F, Artis, E, Cui, W, de Andres, D, De Luca, F, De Petris, M, Ferragamo, A, Giocoli, C, Hanser, C, Mayet, F, Meneghetti, M, Moyer-Anin, A, Paliwal, A, Perotto, L, Rasia, E, Yepes, G
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Bias Estimates Galactic clusters Red shift Uncertainty
Online-Zugang:	Volltext
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