activity
20022018
most citedA Weak Lensing Study of X-ray Groups in the COSMOS survey: Form and Evolution of the Mass-Luminosity Relation

291 citations · 1.7k across the 26 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.CO2016★ 70 cited

SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV

Nicolas Clerc, Andrea Merloni, Yu-Ying Zhang +17

SPIDERS (The SPectroscopic IDentification of eROSITA Sources) is a program dedicated to the homogeneous and complete spectroscopic follow-up of X-ray AGN and galaxy clusters over a…

astro-ph.CO2016★ 5 cited

Probing the dynamical and X-ray mass proxies of the cluster of galaxies Abell S1101

Andreas Rabitz, Yu-Ying Zhang, Axel Schwope +3

Context: The galaxy cluster Abell S1101 (S1101 hereafter) deviates significantly from the X-ray luminosity versus velocity dispersion relation (L-sigma) of galaxy clusters in our p…

astro-ph.CO2016★ 21 cited

HIFLUGCS: X-ray luminosity -- dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys

Yu-Ying Zhang, Thomas H. Reiprich, Peter Schneider +7

We present the X-ray luminosity (L) versus dynamical mass (M) relation for 63 nearby clusters in the HIFLUGCS. The luminosity measurements are obtained based on ~1.3 Ms of clean XM…

astro-ph.GA2016★ 68 cited

Origin of central abundances in the hot intra-cluster medium - II. Chemical enrichment and supernova yield models

François Mernier, Jelle de Plaa, Ciro Pinto +7

The hot intra-cluster medium (ICM) is rich in metals, which are synthesised by supernovae (SNe) and accumulate over time into the deep gravitational potential well of clusters of g…

astro-ph.HE2016★ 29 cited

Insights into the location and dynamics of the coolest X-ray emitting gas in clusters of galaxies

Ciro Pinto, Andrew C. Fabian, Anna Ogorzalek +10

We extend our previous study of the cool gas responsible for the emission of OVII X-ray lines in the cores of clusters and groups of galaxies. This is the coolest X-ray emitting ph…

astro-ph.GA2016★ 67 cited

Origin of central abundances in the hot intra-cluster medium - I. Individual and average abundance ratios from XMM-Newton EPIC

François Mernier, Jelle de Plaa, Ciro Pinto +5

The hot intra-cluster medium (ICM) is rich in metals, which are synthesized by supernovae (SNe) explosions and accumulate over time into the deep gravitational potential well of cl…