Paul Giles
5 ta ish
School of Physics, HH Wills Physics Laboratory, Tyndall Avenue, Bristol, BS8 1TL, UK
The <i>XMM</i> Cluster Survey: automating the estimation of hydrostatic mass for large samples of galaxy clusters – I. Methodology, validation, and application to the SDSSRM-XCS sample
D J Turner, Paul Giles, A. K. Romer +16
MaqolaGalaxies: Formation, Evolution, PhenomenaMonthly Notices of the Royal Astronomical Society20250 iqtibosABI